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Fragmentation and energy dissipation in rockfall: Effects of block shape and non-collinear impact dynamics

Marchelli, Maddalena

Abstract

Understanding fragmentation and energy dissipation during rockfall events is essential for accurate hazard assessment and predictive modelling. To date, most experimental studies have used spherical specimens, primarily because of their geometric simplicity and ease of repeatable testing. This work investigates the dynamic behaviour of angular block shapes, i.e., cubes, prisms, and slabs, which more closely resemble natural rock geometries, through free-fall drop tests up to 10 m/s, complemented by static splitting tests to explore potential links with dynamic response. These geometries often result in non-collinear impacts with multiple contact points and prolonged impact durations, significantly influencing the likelihood of fragmentation and post-impact dynamics. The study examines how block geometry, impact orientation and location (face, edge, vertex) affect failure patterns and energy restitution. Results show that fragmentation probability strongly depends on geometry: slabs fragmented in 33% of tests, prisms in 50%, while cubes only at the highest velocity. Static tests revealed geometry- and loading condition- dependent tensile strength, with prisms showing the highest median value (2.3 MPa) and slabs the lowest (1.1 MPa). Fragmentation severity also varied, with slabs producing finer fragments compared to prisms. For intact specimens, apparent restitution coefficients ranged from 0.13 (prisms) to 0.39 (cubes), significantly lower than spheres (0.34), and impact durations were up to two orders of magnitude longer than for spherical blocks. The results highlight the complex interplay between block geometry, impact conditions, and energy dissipation, providing shape-dependent metrics for improving rockfall trajectory models.

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Contents lists available at ScienceDirect International Journal of Rock Mechanics and Mining Sciences journal homepage: www.elsevier.com/locate/ijrmms Research paper Fragmentation and energy dissipation in rockfall: Effects of block shape and non-collinear impact dynamics Maddalena Marchelli a,∗, Davide Ettore Guccione b, Anna Giacomini b, Olivier Buzzi b aDepartment of Environment, Land and Infrastructure Engineering (DIATI)- Politecnico di Torino, C.so Duca degli Abruzzi 24, I–10129 Torino, Italy bCentre for Geotechnical Science and Engineering, College of Engineering, Science and Environment, University of Newcastle, University Dr, 2308 Callaghan, NSW, Australia A R T I C L E I N F O Keywords: Non-collinear impact Fragmentation in rockfall Restitution coefficient Trajectories Block shapes A B S T R A C T Understanding fragmentation and energy dissipation during rockfall events is essential for accurate hazard assessment and predictive modelling. To date, most experimental studies have used spherical specimens, primarily because of their geometric simplicity and ease of repeatable testing. This work investigates the dynamic behaviour of angular block shapes, i.e., cubes, prisms, and slabs, which more closely resemble natural rock geometries, through free-fall drop tests up to 10 m/s, complemented by static splitting tests to explore potential links with dynamic response. These geometries often result in non-collinear impacts with multiple contact points and prolonged impact durations, significantly influencing the likelihood of fragmentation and post-impact dynamics. The study examines how block geometry, impact orientation and location (face, edge, vertex) affect failure patterns and energy restitution. Results show that fragmentation probability strongly depends on geometry: slabs fragmented in 33% of tests, prisms in 50%, while cubes only at the highest velocity. Static tests revealed geometryand loading conditiondependent tensile strength, with prisms showing the highest median value (≈ 2.3MPa) and slabs the lowest (≈ 1.1MPa). Fragmentation severity also varied, with slabs producing finer fragments compared to prisms. For intact specimens, apparent restitution coefficients ranged from 0.13 (prisms) to 0.39 (cubes), significantly lower than spheres (≈ 0.34), and impact durations were up to two orders of magnitude longer than for spherical blocks. The results highlight the complex interplay between block geometry, impact conditions, and energy dissipation, providing shape-dependent metrics for improving rockfall trajectory models. 1. Introduction Rockfall is a high-energy, gravity-driven process involving the detachment, free fall, and successive impacts of rock blocks along steep natural or engineered slopes. These events pose significant hazards to infrastructure, transportation corridors, and human life in mountainous regions.1,2 The kinematic behaviour of falling blocks, including translational and rotational motion, fragmentation, impact-induced energy dissipation, and rebound trajectories, critically influences subsequent propagation, runout distances, and impact forces.3–5 Accurate prediction of rockfall behaviour requires a detailed understanding of both the mechanical response of blocks upon impact and the energy transfer mechanisms that govern fragmentation and post-impact motion.6 While substantial progress has been made in modelling rockfall kinematics, understanding of fragmentation mechanisms and post-impact dynamics remains limited, particularly for blocks with realistic geometries.7,8 Dynamic impact tests, particularly free-fall and parabolic drop tests, have been widely employed to simulate rockfall events and ∗Corresponding author. E-mail address: [email protected] (M. Marchelli). investigate fragmentation thresholds, energy dissipation, and rebound behaviour.9–18 A key parameter in such studies is the coefficient of restitution (CoR), defined as the ratio of rebound velocity to impact velocity, which quantifies the energy retained after impact. The CoR is now routinely incorporated into rockfall trajectory models to estimate post-impact velocities and angles.19–21 While laboratory experiments provide controlled conditions for isolating specific variables, most experimental and related numerical investigations have predominantly focused on spherical specimens.22,23 which offer geometric simplicity and predictable contact behaviour. Spheres tend to generate collinear impacts with well-defined stress distributions, which makes them ideal for repeatable studies but less representative of the irregular and angular blocks typically involved in natural rockfall events.24 Some laboratory studies have explored the influence of block shape,10,25 but they have primarily focused on its effect on the coefficient of restitution, without addressing other critical aspects such as contact duration, detailed post-impact motion, and fragmentation behaviour. Several https://doi.org/10.1016/j.ijrmms.2025.106381 Received 12 September 2025; Received in revised form 14 November 2025; Accepted 7 December 2025 International Journal of Rock Mechanics & Mining Sciences 198 (2026) 106381 Available online 11 December 2025 1365-1609/© 2025 The Authors. Published by Elsevier Ltd. This is an open access article under the CC BY license ( http://creativecommons.org/licenses/by/4.0/ ). M. Marchelli et al. numerical studies have similarly focused on kinematic aspects without incorporating fragmentation. For instance, Krengel et al.26 used 2D discrete element method (DEM) simulations to show that block shape and initial orientation significantly influence runout and restitution coefficients, with outcomes highly sensitive to even minor variations in geometry or launch conditions. Similarly, Dattola et al.27 proposed a rheological model for ellipsoidal block impacts that accounts for eccentricity, rotation, and impact angle, offering a refined approach to restitution analysis by considering non-point-like contacts; however, their work did not address fragmentation. In contrast, other studies have explicitly examined fragmentation, focusing on fracture outcomes and energy dissipation. In detail, investigations on concrete armour units and engineered blocks28,29 have demonstrated that block geometry and impact configuration strongly affect breakage. Das et al.30 explored how block shape influences fracture patterns and energy dissipation during impact, while Ye et al.31 employed DEM simulations to assess the effects of elongation and flatness ratios on dynamic breakage, including rebound and post-impact motion. Nevertheless, these simulations commonly assume planar, horizontal contacts and do not account for inclined impacts or multiple simultaneous contact points, thereby limiting the realism of contact dynamics in rockfall scenarios. Only a limited number of in situ tests have been conducted to capture the complexity of real-scale rockfall dynamics, including irregular terrain, natural block geometries, and heterogeneous surface conditions,32–34 but their interpretability is often constrained by the variability in block shape and impact conditions, which introduces significant scatter in motion parameters. Recent advances in experimental techniques, including high-speed imaging, multi-view photogrammetry, and 3D scanning technologies, have enabled more detailed investigations of fragmentation processes and post-impact motion.35–37 Although some rockfall trajectory models now incorporate shapedependent rolling and bouncing behaviour,38–40 they rarely account for fragmentation or non-collinear impact effects, limiting their predictive accuracy. Fragmentation is often treated as a binary outcome or modelled using empirical rules, without addressing the underlying mechanics of failure or the influence of block shape and contact dynamics.41,42 While a few models do include fragmentation processes,43–46 they are generally limited to spherical blocks or rely on lumped-mass representations that fail to capture the geometric complexity and contact variability inherent to angular rock blocks. Notably, Guccione et al.46 proposed a fragmentation model based on survival probability, offering a more robust criterion, though still limited to spherical blocks. This study aims to provide new insights into the fragmentation processes and energy dissipation of brittle blocks with geometries that approximate real rock shapes. To this end, the study focuses on three distinct specimen geometries, i.e., prisms, cubes, and slabs, selected to ensure repeatability and minimising geometric variability. Although the experimental setup, i.e., free fall drop tests on artificial mortar specimens, represents a simplification of natural rockfall events, it enables controlled exploration of shape-dependent failure mechanisms. The primary objective is to understand how block geometry, impact orientation and location (face, edge, vertex) influence fragmentation patterns, interaction (number, duration, and sequence of contacts), and post-impact dynamics. To complement the dynamic tests, a targeted series of static splitting tests (indirect tensile tests), encompassing both conventional and non-standard configurations, was conducted to characterise quasi-static fracture behaviour. These tests, under controlled conditions, aim to identify geometry-driven stress concentrations and fracture modes that may affect fragmentation occurrence and rebound behaviour in the free-fall cases. Although numerical modelling is essential for predictive purposes, this study focuses specifically on controlled experiments to isolate the effect of block geometry and non-collinear impacts. The resulting dataset provides a benchmark for future numerical validation. 2. Methodology 2.1. Experimental setup 2.1.1. Dynamic tests: free-fall drop tests A series of vertical free-fall drop tests was carried out using the fragmentation facility developed at the University of Newcastle47 (Fig. 1.a). The enclosed hexagonal chamber is equipped with a fibre-reinforced concrete slab, a vacuum-based release mechanism, and a high-speed imaging system comprising six externally mounted cameras, i.e., two Phantom VEO-E340L cameras and four Optronics. This configuration enables the capture of the free-fall, impact, rebound, and fragmentation phases of the specimens. Images were recorded at 500 frames per second, with exposure times of 500 μs for the Optronics and 100 μs for the Phantom cameras. Specimens were lifted using a vacuum tube and pulley system, suspended from the roof structure of the building. Specimens were positioned in the vacuum-release mechanism to achieve different impact configurations (face, edge, or vertex) and orientations relative to the slab surface, then released smoothly by disengaging the vacuum. The maximum drop height is 5.1 m, which results in a maximum impact velocity of about 10 m/s. After each test, all the samples, or all fragments in case of fragmentation, were recorded, collected and weighted. 2.1.2. Static test: diagonal splitting and vertex-to vertex loading tests During the static testing campaign, displacement-controlled compression tests were conducted using a servo-hydraulic MTS Criterion testing machine (maximum load capacity: 300 kN) with a spherical seat, operated at a constant rate of 5 mm/min (Fig. 1.b). Force– displacement data were recorded for each test. A high-resolution video camera Nikon D800e (frame rate: 30 fps, resolution: 1.920 × 1.080 pixel) was positioned laterally to capture the evolution of fracture patterns and crack propagation in real time. Two distinct loading configurations were adopted to investigate the fracture behaviour of geometrically diverse specimens (prisms, slabs, and cubes). The first involved diagonal splitting tests, in which compressive loads were applied along opposing edges to induce tensile failure along oblique planes. This configuration deviates from conventional Brazilian-type tests48 or standard splitting tensile strength methods,48–52 which typically apply diametral compression to cylindrical specimens or concentrated loading along a narrow strip on the lateral face of prismatic or cubic specimens. Although less commonly used, diagonal configurations have previously been explored in the literature for cubic specimens,53–57 demonstrating its relevance for assessing tensile failure under complex loading paths. The second configuration consisted of vertex-to-vertex loading, where compressive forces were applied at opposing corners of the specimens. This setup mimics the point load test used in rock mechanics,58,59 generating highly localised stress concentrations at the vertices. The rationale for employing these two complementary configurations lies in their ability to probe different aspects of the material’s mechanical response under quasi-static conditions. The diagonal splitting tests were designed to promote oblique fracture planes and induce non-uniform tensile stress fields, enabling a comparative assessment of failure mechanisms across different shapes. In contrast, the vertex-tovertex tests focused on stress localisation and vertex fragility, capturing the onset of fracture under extreme boundary conditions. Together, these configurations provide insight into geometry-driven stress redistribution and crack initiation. It is important to note that these static tests were meant to serve as a preliminary investigation into the fracture behaviour of the material. While limited in scope, they provide a foundational understanding of failure mechanisms and stress localisation effects, which can meaningfully inform the interpretation of more complex dynamic impact responses examined in subsequent phases of the study. International Journal of Rock Mechanics and Mining Sciences 198 (2026) 106381 2 M. Marchelli et al. Fig. 1. Experimental setup comprising: the fragmentation cell (a) and the servo-hydraulic MTS testing machine (b). 2.2. Data analysis 2.2.1. Impact data from image analysis All high-speed image sequences were analysed using TEMA3Ds software60 to extract key impact parameters, following the calibration procedure described in Guccione et al.47 For each test, the impact location was classified as occurring on a face, edge, or vertex, while the impact orientation was defined by the three angles 𝜃 formed between the three orthogonal faces of the specimen converging at the impact point (𝐴) and the impacted surface. In cases where the contact occurs on an edge or a face, 𝐴 is defined as the midpoint of the respective edge or face. Fig. 2 presents a schematic of a generic specimen impacting the target surface. The three planes defined by the vertices 𝐴-𝐵-𝐶, 𝐴-𝐵-𝐷, and 𝐴-𝐶-𝐷 represent the three orthogonal faces from which the angles with the impacted surface, namely 𝜃𝐴𝐵𝐶−𝑧, 𝜃𝐴𝐵𝐷−𝑧, and 𝜃𝐴𝐶𝐷−𝑧, are computed. Some conventions were adopted: for prismatic specimens, the edge 𝐴–𝐷 corresponds to the longest edge, whereas for slab-like specimens, 𝐴–𝐵 represents the shortest edge (Fig. 3). Fragmentation was systematically assessed for each test. The presence, extent (number of fragments), and type of fragmentation, ranging from minor chipping to complete breakage, were identified through frame-by-frame analysis of high-speed footage and post-impact specimen inspection. The nature of the specimen/impacted surface interaction was further analysed in terms of impact duration, number and sequence of contact points (or edges or surfaces) occurring during the first impact event. In the case of collinear impacts, typically observed in spherical specimens, the contact with the ground surface is point-like, involving a single contact point and a brief interaction before rebound, sliding, or rest. In contrast, specimens with angular or elongated geometries often exhibit complex interaction during the initial impact, involving multiple sequential contacts on vertices, edges, and faces. These multicontact configurations extend the duration of the impact and reflect the body’s search for a stable post-impact configuration. To quantify this, we defined the impact duration 𝑡𝐼 as the time interval during which the centre of gravity remained at or below its position from the preceding instant, without sliding or coming to rest. This ensures that only the active contact phase is considered, ending when the centre of gravity begins to rise. All contact events occurring within this interval were considered part of a single impact and the moment the centre of gravity begins to rise marks the onset of rebound and the end of the impact phase. For each test, the number of distinct contact events prior to Fig. 2. Sketch of the local reference system. A generic specimen impacting the target surface is shown. SV = side view; PV = plan view; LV = lateral view. Point A indicates the impact location, while CoG denotes the centre of gravity. The global and local reference systems are represented by 𝑥–𝑦–𝑧 and 𝜉–𝜂–𝑧, respectively. International Journal of Rock Mechanics and Mining Sciences 198 (2026) 106381 3 M. Marchelli et al. Fig. 3. Sketch of the 𝐴-𝐵-𝐶, 𝐴-𝐵-𝐷, and 𝐴-𝐶-𝐷 planes for prism and slab-like specimens. Point 𝐴 indicates the impact point. rebound, sliding, or rest was manually counted through frame-by-frame image analysis, allowing an estimate of the total impact duration 𝑡𝐼 (Fig. 4). This metric is particularly relevant for propagation modelling, where impact duration influences energy dissipation and post-impact motion. Sample motion was analysed using TEMA3Ds software.60 The software employs an outline tracking algorithm to reconstruct 3D trajectories from multi-view silhouettes. The rebound and post-impact trajectories of non-fragmented samples were tracked to evaluate the coefficient of restitution and investigate the influence of sample shape on energy dissipation and motion. Fragment tracking was not performed at this stage, as the current study focuses on the dynamics of intact specimens. Due to the complexity of fragment motion, characterised by irregular geometries, rapid rotations, and frequent visual obstructions, quantitative tracking of individual fragments is deferred to a subsequent phase of the research. At this stage, fragmentation was assessed qualitatively through visual inspection of the high-speed footage. Tracked tests were post-processed in MATLAB61 to examine the trajectories and analyse the influence of block shape, impact orientation and location on post-impact dynamics. The global reference system (O𝑥𝑦𝑧) used to track the specimens was centred at the middle of the impact plane, with the 𝑥–𝑦 axes lying on the target surface and the 𝑧 axis oriented normal to it along the trajectory of the centre of gravity of the falling mass. To enable consistent comparison across tests, a local reference system (O𝜉𝜂𝑧) was defined for each specimen, centred at the projection of its centre of gravity (CoG) onto the impact plane. The vector  𝑟, connecting the impact point 𝐴 to the specimen’s centre of gravity (CoG), was used to define the orientation of the local reference system. Specifically, the direction of the 𝜉-axis was defined in such a way that the corresponding unit vector  𝑖𝜉 is oriented along the projection of  𝑟 onto the global 𝑥–𝑦 plane. The 𝜂-axis, orthogonal to 𝜉, lies within the 𝑥–𝑦 plane and is defined as positive in the anti-clockwise direction from 𝜉. The 𝑧-axis remains aligned in both the global and local reference systems. The angle 𝜙, which determines the rotation between global and local reference systems, is defined as the positive anti-clockwise angle between the unit vectors  𝑖𝑥 and  𝑖𝜉, and is computed as:  𝑖𝜉⋅ 𝑖𝑥= cos 𝜙. (1) The impact eccentricity 𝑑 is defined as the length of the projection of  𝑟 onto  𝑖𝜉, i.e., the distance between the impact point 𝐴 and the projection of the CoG onto the impact plane, measured along the 𝜉-axis: 𝑑= 𝑟⋅ 𝑖𝜉.(2) Accordingly, the post-impact velocity components transform as follows: 𝑣𝑥= cos 𝜙𝑣𝜉− sin 𝜙𝑣𝜂(3) 𝑣𝑦= sin 𝜙𝑣𝜉+ cos 𝜙𝑣𝜂,(4) while 𝑣𝑧 remains unchanged. The choice of this local reference system lies in the mechanics of the initial interaction between the block and the impacted surface. Upon contact, an upward reaction force is generated at the impact point. Since this force is not collinear with the inertial force acting through the centre of gravity (CoG) of the falling body, a moment is induced. This moment initiates the first rotational motion of the specimen during the impact phase. The moment vector is oriented normal to the plane defined by the vector  𝑟, connecting the impact point to the CoG, and the global vertical axis (𝑧-axis). To analyse the rebound direction, two angles were defined in the local reference system (O𝜉𝜂𝑧). The planar angle 𝛽 is measured clockwise between the 𝜂-axis and the post-impact velocity vector projected onto the 𝜉–𝜂 plane. This angle captures the directionality of rebound motion relative to the specimen’s geometry. Trajectories aligned with the positive 𝜉-axis correspond to 𝛽≈ 90◦, indicating motion predominantly along the line connecting the impact point to the CoG. Additionally, the vertical projection angle 𝛼 is defined between the vertical velocity component (𝑣𝑧) and the horizontal velocity magnitude in the 𝜉–𝜂 plane, computed as √𝑣2 𝜉+𝑣2 𝜂. This angle quantifies the proportion of vertical motion relative to horizontal motion, providing insight into energy dissipation and rebound potential. Both angles are illustrated in Fig. 5. Whereas traditional trajectory models typically treat the block as a material point and rely solely on restitution coefficients to encapsulate impact behaviour, our approach acknowledges that these coefficients implicitly include effects such as rotational exchange, and multiple contacts, consistent with the extended modelling frameworks proposed by Vijayakumar et al.62 and Dattola et al.27 Accordingly, we computed an apparent restitution coefficient, evaluated with reference to the CoG, as the ratio between is the translational velocity at the end of the impact 𝑣𝑒 and the incident impact velocity 𝑣𝑖. Rotational motion was not quantitatively analysed in this phase. This decision was guided by several considerations. The primary objective of the current phase was to isolate the influence of shape and contact configuration on translational energy dissipation and rebound behaviour in intact specimens. In the context of apparent restitution analysis, the rotational contribution is implicitly embedded in the postimpact translational velocity of the centre of gravity, as discussed in Dattola et al.27 This approach aligns with the assumptions commonly adopted in lumped-mass trajectory models, where the block is treated as a single mass point and rotational effects are not explicitly resolved but are instead incorporated into effective translational parameters. Therefore, while rotation undoubtedly influences energy redistribution during impact, its explicit quantification is deferred to a subsequent phase of the study, where enhanced tracking protocols and higher-resolution imaging will be employed. 2.2.2. Static test analysis High-resolution video footage was used to qualitatively classify fracture types, including single cracks, multiple branching cracks, and localised crushing at contact points, giving attention to identifying crack initiation zones and tracking propagation paths, where visible, to understand how stress redistributes across different geometries and loading configurations. Fracture patterns were correlated with specimen shape (cubes, slabs, prisms) and loading type (diagonal edgeto-edge vs. vertex-to-vertex) to explore how geometry influences failure mechanisms. For each test, the symmetry of crack propagation was qualitatively assessed based on visual inspection. Fractures were considered symmetric when crack development occurred in a mirrored fashion on either side of the loading axis. In contrast, asymmetric fractures were identified by uneven crack propagation, branching, or deviation from the expected path. Special attention was given to linking the observed static fracture features to the dynamic behaviour of the same specimen types under drop-weight impact. In particular, the presence of vertex fragility, oblique cracking, or asymmetric fracture International Journal of Rock Mechanics and Mining Sciences 198 (2026) 106381 4 M. Marchelli et al. Fig. 4. Schematic representation of impact duration 𝑡𝐼 and contacts sequence during the first impact event. The interval 𝑡1 to 𝑡3 defines the active contact phase, during which the specimen’s CoG remains at or below its position from the preceding instant. After 𝑡3, the CoG begins to rise, marking the end of the impact and the onset of rebound. All contact events occurring within this interval are considered part of a single impact. Fig. 5. Sketch of a post-impact specimen with its velocity vector, highlighting the angles 𝛼 (front view, top part of the figure) and 𝛽 (plane view, bottom part of the figure). For simplicity, no rotation of the specimen and a unique contact is considered during the impact time 𝑡𝐼. SV = side view; PV = plan view. in static tests was evaluated as potential indicators of fragmentation propensity in dynamic conditions. Force–displacement curves obtained from the MTS machine were analysed to extract key mechanical indicators. While the initial slope of the curve can provide insight into the elastic stiffness of the specimen, the post-peak behaviour can allow to distinguish between brittle failure (sharp load drop) and more gradual softening, possible indicators of progressive damage or frictional effects along the fracture plane. The peak load 𝐹𝑝 was identified as a measure of tensile strength or vertex resistance, depending on the loading configuration. To enable comparison across specimens of different sizes and shapes, for edge-to-edge configurations, an equivalent splitting tensile strength was computed by dividing the peak force 𝐹𝑝 by the area associated with the fracture plane 𝐴𝑝: 𝜎𝑡∝𝐹𝑝 𝐴𝑝 .(5) Similarly, for vertex-to-vertex tests the tensile strength was estimated following the approach proposed by Hiramatsu and Oka,63 who demonstrated that the tensile strength of rock can be approximated by: 𝜎𝑡= 0.9𝐹𝑝 𝐷2,(6) where 𝐷 is the distance between the loading points. Although this method does not produce a uniform stress field and is influenced by the material properties and geometry of the specimen, it provides a reasonable estimate of tensile strength under concentrated loading conditions. To account for geometric influences, Broch and Franklin64 introduced a shape-dependent correction factor, applied multiplicatively to the vertex-to-vertex tensile strength formulation of Eq. (6), to account for geometric influences, typically ranging from 0.5 to 1.0 depending on the specimen’s shape and dimensions. Given this variability, comparisons of tensile strength across different geometries (e.g., prisms, slabs, cubes) require careful consideration. Accordingly, the possibility of identifying a consistent conversion factor across specimen shapes was thus examined to support more robust interpretation of geometry-dependent fracture behaviour. 3. Material and experimental program 3.1. Material and specimen preparation To ensure consistency and minimise the variability associated with natural rock materials, all specimens were cast from a mortar composed of silica sand, Portland cement, hydrated lime, and water, mixed in a mass ratio of 3:1:0.125:1. A cement accelerant (2% by weight of cement) was added to accelerate the curing process. Once cured, the mortar exhibited a density of approximately 2000 kg/m3. This mixture was selected to replicate the material used in previous studies involving spherical specimens, thereby enabling direct comparison of fragmentation probability and energy dissipation characteristics across different geometries.15,16 Guccione et al.15 also tested different mortar compositions and observed that, while fragmentation probability varies with tensile strength, the general trends in fragmentation mechanisms and rebound behaviour remain consistent across mixtures. This suggests that block geometry effects on fragmentation and rebound can be considered independent of mortar composition, and it is reasonable to assume that similar trends will hold across different brittle materials. The specimens were cast using custom-made PVC and wooden moulds (Fig. 6.a). After casting, the samples underwent a two-stage curing process: they were first cured for 14 days in a 100% humid environment, followed by 21 days of drying in a ventilated oven at 40 ◦C. Both the vertical drop tests and the static loading tests were performed immediately after the curing period to ensure consistent material conditions. Because the specimens were produced in different batches, a comprehensive material characterisation campaign was carried out for each batch. This included Brazilian tensile strength (BT) tests,48 unconfined compressive strength (UCS) tests,65 and fracture toughness tests.66 In International Journal of Rock Mechanics and Mining Sciences 198 (2026) 106381 5 M. Marchelli et al. Fig. 6. (a) Custom-made PVC and timber moulds. (b) Classification of the prism, slab, and cube specimens used in this study, plotted on the particle form chart proposed by Angelidakis et al.67: solid lines denote the boundaries between bladed, elongated, compact, and flat particles according to Angelidakis et al. while dashed lines represent the Zingg classification system,68 from which Angelidakis adapted the chart. Specimen dimensions follow the convention 𝑎>𝑏>𝑐, where 𝑎, 𝑏, and 𝑐 denote the principal lengths of the specimen. (c) Schematic representation of the investigated specimen shapes (prisms, slabs, and cubes), with dimensions indicated. Table 1 Characteristics of mortar mixtures. The values are presented as averages, with standard deviations indicated. The abbreviations ‘sec’ and ‘tan’ denote secant and tangent modulus, respectively. Proportions: sand/cement/ lime/water Young modulus (tan) (MPa) Young modulus (sec) (MPa) Unconfined compressive strength 𝜎𝑐 (MPa) Tensile strength 𝜎𝑡 (MPa) Fracture toughness 𝐾𝐼𝑐 (MPa m1∕2) 3/1/0.125/1 2517 ± 369 1756 ± 253 17.40 ± 1.49 2.05 ± 0.34 0.3758 ± 0.070 total, 35 BT, 36 UCS, and 31 toughness tests were performed. The average values and standard deviations of the measured mechanical properties are reported in Table 1. 3.2. Experimental program Three regular shapes, i.e., prisms, slabs, and cubes were selected to simulate angular rock blocks without internal discontinuities. All specimens have a volume of approximately 500 cm3, enabling direct comparison across geometries and with previous studies on spherical specimens.15,16 In particular, the reference sphere used in earlier work had a volume of 523 cm3, i.e., a diameter of 10 cm, while the prism, slab and cube used in this study had volumes of 500, 507, and 512 cm3, respectively, yielding an equivalent diameter 𝑑𝑒𝑞 of 10 cm for all shapes. This choice ensures repeatability and enables direct comparison across shapes, minimising variability and highlighting shape-dependent effects. To further reduce variability in shape parameters, the prism and slab specimens were designed with two equal sides, ensuring a consistent aspect ratio and simplifying the interpretation of shapedependent effects. The geometrical dimensions and proportions of the tested shapes are illustrated in Fig. 6.c. The figure also includes a classification of the adopted specimens on the particle form chart proposed by Angelidakis et al.,67 which provides a shape-based framework that may support the generalisation of the experimental findings to other block geometries with similar aspect ratios Fig. 6.b. 3.2.1. Dynamic tests A total of 112 drop tests were performed across the three specimen shapes. The impact velocities were controlled by varying the release height of the vacuum-based drop mechanism. Initially, a single velocity was intended for all shapes to enable direct comparison across different impact orientations and with previous results on spherical specimens. Based on the findings of Guccione et al.,15 who reported that 10 cm mortar spheres exhibit probabilities of not fragmenting equal to 100% at velocities ≤5 m/s, 50% at 6 m/s, and 0% at higher velocities, an initial velocity of 7 m/s was selected to promote fragmentation while maintaining comparability. However, during testing, it was observed that this velocity was insufficient to induce fragmentation in cubes. As a result, the velocity for cube specimens was iteratively increased to ensure the occurrence of breakage events. Ultimately, 40 tests were conducted on cubes at three different velocities: 11 at 7 m/s (corresponding to a drop height of 2.49 m), 15 at 8 m/s (3.26 m), and 14 at 10 m/s (5.10 m). For prisms and slabs, 36 tests were performed for each shape at the original velocity of 7 m/s. The number of tests per configuration was also informed by the same study, which showed that approximately 10 repetitions are sufficient for the probabilities of not fragmenting to stabilise in spheres of this size. This benchmark was used to guide the minimum number of tests required for each velocity and shape, ensuring statistical reliability while maintaining experimental feasibility. International Journal of Rock Mechanics and Mining Sciences 198 (2026) 106381 6 M. Marchelli et al. Table 2 Summary of test parameters. ‘‘Imp. loc.’’ denotes the impact location: V = vertex, E = edge (with s = short, l = long), and F = face. Prism Slab 𝑣𝑖7 m/s 7 m/s Imp. loc. V E (s) E (l) F V E (s) E (l) F n◦ (–) 31 5 – – 29 2 4 1 Tot. n◦ (–) 36 36 Cube 𝑣𝑖7 m/s 8 m/s 10 m/s Imp. loc. V E F V E F V E F n◦ (–) 7 4 – 11 4 – 10 4 – Tot. n◦ (–) 11 15 14 Impact orientation and contact location (i.e., face, edge, or vertex) were systematically varied to explore a broad range of impact scenarios. Despite efforts to randomise initial orientations, vertex impacts occurred more frequently than expected. The cause of this bias remains unclear; however it may be attributed to subtle asymmetries in specimen geometry, release alignment, or the dynamics of free fall.11,25,26,35 Table 2 reports the investigated velocities and number of samples. 3.2.2. Static tests A total of 60 static tests were conducted on mortar specimens of three geometries: cubes, prisms, and slabs. Two loading configurations were adopted: (i) edge-to-edge (diagonal splitting) and (ii) vertex-tovertex (point-load-like). For cubic specimens, 10 tests were performed for each configuration. For prisms and slabs, the edge-to-edge configuration was applied in two orientations, i.e., along the short side and along the long side, with 8 tests conducted for each orientation. Additionally, 8 vertex-to-vertex tests were performed for each of these geometries. Fig. 7 illustrates all adopted configurations. 4. Results and discussion 4.1. Fragmentation 4.1.1. Dynamic loading Drop test data were initially grouped according to the impact location: vertex, edge, or face. Three distinct outcomes were observed: (i) no fragmentation, but with localised damage at the impacted vertex, edge, or face, referred to as ‘‘chipping’’. This case is defined as the detachment of small fragments up to 0.5% of the initial mass from the impacted region, reflecting localised stress concentration and minor failure; (ii) fragmentation into two main parts, defined as ‘‘single fragmentation’’; (iii) fragmentation into multiple pieces, referred to as ‘‘multiple fragmentation’’. In both fragmentation cases, chipping was also present, indicating that localised damage precedes or accompanies full breakage. For each specimen shape and impact location, Table 3 reports the percentages of occurrence for the three outcomes. For prismatic and slab-like specimens, edge impacts are further distinguished between short and long edges to account for the elongated geometry. Across all configurations, chipping was the most prevalent outcome, particularly for cubic specimens. Fragmentation, in fact, occurred in approximately 50% of prismatic specimens and 33% of slab-like specimens, while for cubes, fragmentation was only recorded at higher velocities, with 29% of specimens fragmenting at 10 m/s, mainly under edge impact conditions. Prismatic specimens showed a more variable response. Under vertex impacts, 55% of the samples exhibited chipping, while the remaining 45% fragmented. In contrast, edge impacts (short edge only) resulted in fragmentation in 80% of the cases, indicating a lower resistance to failure along this axis. Slab-like specimens displayed similar trends under vertex impacts, as 59% of the samples chipped without fragmenting. Edge impacts, regardless of orientation, instead, Table 3 Percentage of fragmentation modes, specimen geometry (prism, slab, and cube). Fragmentation modes include chipping, single, and multiple fractures. Percentages should be considered per column, i.e., for equal impact velocity and impact location (Imp. loc.), or for equal velocity only (‘Tot.’). V = vertex, E = edge (with s = short, l = long), and F = face. Prism Slab 𝑣𝑖7 m/s 7 m/s Imp. loc. V E (s) E (l) F V E (s) E (l) F Chipping (%) 55 20 – – 59 100 100 – Single (%) 29 40 – – 8 – – – Multiple (%) 16 40 – – 33 – – 100 Tot. chip. (%) 50 66 Tot. single (%) 31 5 Tot. mult. (%) 19 28 Cube 𝑣𝑖7 m/s 8 m/s 10 m/s Imp. loc. V E F V E F V E F Chipping (%) 100 100 – 100 100 – 95 67 – Single (%) – – – – – – 5 33 – Multiple (%) – – – – – – – – – Tot. chip. (%) 100 100 71 Tot. single (%) – – 29 Tot. mult. (%) – – – resulted exclusively in chipping, suggesting that slabs are more resilient to edge impacts. These results suggest the influence of geometry and impact energy on fragmentation thresholds, indicating a higher fragmentation threshold for cubes, likely due to their symmetric geometry and uniform stress distribution. Fragmentation in prismatic specimens typically occurs at the second contact rather than the first (Fig. 8.a1, a2), within the duration of the first impact event 𝑡𝐼 as defined in Section 2.2.1 (Fig. 4). A similar behaviour is observed for slab specimens (Fig. 8.b1, b2), except in cases of face impact (Fig. 8.c) where fragmentation may initiate at the first contact. For cubic specimens, fragmentation, when it occurs, is typically aligned with the loading axis, i.e. normal to the impacted surface and intersecting the contact point, suggesting a more direct and symmetric failure mechanism (Fig. 8.d). The fracture pattern confirms the observed diagonal primary fractures and occasional secondary planes observed for rock specimens under edge impacts.30 In addition, cubes exhibited fewer fracture occurrences compared to slabs and prisms, highlighting their higher resistance to dynamic failure, which is consistent with their greater compactness as illustrated in the particle form chart (Fig. 6.b). In addition to impact location, the orientation of the specimen at impact was analysed to investigate its correlation with fragmentation occurrence and type. Ternary plots represent the angular configuration between each of the three orthogonal planes converging at the impact point, as reported in Section 2.2.1. The sum of the three angles is geometrically constrained to 180◦. Separate plots are shown for prism, slab, and cube specimens (Fig. 9). For prismatic specimens, particular attention was given to the angle 𝜃𝐴𝐵𝐶−𝑧, which corresponds to the angle between the smallest square face and the impacted surface (Fig. 3). No fragmentation was observed for 𝜃𝐴𝐵𝐶−𝑧≤40◦, indicating that when the longest face is nearly vertical, the specimen tends to resist breakage. Slab specimens exhibited an even clearer trend. When 𝜃𝐴𝐶𝐷−𝑧<45◦, i.e., the angle between the largest face and the impacted surface, multiple fragmentation was consistently observed. At 𝜃𝐴𝐶𝐷−𝑧≈ 50◦, single fragmentation occurred, while for 𝜃𝐴𝐶𝐷−𝑧>60◦, only chipping was recorded. This suggests that the more the largest face impacts parallel to the target surface, the greater the likelihood of fragmentation. For cube specimens, where all faces are geometrically identical, the angles were labelled as 𝜃𝑚, 𝜃𝑖, and 𝜃𝑀, denoting the minimum, intermediate, and maximum values, respectively. Fragmentation was observed when International Journal of Rock Mechanics and Mining Sciences 198 (2026) 106381 7 M. Marchelli et al. Fig. 7. Static test setups illustrating edge-to-edge and vertex-to-vertex loading conditions across different specimen geometries (prisms, slabs, cubes). Fig. 8. Impact and fragmentation sequences for different specimen shapes and contact configurations. (a1) Vertex impact with single fragmentation occurring at the second contact (prism); (a2) corresponding fragmentation event. (b1) Vertex impact with fragmentation at the second contact (slab); (b2) corresponding fragmentation event. (c) Face impact on a slab specimen. (d) Edge impact on a cube specimen with single fragmentation. All images are shown in side view, except for (b), which is presented in plan view. one face was nearly normal to the impacted surface, i.e., typically corresponding to an impact location on the edge. Results from slab and prism specimens suggest that fragmentation is more prone to occur when the shortest side is aligned with the loading axis. This configuration appears to promote stress concentration and reduce the ability of the specimen to redistribute impact forces, thereby increasing the likelihood of breakage. To complement the orientation analysis, the effect of the normalised impact eccentricity 𝑑∕𝑑𝑒𝑞, defined as the horizontal distance between the impact point 𝐴 and the projection of the specimen’s centre of gravity (CoG) onto the impact plane, normalised by the diameter of a sphere with equivalent volume 𝑑𝑒𝑞, was investigated (Fig. 10). Prismatic specimens display a wider range of 𝑑∕𝑑𝑒𝑞 values, attributed to their elongated geometry, which allows for greater variability in impact configurations. It was observed that fragmentation becomes increasingly likely as 𝑑∕𝑑𝑒𝑞 increases, consistent with trends identified through orientation analysis. Specimens impacted closer to their CoG tended to rebound or chip without fragmenting, whereas those with larger International Journal of Rock Mechanics and Mining Sciences 198 (2026) 106381 8 M. Marchelli et al. Fig. 9. Ternary plots of the angles between each of the three orthogonal planes, 𝐴–𝐵–𝐶, 𝐴-𝐵-𝐷, and 𝐴-𝐶-𝐷 and the impacted surface, corresponding to the angles 𝜃𝐴𝐵𝐶−𝑧, 𝜃𝐴𝐵𝐷−𝑧, and 𝜃𝐴𝐶𝐷−𝑧, respectively. Separate plots are shown for prism, slab, and cube specimens. For cube specimens, where the faces are equal, the subscripts 𝑚, 𝑖, and 𝑀 denote the minimum, intermediate, and maximum 𝜃 angles, respectively. Symbols indicate the impact location: circles for vertex impacts, diamonds and stars for edge impacts, and crosses for face impacts. Fig. 10. Boxplot of the normalised impact eccentricity 𝑑∕𝑑eq. The data are subdivided by specimen shape (cubes, prisms, slabs) and grouped by fragmentation mode (C = chipping, i.e., no clear fragmentation, S = single, M = multiple fragmentation) to highlight the influence of impact eccentricity on breakage severity. Each test is colour-coded according to impact location: vertex (V), edge (E), or face (F). normalised eccentricities exhibited higher fragmentation rates. This suggests that eccentric impacts, often with the shortest side aligned to the loading axis, promote stress concentrations and bending (flexural) stresses, increasing the likelihood of fragmentation. As with previous findings, this reinforces the role of impact orientation, in conjunction with geometry, contact location, and asymmetry, in governing failure mechanisms and fragmentation behaviour. To further characterise the fragmentation behaviour, the empirical cumulative distribution function 𝐹(𝑥) was computed for fragments with mass 𝑚𝑓≥1% of the initial specimen mass 𝑚𝑖 (Fig. 11.a). This threshold was selected to exclude small chips, which were present Table 4 Number of fragments (𝑛𝑓) with 𝑚𝑓≥10% 𝑚𝑖 for multiple fragmentation cases. Shape Minimum Median Maximum Prism 3 3 5 Slab 3 5 8 in all tests and do not reflect significant breakage. As fragmentation in cubes was limited to four cases of single fracture, only prism and slab specimens were included in this analysis. For each geometry, the cumulative distribution was constructed by analysing the fragments of all the tests, without averaging across specimens. This approach provides a representative view of the overall fragmentation severity and mass distribution, preserving the variability in fragment number and size inherent to each impact event, which is particularly relevant given the limited sample size and the stochastic nature of fragmentation. The results reveal distinct trends. For prismatic specimens, fragmentation typically involved a single fracture dividing the specimen approximately in half. Accordingly, the 95th percentile of 𝐹(𝑥) corresponds to fragments retaining about 65% of the initial mass. In contrast, slab specimens exhibited more extensive fragmentation, with smaller fragments dominating the mass distribution. For slabs, the 80th percentile of 𝐹(𝑥) falls below 30% of the initial mass, indicating a higher degree of fragmentation and finer fragment sizes. To complement this analysis, the number of fragments with mass 𝑚𝑓 larger than 10% 𝑚𝑖 was recorded for cases classified as multiple fragmentation (Table 4). The data shows differences in fragmentation severity between shapes. Slabs consistently produced a greater number of substantial fragments, while prisms tended to yield fewer, larger pieces. International Journal of Rock Mechanics and Mining Sciences 198 (2026) 106381 9 M. Marchelli et al. Fig. 20. Left column: planar angle 𝛽, measured clockwise from the 𝜂-axis to the velocity vector, plotted against a representative impact orientation angle: 𝜃𝐴𝐵𝐶−𝑧 for prisms, 𝜃𝐴𝐶𝐷−𝑧 for slabs, and 𝜃𝑚 for cubes. Right column: vertical projection angle 𝛼, defined between the vertical and horizontal velocity components, plotted against the same orientation angles. Table 9 Maximum and minimum (maximum in negative direction) values of the velocity components observed in each shape for each impact velocity 𝑣𝑖. Prism Slab 𝑣𝑖7 m/s 7 m/s Axis ≥0<0≥0<0 𝑣𝜉 (m/s) 0.75 0.06 1.90 0.17 𝑣𝜂 (m/s) 0.90 1.30 1.42 0.24 𝑣𝑧 (m/s) 1.14 – 1.32 – Cube 𝑣𝑖7 m/s 8 m/s 10 m/s Axis ≥0<0≥0<0≥0<0 𝑣𝜉 (m/s) 1.72 – 2.42 1.78 2.10 0.47 𝑣𝜂 (m/s) 1.44 1.53 1.37 1.54 2.83 0.04 𝑣𝑧 (m/s) 1.54 – 1.57 – 2.75 0 4.2.3. Apparent coefficient of restitution Fig. 21 presents the relationship between impact orientation and rebound behaviour for non-fragmented specimens. The left column shows the apparent coefficient of restitution (|𝑣𝑒∕𝑣𝑖|), while the right column displays the normal restitution coefficient (|𝑣𝑧∕𝑣𝑖|), both plotted against a representative orientation angle for each shape, selected as for 𝛽 and 𝛼 analysis. The apparent restitution coefficient remains below 0.25 for prisms, about 0.35 for slabs, and up to 0.39 for cubes, confirming the trend observed in 𝑡𝐼: prisms tend to have longer contact durations and higher energy dissipation. Similarly, the normal restitution coefficient |𝑣𝑧∕𝑣𝑖| is the lowest for prisms (below 0.17), followed by slabs (below 0.19), and the highest for cubes (up to 0.28), indicating that postimpact motion is predominantly tangential to the impacted surface in all cases. For prismatic specimens, a slight increasing trend in both |𝑣𝑒∕𝑣𝑖| and |𝑣𝑧∕𝑣𝑖| is observed with increasing 𝜃𝐴𝐵𝐶−𝑧, suggesting that when the largest face is parallel to the impacted surface, energy dissipation is reduced. This behaviour is attributed to the high non-collinearity of the contact, which results in lower impact forces at the contact point. Slabs show an opposite trend with increasing 𝜃𝐴𝐶𝐷−𝑧, indicating that impacts with the largest face normal to the surface result in lower dissipation because of the number of contacts is generally limited to 2 or 3. Finally, cube specimens exhibit a strong decreasing trend in both restitution coefficients with increasing 𝜃𝑚, meaning that impacts with a face parallel to the impacted surface dissipate less energy. This trend holds for both vertex and edge impacts and for all impact velocities. Observed restitution coefficient values for cubes are lower than those reported for harder rocks, consistent with Asteriou et al.10 Although they did not report specimen orientation at impact, nor the exact impact point or number of contacts, they found mean normal restitution coefficients at 5m/s ranging from 0.36 (marl) to 0.66 (sandstone) for cubic specimens, noting that the normal coefficient of restitution increases with material hardness. These observations are consistent with Dattola et al.,27 who reported a strong sensitivity of the restitution coefficient to initial orientation and a decrease in restitution coefficient with increasing aspect ratio. Our results confirm these trends, with cubes consistently exhibiting higher restitution coefficients than slabs and prisms. International Journal of Rock Mechanics and Mining Sciences 198 (2026) 106381 16 M. Marchelli et al. Fig. 21. Restitution analysis for non-fragmented specimens. Left column: apparent coefficient of restitution (|𝑣𝑒∕𝑣𝑖|) plotted against a representative impact orientation angle, 𝜃𝐴𝐵𝐶−𝑧 for prisms, 𝜃𝐴𝐶𝐷−𝑧 for slabs, and 𝜃𝑚 for cubes. Right column: normal restitution coefficient (|𝑣𝑧∕𝑣𝑖|) versus the same angles. 4.2.4. Comparison with spheres To contextualise the rebound behaviour of angular specimens, Table 10 compares the apparent coefficient of restitution ||𝑣𝑒∕𝑣𝑖|| and impact duration 𝑡𝐼 across cubes, prisms, slabs, and spherical specimens of equivalent volume and material. A visual representation of this comparison is provided in Fig. 22, which illustrates the variability in rebound behaviour across shapes and velocities. For spheres, tested under similar conditions at the University of Newcastle,15,16 the impact is collinear and occurs at a single point. In this case, 𝑡𝐼 is theoretically estimated using the formulation by Deresiewicz,69 as function of impact velocity, mass, yield stress, equivalent Young’s modulus, and equivalent radius. The resulting durations (0.493, 0.480, and 0.459 ms for impact velocities of 7, 8, and 10 m/s, respectively) are significantly shorter than those observed for angular specimens. The corresponding restitution values (0.34, 0.33, and 0.31) align well with the analytical model proposed by Stronge,70 which incorporates impact velocity, mass, yield stress, equivalent Young’s modulus, and radius. In contrast, angular specimens, particularly prisms and slabs, exhibit markedly lower restitution values and longer impact durations. This is attributed to the non-collinear nature of the impact and the presence of multiple contact points during the impact phase. Unlike spheres, which engage in a single, brief contact, angular shapes often undergo complex multi-contact interactions involving edges, vertices, and faces. This discrepancy is most pronounced for slabs and prisms, where 𝑡𝐼 can exceed 300 ms and involve up to 8 distinct contact events, as previously discussed. These extended durations and complex contact sequences are primarily due to the geometric asymmetry of the specimens, which amplifies the effects of orientation and impact location. These interactions extend the duration of energy exchange and increase dissipation. For instance, at 𝑣𝑖= 7 m∕s, median restitution values for prisms and slabs are 0.13 and 0.16, respectively, compared to 0.24 for cubes and over 0.30 for spheres. Considering the evidence from Guccione et al.,16 where fragmentation behaviour remained consistent across different sphere sizes when impact velocity is normalised by the critical velocity corresponding to 37% survival probability, and the similarity between our results for cubes and those reported by Das,30 it is reasonable to expect that the general trends observed for angular blocks are likely scalable. 5. Conclusions This study presents a comprehensive experimental investigation into the fragmentation and rebound dynamics of brittle mortar specimens resembling realistic geometries, i.e., cubes, prisms, and slabs, under free-fall impact conditions. The findings offer practical implications for rockfall propagation analysis, particularly in modelling post-impact behaviour and energy dissipation of angular blocks. From a propagation modelling perspective, two key aspects were addressed: the occurrence of fragmentation and the rebound mechanics of intact specimens. The main conclusions to be drawn are as follows. •Fragmentation occurrence is shapeand orientation-dependent: fragmentation has been observed to be highly sensitive to block geometry, impact location, and orientation. Cubes have exhibited the highest fragmentation threshold, fragmenting only at higher velocities and under edge impacts. Slabs and prisms have shown more frequent fragmentation, especially under eccentric International Journal of Rock Mechanics and Mining Sciences 198 (2026) 106381 17 M. Marchelli et al. Table 10 Minimum, maximum, median (50th-percentile) values of the apparent coefficient of restitution |𝑣𝑒∕𝑣𝑖| observed in each shape for each impact velocity 𝑣𝑖. These values provide a quantitative basis for interpreting the trends shown in Fig. 22. Prism Slab 𝑣𝑖7 m/s 7 m/s min max 50th min max 50th |𝑣𝑒∕𝑣𝑖|0.02 0.23 0.13 0.09 0.32 0.16 𝑡𝑖 (s) 0.008 0.316 0.162 0.008 0.344 0.039 Cube 𝑣𝑖7 m/s 8 m/s 10 m/s min max 50th min max 50th min max 50th |𝑣𝑒∕𝑣𝑖|0.12 0.37 0.24 0.15 0.35 0.24 0.15 0.39 0.27 𝑡𝑖 (s) 0.008 0.290 0.024 0.008 0.042 0.024 0.004 0.292 0.026 Sphere 𝑣𝑖7 m/s 8 m/s 10 m/s |𝑣𝑒∕𝑣𝑖|0.34 0.33 0.31 𝑡𝑖 (s) 0.493⋅10−3 0.480⋅10−3 0.459⋅10−3 Fig. 22. Comparison of apparent coefficient of restitution (|𝑣𝑒∕𝑣𝑖|) and impact duration (𝑡𝐼) for prism, slab, and cube specimens at different impact velocities. Symbols represent median values, while error bars indicate minimum and maximum ranges. This visual representation complements Table 10. impacts and when large faces are oriented parallel to the impacted surface. These findings suggest that fragmentation probability should be explicitly incorporated into trajectory models through shape-specific probabilities and orientation criteria. •Static tests provide predictive insight into dynamic fragmentation: the fracture modes observed in static splitting tests, particularly tensile splitting and delamination, can be correlated with dynamic fragmentation behaviour. Specimens exhibiting vertex fragility or asymmetric fracture patterns under static loading are more prone to fragmentation during impact. This suggests that static mechanical characterisation can serve as a valuable tool for assessing dynamic fragility and pre-damage effects in rockfall scenarios. •Energy dissipation and rebound mechanics are governed by contact complexity: for intact specimens, rebound behaviour has been analysed in terms of impact duration, number of contact events, and post-impact velocity components. Prisms and slabs have exhibited longer contact durations and more complex multicontact sequences, resulting in greater energy dissipation and lower apparent restitution coefficients compared to cubes. These differences are primarily attributed to the geometric asymmetry of the specimens, which promotes uneven stress distribution and irregular contact configurations during impact. Defining an apparent coefficient of restitution has proved to be effective for non-collinear impacts, where multiple contact points and complex motion patterns challenge traditional restitution definitions. Although not a predictive model, the consistent trends observed across shapes and orientations provide a basis for anticipating impact outcomes and energy dissipation behaviour. This supports the integration of shape-dependent restitution parameters into trajectory models, enhancing their predictive capability. •Orientation influences rebound metrics and energy partitioning: the apparent and normal restitution coefficients, as well as the vertical projection angle 𝛼, vary systematically with impact orientation and are affected by the shape. •Rebound directionality is consistently biased yet probabilistic: across all shapes, rebound motion is predominantly aligned with the positive 𝜉 axis, i.e., from the impact point towards the centre of gravity. However, due to the inherent unpredictability of impact orientation and contact location in real rockfall scenarios, this directionality must be treated probabilistically. The observed bias supports the use of shape-aligned local reference systems, but trajectory models should incorporate stochastic elements to account for variability in initial conditions. Overall, the results underscore the limitations of spherical simplifications in rockfall models. The dataset provided by this study offers quantitative metrics, such as shape-dependent fragmentation probabilities and apparent restitution coefficients, that can be directly integrated into numerical rockfall models. These parameters can enable calibration of DEM and rigid-body trajectory models, replacing generic spherical assumptions and improving predictions of rebound behaviour and energy dissipation. For lumped-mass approaches, apparent restitution coefficients can be adopted to better capture non-collinear impacts. Furthermore, incorporating geometry-dependent fragmentation probabilities into stochastic fragmentation models enhances the realism of International Journal of Rock Mechanics and Mining Sciences 198 (2026) 106381 18 M. Marchelli et al. trajectory simulations, allowing for more accurate estimation of runout distances, potential impact energies, and impact heights, and ultimately supports more reliable hazard and risk assessments71. Building on these results, future research will focus on deriving predictive equations that link impact conditions, block geometry, and fragmentation probability to enable direct integration into propagation models. Future studies will explicitly address size effects by testing different specimen scales and investigating whether scale-independent fragmentation patterns can be applied to angular blocks. Additional work will include testing natural rock specimens and alternative materials, as well as validating these results within numerical models to enhance predictive accuracy and strengthen hazard assessment frameworks. CRediT authorship contribution statement Maddalena Marchelli: Writing – review & editing, Writing – original draft, Validation, Project administration, Methodology, Investigation, Funding acquisition, Formal analysis, Data curation, Conceptualization. Davide Ettore Guccione: Writing – review & editing, Validation, Project administration, Methodology, Funding acquisition, Conceptualization. Anna Giacomini: Writing – review & editing, Project administration, Funding acquisition, Conceptualization. Olivier Buzzi: Writing – review & editing, Project administration, Funding acquisition, Conceptualization. Open access This article is licensed under a Creative Commons Attribution 4.0 International License, which permits use, sharing, adaptation, distribution and reproduction in any medium or format, as long as you give appropriate credit to the original author(s) and the source, provide a link to the Creative Commons licence, and indicate if changes were made. The images or other third party material in this article are included in the article’s Creative Commons licence, unless indicated otherwise in a credit line to the material. If material is not included in the article’s Creative Commons licence and your intended use is not permitted by statutory regulation or exceeds the permitted use, you will need to obtain permission directly from the copyright holder. To view a copy of this licence, visit http://creativecommons.org/licenses/by/4. 0/. Funding This work was supported by Marie Curie Postdoctoral Fellowship 2022 (Call Horizon-MSCA-2022-PF-01, grant GA101103401 - RIDETHERISK project), by Australian Research Council (IE230100410 and DP160103140) and Rocscience Inc. Acknowledgements The help received from Dr. Michele Spadari in preparing the samples and conducting the experiments is also gratefully acknowledged. Declaration of competing interest The authors declare that there are no conflicts of interests. 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