Effects of input energy and impactor shape on cranial fracture patterns

This study documents relationships between input energy, impactor shape, and the formation of fractures in human crania. Parietal impact experiments (n = 12) were performed at 67% higher input energy compared to previously reported experiments. Fracture origins, characteristics, and locations were c...

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Veröffentlicht in:Forensic science international 2023-11, Vol.352, p.111859-111859, Article 111859
Hauptverfasser: Isa, Mariyam I., Fenton, Todd W., Goots, Alexis C., Watson, Elena O., Vaughan, Patrick E., Wei, Feng
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Sprache:eng
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Zusammenfassung:This study documents relationships between input energy, impactor shape, and the formation of fractures in human crania. Parietal impact experiments (n = 12) were performed at 67% higher input energy compared to previously reported experiments. Fracture origins, characteristics, and locations were compared at two input energy levels with three impactor shapes (focal “hammer”, flat “brick”, and curved “bat”). Impacts with all three impactors at both energy levels produced fractures originating at and remote to the impact site, indicating both mechanisms are typical in temporoparietal blunt force impacts. Higher energy impacts generally produced more impact site fractures, depression, and comminution than lower energy impacts. A small, focal impactor produced cone cracks, depression, and fractures localized near the impact site. A broad, curved impactor produced circumferential fractures and linear fractures extending into adjacent bones. A broad, flat impactor produced fracture patterns ranging from linear fractures to large depressed and comminuted defects. •Parietal impacts can produce fractures at the impact site, remotely, or both.•Generally, higher energy impacts produced more impact site fracture.•Fracture characteristics varied within both the higher and lower energy groups.•Fracture characteristics varied between focal and broader impacts.•The presence of only linear fractures cannot be used to exclude an impact surface.
ISSN:0379-0738
1872-6283
DOI:10.1016/j.forsciint.2023.111859