CALIBRATING THE JOHNSON-HOLMQUIST CERAMIC MODEL FOR SIC USING CTH
Creators
- 1. University of Alabama at Birmingham (United States)
- 2. U.S. Army Research Laboratory, APG, MD 21005 (United States)
Description
The Johnson-Holmquist ceramic material model has been calibrated and successfully applied to numerically simulate ballistic events using the Lagrangian code EPIC. While the majority of the constants are ''physics'' based, two of the constants for the failed material response are calibrated using ballistic experiments conducted on a confined cylindrical ceramic target. The maximum strength of the failed ceramic is calibrated by matching the penetration velocity. The second refers to the equivalent plastic strain at failure under constant pressure and is calibrated using the dwell time. Use of these two constants in the CTH Eulerian hydrocode does not predict the ballistic response. This difference may be due to the phenomenological nature of the model and the different numerical schemes used by the codes. This paper determines the aforementioned material constants for SiC suitable for simulating ballistic events using CTH.
Additional details
Identifiers
- DOI
- 10.1063/1.3295073;
Publishing Information
- Journal Title
- AIP Conference Proceedings
- Journal Volume
- 1195
- Journal Issue
- 1
- Journal Page Range
- p. 1405-1408
- ISSN
- 0094-243X
- CODEN
- APCPCS
Conference
- Title
- American Physical Society Topical Group on shock compression of condensed matter
- Dates
- 28 Jun - 3 Jul 2009
- Place
- Nashville, TN (United States)
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 41099112
- Subject category
- S36: MATERIALS SCIENCE;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- CERAMICS; CYLINDRICAL CONFIGURATION; FAILURES; LAGRANGIAN FUNCTION; PLASTICITY; SILICON CARBIDES; STRAINS
- Descriptors DEC
- CARBIDES; CARBON COMPOUNDS; CONFIGURATION; FUNCTIONS; MECHANICAL PROPERTIES; SILICON COMPOUNDS
Optional Information
- Notes
- (c) 2009 American Institute of Physics