Thermal Properties of Close-Packed Iron Determined Using Hugoniot Functions
Creators
- 1. Kobe University of Mercantile Marine (Japan)
- 2. Graduate School of Engineering, Osaka University, Suita, Osaka 565-0871 (Japan)
Description
A quadratic equation for the temperature-independent Grueneisen coefficient γ was derived by a method in which the Walsh-Christian and Mie-Grueneisen equations are combined. Some previously existing ab initio temperature Hugoniots for hexagonal close-packed solid Fe are inaccurate because the constant-volume specific heats on the Hugoniots CVH, which are related uniquely to the solutions of the quadratic equation, have values that are too small. A CVH distribution in the solid phase range was demonstrated to agree approximately with a previous ab initio distribution. In contrast, the corresponding γ distribution was significantly different from the ab initio distribution in the lower pressure region. The causes of these disagreements are clarified
Additional details
Identifiers
- DOI
- 10.1063/1.2263283;
Publishing Information
- Journal Title
- AIP Conference Proceedings
- Journal Volume
- 845
- Journal Issue
- 1
- Journal Page Range
- p. 135-138
- ISSN
- 0094-243X
- CODEN
- APCPCS
Conference
- Title
- American Physical Society Topical Group conference on shock compression of condensed matter
- Dates
- 31 Jul - 5 Aug 2005
- Place
- Baltimore, MD (United States)
INIS
- Country of Publication
- United States
- Country of Input or Organization
- International Atomic Energy Agency (IAEA)
- INIS RN
- 38043225
- Subject category
- S75: CONDENSED MATTER PHYSICS, SUPERCONDUCTIVITY AND SUPERFLUIDITY; S36: MATERIALS SCIENCE;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- DISTRIBUTION; EQUATIONS OF STATE; HCP LATTICES; IRON; MATHEMATICAL SOLUTIONS; SOLIDS; SPECIFIC HEAT
- Descriptors DEC
- CRYSTAL LATTICES; CRYSTAL STRUCTURE; ELEMENTS; EQUATIONS; HEXAGONAL LATTICES; METALS; PHYSICAL PROPERTIES; THERMODYNAMIC PROPERTIES; TRANSITION ELEMENTS
Optional Information
- Notes
- (c) 2006 American Institute of Physics