The equation of state of nuclear material to explore in the neutron star
Creators
- 1. Tokyo University of Science, Faculty of Science and Technology, Noda, Chiba (Japan)
Description
A neutron star is considered to be composed of the central region 'core' with the density of equivalent to or several times of nucleus density, and the low-density region called 'crust' surrounding the outside of the core. This paper starts from the basic knowledge of the state equation of uniform nuclear material, and discusses how the state equation of the material constituting neutron star is characterized. It also describes the state equation of the core of neutron star and the maximum mass of neutron star. The maximum mass of neutral star does not reach twice the mass of the sun when considering hyperon, which poses a question called 'hyperon puzzle.' Finally, this paper refers to the neutron star crust, and explains the shape and size of the aggregation formed by nucleons themselves that can be regarded as 'nuclei' in the region close to the inner core. (A.O.)
Additional details
Publishing Information
- Journal Title
- Genshikaku Kenkyu
- Journal Volume
- 59
- Journal Issue
- suppl.1
- Journal Page Range
- p. 46-51
- ISSN
- 0367-4169
Conference
- Title
- 2014 summer school of young nuclear and particle physicist group of Japan
- Dates
- 4-9 Aug 2014
- Place
- Kijimadaira, Nagano (Japan)
INIS
- Country of Publication
- Japan
- Country of Input or Organization
- Japan
- INIS RN
- 47026806
- Subject category
- S73: NUCLEAR PHYSICS AND RADIATION PHYSICS;
- Resource subtype / Literary indicator
- Conference
- Descriptors DEI
- BINDING ENERGY; DENSITY; EQUATIONS OF STATE; HYPERONS; MASS; NEUTRON STARS; NUCLEAR MATTER; NUCLEAR RADII; SHAPE; STAR MODELS
- Descriptors DEC
- BARYONS; ELEMENTARY PARTICLES; ENERGY; EQUATIONS; FERMIONS; HADRONS; MATHEMATICAL MODELS; MATTER; NUCLEAR PROPERTIES; PHYSICAL PROPERTIES; STARS; STRANGE PARTICLES
Optional Information
- Notes
- 9 refs., 1 fig.