Published March 2015 | Version v1
Journal article

The equation of state of nuclear material to explore in the neutron star

  • 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.