Published November 2, 2006 | Version v1
Journal article Metadata-only

Magnetic susceptibility oscillation in neutron stars with the hadron-quark transition

Creators

  • 1. Institute of Applied Physics, Chinese Academy of Sciences, Shanghai 201800 (China)
  • 2. Institut de Physique Nucleaire, F-91406 Orsay cedex (France)

Description

We analyze the de Hass-van Alphen (HVA) oscillation of magnetic susceptibility in the nuetron star matter using an analytic relativistic expression obtained before, showing that the oscillation frequency is proportional to the squared chemical potential and the reciprocal of the field, and is independent of the temperature. The numerical results for the HVA oscillation are also shown. A superposition of the HVA oscillations changes the oscillation properties drastically if the color deconfinement occurs at high densities

Additional details

Identifiers

DOI
10.1063/1.2398859;

Publishing Information

Journal Title
AIP Conference Proceedings
Journal Volume
865
Journal Issue
1
Journal Page Range
p. 256-261
ISSN
0094-243X
CODEN
APCPCS

Conference

Title
6. China-Japan joint nuclear physics symposium
Dates
16-20 May 2006
Place
Shanghai (China)

INIS

Country of Publication
United States
Country of Input or Organization
International Atomic Energy Agency (IAEA)
INIS RN
38056280
Subject category
S72: PHYSICS OF ELEMENTARY PARTICLES AND FIELDS;
Resource subtype / Literary indicator
Conference
Descriptors DEI
COLOR MODEL; MAGNETIC SUSCEPTIBILITY; NEUTRON STARS; OSCILLATIONS; QUANTUM CHROMODYNAMICS; QUARK-HADRON INTERACTIONS; RELATIVISTIC RANGE
Descriptors DEC
COMPOSITE MODELS; ENERGY RANGE; FIELD THEORIES; INTERACTIONS; MAGNETIC PROPERTIES; MATHEMATICAL MODELS; PARTICLE INTERACTIONS; PARTICLE MODELS; PHYSICAL PROPERTIES; QUANTUM FIELD THEORY; QUARK MODEL; STARS

Optional Information

Notes
(c) 2006 American Institute of Physics