Published December 2010 | Version v1
Book Metadata-only

Composition and EOS of β-stable charge neutral n + p + e + μ matter at finite temperature

Creators

  • 1. Department of Physics, Sambalpur University, Sambalpur (India)

Description

The work has calculated the equilibrium proton fraction in hot charge neutral β - stable n + p + e + μ matter that constitutes the bulk of supernovae matter and PNS core, by using the free symmetry energy

Part of:
DAE-BRNS symposium on nuclear physics. V. 55

Additional details

Publishing Information

Publisher
Bhabha Atomic Research Centre
Imprint Place
Mumbai (India)
Imprint Title
DAE-BRNS symposium on nuclear physics. V. 55
Imprint Pagination
[944 p.]
Journal Page Range
p. 464-465

Conference

Title
DAE-BRNS symposium on nuclear physics
Dates
20-24 Dec 2010
Place
Pilani (India)

INIS

Country of Publication
India
Country of Input or Organization
India
INIS RN
42103763
Subject category
S79: ASTROPHYSICS, COSMOLOGY AND ASTRONOMY;
Resource subtype / Literary indicator
Conference
Descriptors DEI
DEGREES OF FREEDOM; EQUATIONS OF STATE; NEUTRON STARS; NEUTRON-RICH ISOTOPES; SUPERNOVAE; SYMMETRY; TEMPERATURE DEPENDENCE
Descriptors DEC
BETA DECAY RADIOISOTOPES; BETA-MINUS DECAY RADIOISOTOPES; BINARY STARS; EQUATIONS; ERUPTIVE VARIABLE STARS; ISOTOPES; RADIOISOTOPES; STARS; VARIABLE STARS

Optional Information

Notes
3 refs., 2 figs.