Nuclear constraints on the equation of state and rotating neutron stars

A. E L Dieperink, C. Korpa

Research output: Contribution to journalArticle

Abstract

In this contribution nuclear constraints on the equation of state for a neutron star are discussed. A combined fit to nuclear masses and charge radii leads to improved values for the symmetry energy and its derivative at nuclear saturation density, Sv 31 MeV and L 68 ± 8 MeV. As an application the sensitivity of some properties of rotating supramassive neutron stars on the EoS is discussed.

Original languageEnglish
Article number012004
JournalJournal of Physics: Conference Series
Volume496
Issue number1
DOIs
Publication statusPublished - 2014

Fingerprint

neutron stars
equations of state
saturation
radii
sensitivity
symmetry
energy

ASJC Scopus subject areas

  • Physics and Astronomy(all)

Cite this

Nuclear constraints on the equation of state and rotating neutron stars. / Dieperink, A. E L; Korpa, C.

In: Journal of Physics: Conference Series, Vol. 496, No. 1, 012004, 2014.

Research output: Contribution to journalArticle

@article{0f9102e4db444252b271f9d179e5e594,
title = "Nuclear constraints on the equation of state and rotating neutron stars",
abstract = "In this contribution nuclear constraints on the equation of state for a neutron star are discussed. A combined fit to nuclear masses and charge radii leads to improved values for the symmetry energy and its derivative at nuclear saturation density, Sv 31 MeV and L 68 ± 8 MeV. As an application the sensitivity of some properties of rotating supramassive neutron stars on the EoS is discussed.",
author = "Dieperink, {A. E L} and C. Korpa",
year = "2014",
doi = "10.1088/1742-6596/496/1/012004",
language = "English",
volume = "496",
journal = "Journal of Physics: Conference Series",
issn = "1742-6588",
publisher = "IOP Publishing Ltd.",
number = "1",

}

TY - JOUR

T1 - Nuclear constraints on the equation of state and rotating neutron stars

AU - Dieperink, A. E L

AU - Korpa, C.

PY - 2014

Y1 - 2014

N2 - In this contribution nuclear constraints on the equation of state for a neutron star are discussed. A combined fit to nuclear masses and charge radii leads to improved values for the symmetry energy and its derivative at nuclear saturation density, Sv 31 MeV and L 68 ± 8 MeV. As an application the sensitivity of some properties of rotating supramassive neutron stars on the EoS is discussed.

AB - In this contribution nuclear constraints on the equation of state for a neutron star are discussed. A combined fit to nuclear masses and charge radii leads to improved values for the symmetry energy and its derivative at nuclear saturation density, Sv 31 MeV and L 68 ± 8 MeV. As an application the sensitivity of some properties of rotating supramassive neutron stars on the EoS is discussed.

UR - http://www.scopus.com/inward/record.url?scp=84898078205&partnerID=8YFLogxK

UR - http://www.scopus.com/inward/citedby.url?scp=84898078205&partnerID=8YFLogxK

U2 - 10.1088/1742-6596/496/1/012004

DO - 10.1088/1742-6596/496/1/012004

M3 - Article

AN - SCOPUS:84898078205

VL - 496

JO - Journal of Physics: Conference Series

JF - Journal of Physics: Conference Series

SN - 1742-6588

IS - 1

M1 - 012004

ER -