Nuclear equation of state and the structure of neutron stars

AEL Dieperink; D Van Neck; Y Dewulf; [No Value] Rodin

Nuclear equation of state and the structure of neutron stars

AEL Dieperink^*, D Van Neck, Y Dewulf, [No Value] Rodin

^*Corresponding author for this work

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution › Academic › peer-review

Abstract

The hadronic equation of state for a neutron star is discussed with a particular emphasis on the symmetry energy. The results of several microscopic approaches are compared and also a new calculation in terms of the self-consistent Green function method is presented. In addition possible constraints on the symmetry energy coming from empirical information on the neutron skin of finite nuclei are considered.

Original language	English
Title of host publication	SUPERDENSE QCD MATTER AND COMPACT STARS
Editors	D Blaschke, D Dedrakian
Place of Publication	DORDRECHT
Publisher	Springer
Pages	93-111
Number of pages	19
ISBN (Print)	1-4020-3428-8
Publication status	Published - 2006
Event	NATO Advanced Research Workshop on Superdense QCD Matter and Compact Stars - , Armenia Duration: 27-Sept-2003 → 4-Oct-2003

Publication series

Name	NATO Science Series II-Mathematics Physics and Chemistry
Publisher	SPRINGER
Volume	197
ISSN (Print)	1568-2609

Other

Other	NATO Advanced Research Workshop on Superdense QCD Matter and Compact Stars
Country/Territory	Armenia
Period	27/09/2003 → 04/10/2003

Keywords

ISOBARIC ANALOG RESONANCES
SYMMETRY ENERGY
OF-STATE
MATTER
APPROXIMATION
CONSISTENCY
EXCITATION
RADII
SKIN

Handle.net

Persistent link

Cite this

@inproceedings{bf92f29c35f44e2fadc65b6a760d8565,

title = "Nuclear equation of state and the structure of neutron stars",

abstract = "The hadronic equation of state for a neutron star is discussed with a particular emphasis on the symmetry energy. The results of several microscopic approaches are compared and also a new calculation in terms of the self-consistent Green function method is presented. In addition possible constraints on the symmetry energy coming from empirical information on the neutron skin of finite nuclei are considered.",

keywords = "ISOBARIC ANALOG RESONANCES, SYMMETRY ENERGY, OF-STATE, MATTER, APPROXIMATION, CONSISTENCY, EXCITATION, RADII, SKIN",

author = "AEL Dieperink and {Van Neck}, D and Y Dewulf and Rodin, {[No Value]}",

year = "2006",

language = "English",

isbn = "1-4020-3428-8",

series = "NATO Science Series II-Mathematics Physics and Chemistry",

publisher = "Springer",

pages = "93--111",

editor = "D Blaschke and D Dedrakian",

booktitle = "SUPERDENSE QCD MATTER AND COMPACT STARS",

note = "NATO Advanced Research Workshop on Superdense QCD Matter and Compact Stars ; Conference date: 27-09-2003 Through 04-10-2003",

}

Dieperink, AEL, Van Neck, D, Dewulf, Y & Rodin, NV 2006, Nuclear equation of state and the structure of neutron stars. in D Blaschke & D Dedrakian (eds), SUPERDENSE QCD MATTER AND COMPACT STARS. NATO Science Series II-Mathematics Physics and Chemistry, vol. 197, Springer, DORDRECHT, pp. 93-111, NATO Advanced Research Workshop on Superdense QCD Matter and Compact Stars, Armenia, 27/09/2003.

Nuclear equation of state and the structure of neutron stars. / Dieperink, AEL; Van Neck, D; Dewulf, Y et al.
SUPERDENSE QCD MATTER AND COMPACT STARS. ed. / D Blaschke; D Dedrakian. DORDRECHT: Springer, 2006. p. 93-111 (NATO Science Series II-Mathematics Physics and Chemistry; Vol. 197).

Research output: Chapter in Book/Report/Conference proceeding › Conference contribution › Academic › peer-review

TY - GEN

T1 - Nuclear equation of state and the structure of neutron stars

AU - Dieperink, AEL

AU - Van Neck, D

AU - Dewulf, Y

AU - Rodin, [No Value]

PY - 2006

Y1 - 2006

N2 - The hadronic equation of state for a neutron star is discussed with a particular emphasis on the symmetry energy. The results of several microscopic approaches are compared and also a new calculation in terms of the self-consistent Green function method is presented. In addition possible constraints on the symmetry energy coming from empirical information on the neutron skin of finite nuclei are considered.

AB - The hadronic equation of state for a neutron star is discussed with a particular emphasis on the symmetry energy. The results of several microscopic approaches are compared and also a new calculation in terms of the self-consistent Green function method is presented. In addition possible constraints on the symmetry energy coming from empirical information on the neutron skin of finite nuclei are considered.

KW - ISOBARIC ANALOG RESONANCES

KW - SYMMETRY ENERGY

KW - OF-STATE

KW - MATTER

KW - APPROXIMATION

KW - CONSISTENCY

KW - EXCITATION

KW - RADII

KW - SKIN

M3 - Conference contribution

SN - 1-4020-3428-8

T3 - NATO Science Series II-Mathematics Physics and Chemistry

SP - 93

EP - 111

BT - SUPERDENSE QCD MATTER AND COMPACT STARS

A2 - Blaschke, D

A2 - Dedrakian, D

PB - Springer

CY - DORDRECHT

T2 - NATO Advanced Research Workshop on Superdense QCD Matter and Compact Stars

Y2 - 27 September 2003 through 4 October 2003

ER -

Nuclear equation of state and the structure of neutron stars

Abstract

Publication series

Other

Keywords

Handle.net

Fingerprint

Cite this