Equations of state for supernovae and compact stars

被引：837

作者：

Oertel, M. ^{[1
]}

Hempel, M. ^{[2
]}

Klahn, T. ^{[3
]}

Typel, S. ^{[4
,5
]}

机构：

[1] Univ Paris Diderot, PSL Res Univ, Sorbonne Paris Cite, Lab Univ & Theories,CNRS,Observ Paris, 5 Pl Jules Janssen, F-92195 Meudon, France

[2] Univ Basel, Dept Phys, Klingelbergstr 82, CH-4056 Basel, Switzerland

[3] Uniwersytet Wroclawski, Inst Fizyki Teoretycznej, Pl M Borna 9, PL-50204 Wroclaw, Poland

[4] Tech Univ Darmstadt, Inst Kernphys, Schlossgartenstr 9, D-64289 Darmstadt, Germany

[5] GSI Helmholtzzentrum Schwerionenforsch, Planckstr 1, D-64291 Darmstadt, Germany

来源：

REVIEWS OF MODERN PHYSICS | 2017年 / 89卷 / 01期

基金：

瑞士国家科学基金会;

关键词：

NUCLEAR SYMMETRY ENERGY; EFFECTIVE-FIELD THEORY; HEAVY-ION COLLISIONS; SELF-CONSISTENT CALCULATIONS; CORE-COLLAPSE SUPERNOVAE; BLACK-HOLE FORMATION; MONTE-CARLO CALCULATIONS; NEUTRON SKIN THICKNESS; GAS PHASE-TRANSITION; GAUGE VECTOR-MESONS;

D O I：

10.1103/RevModPhys.89.015007

中图分类号：

O4 [物理学];

学科分类号：

0702 ;

摘要：

A review is given of various theoretical approaches for the equation of state (EoS) of dense matter, relevant for the description of core-collapse supernovae, compact stars, and compact star mergers. The emphasis is put on models that are applicable to all of these scenarios. Such EoS models have to cover large ranges in baryon number density, temperature, and isospin asymmetry. The characteristics of matter change dramatically within these ranges, from a mixture of nucleons, nuclei, and electrons to uniform, strongly interacting matter containing nucleons, and possibly other particles such as hyperons or quarks. As the development of an EoS requires joint efforts from many directions, different theoretical approaches are considered and relevant experimental and observational constraints which provide insights for future research are discussed. Finally, results from applications of the discussed EoS models are summarized.

引用

页数：68

共 1034 条

[1] Measurement of the Neutron Radius of 208Pb through Parity Violation in Electron Scattering
Abrahamyan, S.
Ahmed, Z.
Albataineh, H.
Aniol, K.
Armstrong, D. S.
Armstrong, W.
Averett, T.
Babineau, B.
Barbieri, A.
Bellini, V.
Beminiwattha, R.
Benesch, J.
Benmokhtar, F.
Bielarski, T.
Boeglin, W.
Camsonne, A.
Canan, M.
Carter, P.
Cates, G. D.
Chen, C.
Chen, J-P
Hen, O.
Cusanno, F.
Dalton, M. M.
De Leo, R.
de Jager, K.
Deconinck, W.
Decowski, P.
Deng, X.
Deur, A.
Dutta, D.
Etile, A.
Flay, D.
Franklin, G. B.
Friend, M.
Frullani, S.
Fuchey, E.
Garibaldi, F.
Gasser, E.
Gilman, R.
Giusa, A.
Glamazdin, A.
Gomez, J.
Grames, J.
Gu, C.
Hansen, O.
Hansknecht, J.
Higinbotham, D. W.
Holmes, R. S.
Holmstrom, T.
[J]. PHYSICAL REVIEW LETTERS, 2012, 108 (11)
[2] Isospin effects and symmetry energy studies with INDRA
Ademard, G.
Borderie, B.
Chbihi, A.
Lopez, O.
Napolitani, P.
Rivet, M. F.
Boisjoli, M.
Bonnet, E.
Bougault, R.
Frankland, J. D.
Galichet, E.
Gruyer, D.
Guinet, D.
Kabtoul, M.
Lehaut, G.
Lautesse, P.
La Commara, M.
Le Neindre, N.
Marini, P.
Parlog, M.
Pawlowski, P.
Rosato, E.
Roy, R.
Spadaccini, G.
Vient, E.
Vigilante, M.
Wieleczko, J. P.
[J]. EUROPEAN PHYSICAL JOURNAL A, 2014, 50 (02) : 1 - 19
[3] Evidence for Heavy Hyperhydrogen Λ6H
Agnello, M.
Benussi, L.
Bertani, M.
Bhang, H. C.
Bonomi, G.
Botta, E.
Bregant, M.
Bressani, T.
Bufalino, S.
Busso, L.
Calvo, D.
Camerini, P.
Dalena, B.
De Mori, F.
D'Erasmo, G.
Fabbri, F. L.
Feliciello, A.
Filippi, A.
Fiore, E. M.
Fontana, A.
Fujioka, H.
Genova, P.
Gianotti, P.
Grion, N.
Lucherini, V.
Marcello, S.
Mirfakhrai, N.
Moia, F.
Morra, O.
Nagae, T.
Outa, H.
Pantaleo, A.
Paticchio, V.
Piano, S.
Rui, R.
Simonetti, G.
Wheadon, R.
Zenoni, A.
Gal, A.
[J]. PHYSICAL REVIEW LETTERS, 2012, 108 (04)
[4] Symmetry energy of warm nuclear systems
Agrawal, B. K.
De, J. N.
Samaddar, S. K.
Centelles, M.
Vinas, X.
[J]. EUROPEAN PHYSICAL JOURNAL A, 2014, 50 (02) : 1 - 11
[5] Determining the Density Content of Symmetry Energy and Neutron Skin: An Empirical Approach
Agrawal, B. K.
De, J. N.
Samaddar, S. K.
[J]. PHYSICAL REVIEW LETTERS, 2012, 109 (26)
[6] Determination of the parameters of a Skyrme type effective interaction using the simulated annealing approach
Agrawal, BK
Shlomo, S
Au, VK
[J]. PHYSICAL REVIEW C, 2005, 72 (01):
[7] Measurement of the Ξ- p scattering cross sections at low energy
Ahn, JK
Aoki, S
Chung, KS
Chung, MS
En'yo, H
Fukuda, T
Funahashi, H
Goto, Y
Higashi, A
Ieiri, M
Iijima, T
Iinuma, M
Imai, K
Itow, Y
Lee, JM
Makino, S
Masaike, A
Matsuda, Y
Matsuyama, Y
Mihara, S
Nagoshi, C
Nomura, I
Park, IS
Saito, N
Sekimoto, M
Shin, YM
Sim, KS
Susukita, R
Takashima, R
Takeutchi, F
Tlusty, P
Weibe, S
Yokkaichi, S
Yoshida, K
Yoshida, M
Yoshida, T
Yamashita, S
[J]. PHYSICS LETTERS B, 2006, 633 (2-3) : 214 - 218
[8] QUANTUM MOLECULAR-DYNAMICS - A DYNAMIC MICROSCOPIC N-BODY APPROACH TO INVESTIGATE FRAGMENT FORMATION AND THE NUCLEAR-EQUATION OF STATE IN HEAVY-ION COLLISIONS
AICHELIN, J
[J]. PHYSICS REPORTS-REVIEW SECTION OF PHYSICS LETTERS, 1991, 202 (5-6): : 233 - 360
[9] Aichelin J., 2009, RELATIVISTIC HEAVY I, VI
[10] Equation of state of nucleon matter and neutron star structure
Akmal, A
Pandharipande, VR
Ravenhall, DG
[J]. PHYSICAL REVIEW C, 1998, 58 (03): : 1804 - 1828

← 1 2 3 4 5 6 7 8 9 10 →