Работы, на которые ссылается эта работа
Работ: 89
Работа: Constraining the high-density behavior of the nuclear symmetry energy with the tidal polarizability of neutron stars
A two-solar-mass neutron star measured using Shapiro delay
Paul B. Demorest, Timothy T. Pennucci, S. M. Ransom +2
Статья2010Цитирований: 13ABIReaction dynamics with exotic nuclei
V. Baran, M. Colonna, Vincenzo Greco +1
Статья2005Цитирований: 11ABIA Skyrme parametrization from subnuclear to neutron star densities
E. Chabanat, P. Bonche, P. Haensel +2
Статья1997Цитирований: 10ABIIsospin asymmetry in nuclei and neutron stars
A.W. Steiner, M. Prakash, J.M. Lattimer +1
Статья2005Цитирований: 10ABIEffective Nucleon Masses in Symmetric and Asymmetric Nuclear Matter
E. N. E. van Dalen, Christian Fuchs, Amand Faessler
Статья2005Цитирований: 9ABIDetermination of the Equation of State of Dense Matter
Paweł Danielewicz, R. Lacey, W. G. Lynch
Статья2002Цитирований: 8ABIConstraining neutron-star tidal Love numbers with gravitational-wave detectors
Éanna É. Flanagan, Tanja Hinderer
Статья2008Цитирований: 6ABIRelativistic effective interaction for nuclei, giant resonances, and neutron stars
F. J. Fattoyev, C. J. Horowitz, J. Piekarewicz +1
Статья2010Цитирований: 6ABINew parametrization for the Lagrangian density of relativistic mean field theory
G. A. Lalazissis, Joshua Leon Konig, P. Ring
Статья1997Цитирований: 6ABIEffective masses in relativistic approaches to the nucleon-nucleus mean field
Статья1989Цитирований: 6ABIAsymmetric nuclear matter: The role of the isovector scalar channel
Benye Liu, Vincenzo Greco, V. Baran +2
Статья2002Цитирований: 6ABIRecent Progress in Quantum Hadrodynamics
Brian D. Serot, John Dirk Walecka
Статья1997Цитирований: 6ABIRecent progress and new challenges in isospin physics with heavy-ion reactions
B LI, Lie-Wen Chen, Che Ming Ko
Статья2008Цитирований: 5ABIRelativistic mean-field theory and the high-density nuclear equation of state
Статья1996Цитирований: 5ABINeutron Star Structure and the Neutron Radius of<mml:math xmlns:mml="http://www.w3.org/1998/Math/MathML" display="inline"><mml:mrow><mml:mmultiscripts><mml:mrow><mml:mi>P</mml:mi></mml:mrow><mml:mprescripts/><mml:mrow/><mml:mrow><mml:mn>208</mml:mn></mml:mrow><mml:mrow/><mml:mrow/></mml:mmultiscripts></mml:mrow><mml:mi>b</mml:mi></mml:math>
C. J. Horowitz, J. Piekarewicz
Статья2001Цитирований: 5ABIDensity slope of the nuclear symmetry energy from the neutron skin thickness of heavy nuclei
Lie-Wen Chen, Che Ming Ko, Bao-An Li +1
Статья2010Цитирований: 4ABIIncompressibility of Nuclear Matter from the Giant Monopole Resonance
D. H. Youngblood, H. L. Clark, Y.-W. Lui
Статья1999Цитирований: 4ABIRelativistic mean field theory of nuclei with a vector meson self-interaction
Статья1991Цитирований: 4ABIIsospin-dependent properties of asymmetric nuclear matter in relativistic mean field models
Lie-Wen Chen, Che Ming Ko, Bao-An Li
Статья2007Цитирований: 4ABI