Maximum mass and radius of neutron stars, and the nuclear symmetry energy
作者： S. Gandolfi , J. Carlson , Sanjay Reddy
DOI: 10.1103/PHYSREVC.85.032801
关键词:
摘要: We calculate the equation of state of neutron matter with realistic two-and three-nucleon interactions using quantum Monte Carlo techniques and illustrate that the short-range three-neutron interaction determines the correlation between neutron matter energy at nuclear saturation density and higher densities relevant to neutron stars. Our model also makes an experimentally testable prediction for the correlation between the nuclear symmetry energy and its density dependence—determined solely by the strength of the short-range terms in …
harvard.edu
arxiv.org
osti.gov
arxiv-vanity.com参考文章(33)
P. B. Demorest, T. Pennucci, S. M. Ransom, M. S. E. Roberts, J. W. T. Hessels, A two-solar-mass neutron star measured using Shapiro delay Nature. ,vol. 467, pp. 1081- 1083 ,(2010) , 10.1038/NATURE09466
Natalie A. Webb, Didier Barret, Constraining the Equation of State of Supranuclear Dense Matter from XMM-Newton Observations of Neutron Stars in Globular Clusters The Astrophysical Journal. ,vol. 671, pp. 727- 733 ,(2007) , 10.1086/522877
Tolga Güver, Patricia Wroblewski, Larry Camarota, Feryal Özel, The Mass and Radius of the Neutron Star in 4U 1820-30 arXiv: High Energy Astrophysical Phenomena. ,(2010) , 10.1088/0004-637X/719/2/1807
Andrew W. Steiner, James M. Lattimer, Edward F. Brown, THE EQUATION OF STATE FROM OBSERVED MASSES AND RADII OF NEUTRON STARS The Astrophysical Journal. ,vol. 722, pp. 33- 54 ,(2010) , 10.1088/0004-637X/722/1/33
Steven C. Pieper, V. R. Pandharipande, R. B. Wiringa, J. Carlson, Realistic models of pion-exchange three-nucleon interactions Physical Review C. ,vol. 64, pp. 014001- ,(2001) , 10.1103/PHYSREVC.64.014001
A.W. Steiner, M. Prakash, J.M. Lattimer, P.J. Ellis, Isospin asymmetry in nuclei and neutron stars Physics Reports. ,vol. 411, pp. 325- 375 ,(2005) , 10.1016/J.PHYSREP.2005.02.004
D. V. Shetty, S. J. Yennello, G. A. Souliotis, Density dependence of the symmetry energy and the nuclear equation of state: A dynamical and statistical model perspective Physical Review C. ,vol. 76, pp. 024606- ,(2007) , 10.1103/PHYSREVC.76.024606
K.E. Schmidt, S. Fantoni, A QUANTUM MONTE CARLO METHOD FOR NUCLEON SYSTEMS Physics Letters B. ,vol. 446, pp. 99- 103 ,(1999) , 10.1016/S0370-2693(98)01522-6
S. Gandolfi, F. Pederiva, S. Fantoni, K. E. Schmidt, Auxiliary Field Diffusion Monte Carlo calculation of nuclei with A<40 with tensor interactions Physical Review Letters. ,vol. 99, pp. 022507- ,(2007) , 10.1103/PHYSREVLETT.99.022507
A. Sarsa, S. Fantoni, K. E. Schmidt, F. Pederiva, Neutron matter at zero temperature with an auxiliary field diffusion Monte Carlo method Physical Review C. ,vol. 68, pp. 024308- ,(2003) , 10.1103/PHYSREVC.68.024308