The Double Pulsar J0737--3039: Testing the Neutron Star Equation of State
ArXiv astro-ph/0506566 (2005)
Abstract:
The double pulsar J0737--3039 has become an important astrophysical laboratory for testing fundamental physics. Here we demonstrate that the low measured mass of Pulsar B can be used to constrain the equation of state of neutron star matter {\em under the assumption} that it formed in an electron-capture supernova. We show that the observed orbital parameters as well as the likely evolutionary history of the system support such a hypothesis and discuss future refinements that will improve the constraints this test may provide.Dipole giant resonances in deformed heavy nuclei
Physical Review C 71 (2005) 064328 pp.8
First Nuclear Moment Measurement with Radioactive Beams by the Recoil-in-Vacuum Technique: The g Factor of the 2+1 State in 132Te,
Physical Review Letters 94 (2005) 192501 pp 4
Structure And Decay Of Neutron‐Rich Nuclides In The 115 ⩽ A ⩽ 138 Mass Range And r‐Process Nucleosynthesis
AIP Conference Proceedings AIP Publishing 764:1 (2005) 335-339
Magnetic Moments of 2+1 States Around 132Sn
Physical Review C 71 (2005) 044317 pp.6