scholarly journals Flux-Vortex Pinning and Neutron Star Evolution

2017 ◽  
Vol 38 (3) ◽  
Author(s):  
M. Ali Alpar
Keyword(s):  
Neutron Star ◽  
Vortex Pinning ◽  
Star Evolution

scholarly journals MAGNETO-ROTATIONAL NEUTRON STAR EVOLUTION: THE ROLE OF CORE VORTEX PINNING

2011 ◽  
Vol 740 (2) ◽  
pp. L35 ◽  
Author(s):  
Kostas Glampedakis ◽  
Nils Andersson
Keyword(s):  
Neutron Star ◽  
Vortex Pinning ◽  
Star Evolution

scholarly journals Neutron star masses

2012 ◽  
Vol 8 (S291) ◽  
pp. 146-146
Author(s):  
David Nice
Keyword(s):  
Neutron Star ◽  
Equation Of State ◽  
Nuclear Matter ◽  
Observational Data ◽  
Mass Distribution ◽  
Binary Star ◽  
Star Mass ◽  
Star Evolution ◽  
Neutron Star Mass ◽  
Present Understanding

AbstractNeutron star masses can be inferred from observations of binary pulsar systems, particularly by the measurement of relativistic phenomena within these orbits. The observed distribution of masses can be used to infer or constrain the equation of state for nuclear matter and to study astrophysical processes such as supernovae and binary star evolution. In this talk, I will review our present understanding of the neutron star mass distribution with an emphasis on the observational data.

scholarly journals Neutrino signal from proto-neutron star evolution: Effects of opacities from charged-current–neutrino interactions and inverse neutron decay

2020 ◽  
Vol 101 (2) ◽  
Author(s):  
Tobias Fischer ◽  
Gang Guo ◽  
Alan A. Dzhioev ◽  
Gabriel Martínez-Pinedo ◽  
Meng-Ru Wu ◽  
...  
Keyword(s):  
Neutron Star ◽  
Neutron Decay ◽  
Charged Current ◽  
Neutrino Interactions ◽  
Star Evolution ◽  
Proto Neutron Star

Supernova Fallback and Neutron Star Evolution

2002 ◽  
Vol 579 (1) ◽  
pp. L37-L40 ◽  
Author(s):  
Xiang-Dong Li
Keyword(s):  
Neutron Star ◽  
Star Evolution

scholarly journals A possible way to reconcile long-period precession with vortex pinning in neutron stars

2018 ◽  
Vol 482 (3) ◽  
pp. 3032-3044 ◽  
Author(s):  
O A Goglichidze ◽  
D P Barsukov
Keyword(s):  
Neutron Star ◽  
Neutron Stars ◽  
Vortex Pinning ◽  
Component Model ◽  
Observation Data ◽  
Interaction Coefficients ◽  
Long Period

ABSTRACT We propose a possible way to solve the problem of inconsistency between the neutron star long-period precession and superfluid vortex pinning, which is the basis of the most successful theories of pulsar glitches. We assume that the pinning takes place in the region of the neutron star core, which, being magnetically decoupled, can rotate relative to the crust. In the framework of a simple three-component model we show that these two phenomena can coexist in the same pulsar. Some constraints on the formally introduced interaction coefficients following from observation data are formulated.

Neutron star evolution with internal heating

1989 ◽  
Vol 346 ◽  
pp. 808 ◽  
Author(s):  
Noriaki Shibazaki ◽  
Frederick K. Lamb
Keyword(s):  
Neutron Star ◽  
Internal Heating ◽  
Star Evolution

Neutron star evolution and results from the Einstein X-ray Observatory

1981 ◽  
Vol 244 ◽  
pp. L13 ◽  
Author(s):  
K. A. van Riper ◽  
D. Q. Lamb
Keyword(s):  
Neutron Star ◽  
X Ray ◽  
Star Evolution
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