scholarly journals Electron capture reactions in neutron star crusts: deep heating and observational constraints

2010 ◽  
Author(s):  
Edward Brown ◽  
Sanjib S. Gupta ◽  
Hendrik Schatz ◽  
Peter Möller ◽  
Karl Ludwig Kratz
Keyword(s):  
Neutron Star ◽  
Electron Capture ◽  
Observational Constraints

scholarly journals Observational Constraints on the Surface Gravitational Redshift of a Neutron Star

2017 ◽  
Author(s):  
Masachika Iwai ◽  
Tadayasu Dotani ◽  
Masanobu Ozaki ◽  
Yoshitomo Maeda ◽  
Hideyuki Mori ◽  
...  
Keyword(s):  
Neutron Star ◽  
Gravitational Redshift ◽  
Observational Constraints

scholarly journals Strong neutrino cooling by cycles of electron capture and β− decay in neutron star crusts

Nature ◽  
2013 ◽  
Vol 505 (7481) ◽  
pp. 62-65 ◽  
Author(s):  
H. Schatz ◽  
S. Gupta ◽  
P. Möller ◽  
M. Beard ◽  
E. F. Brown ◽  
...  
Keyword(s):  
Neutron Star ◽  
Electron Capture ◽  
Β Decay

scholarly journals Mass measurements of neutron rich isotopes in the Fe region and electron capture processes in neutron star crusts

2011 ◽  
Author(s):  
Alfredo Estrade ◽  
Milan Matos ◽  
Hendrik Schatz ◽  
Matthew Amthor ◽  
Mary Beard ◽  
...  
Keyword(s):  
Neutron Star ◽  
Electron Capture ◽  
Mass Measurements ◽  
Neutron Rich Isotopes

scholarly journals Neutron star cooling: theoretical aspects and observational constraints

2004 ◽  
Vol 33 (4) ◽  
pp. 523-530 ◽  
Author(s):  
D.G Yakovlev ◽  
O.Y Gnedin ◽  
A.D Kaminker ◽  
K.P Levenfish ◽  
A.Y Potekhin
Keyword(s):  
Neutron Star ◽  
Observational Constraints ◽  
Neutron Star Cooling

scholarly journals X-Ray Bursts of Nuclear Origin?

1977 ◽  
Vol 4 (1) ◽  
pp. 127-128 ◽  
Author(s):  
L. Maraschi ◽  
A. Cavaliere
Keyword(s):  
Neutron Star ◽  
Nuclear Energy ◽  
Observational Constraints ◽  
X Ray ◽  
Thermonuclear Reactions ◽  
Cold Star ◽  
Pycnonuclear Reactions

The fate of nuclear energy carried by matter accreted onto a neutron star was considered e.g. by Rosenbluth et al. (1973). They examined pycnonuclear reactions on an originally cold star, and found that the whole star is thereby heated up to 106−107 °K. The thermonuclear reactions that can be ignited then, have been studied by Hansen and Van Horn (1975), who computed stationary burning shells, finding, however, that in most cases the shells are thermally unstable.We consider here the possibility that X-ray bursts are due to instabilities of this type. The observational constraints fix the parameters uniquely.

scholarly journals Electron capture rates for neutron star crusts

2010 ◽  
Author(s):  
Ana Delia Becerril Reyes ◽  
Sanjib S. Gupta ◽  
Hendrik Schatz ◽  
Karl Ludwig Kratz ◽  
Peter Möller
Keyword(s):  
Neutron Star ◽  
Electron Capture ◽  
Capture Rates
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