Corpus ID: 237605355

Dynamic model of a non-equilibrium chemical composition formation in the shell of single neutron stars

@inproceedings{Ignatovskiy2021DynamicMO,
  title={Dynamic model of a non-equilibrium chemical composition formation in the shell of single neutron stars},
  author={A. Yu. Ignatovskiy and Gennadiy Bisnovatyi-Kogan},
  year={2021}
}
The process of a non-equilibrium chemical composition formation in the crust of a new born neutron star is considered, during cooling due to neutrino energy losses. A model is constructed for explaining accumulation of a large quantity of nuclear energy, which can maintain the X-ray luminosity of such compact objects for a long period of time. We studied numerically the dependence of the final chemical composition on various parameters of the model. 

References

SHOWING 1-7 OF 7 REFERENCES
Atomic Data and Nuclear Data Tables
a b s t r a c t The ab initio quasirelativistic Hartree–Fock method developed specifically for the calculation of spectral parameters of heavy atoms and highly charged ions is used to deriveExpand
Nuclear Physics
TLDR
The rapid development of the knowledge of artificial radioactivity and in particular the production of such radioactivity by neutron bombardment is discussed. Expand
"J."
however (for it was the literal soul of the life of the Redeemer, John xv. io), is the peculiar token of fellowship with the Redeemer. That love to God (what is meant here is not God’s love to men)Expand
Theoretical Physics : Statistical Physics Part 1
  • 2002
Prog
  • Theor. Phys. 62, 957
  • 1979
Nadezhin, V.M.Chechetkin, Astrophysics and Space
  • Science, 35,
  • 1975
JETP
  • 42, 875
  • 1962