A hydrogenic molecular atmosphere of a neutron star

Modern Physics Letters A

Volumn 19, Issue 25, 2004, Pages 1919-1923

  Turbiner, A V ^a,b   Lopez Vieyra J C ^a  

^a INSTITUTO DE CIENCIAS NUCLEARES   (Mexico)

^b INSTITUTE FOR THEORETICAL AND EXPERIMENTAL PHYSICS   (Russian Federation)

Author keywords

Exotic molecular matter; Neutron star atmosphere; Strong magnetic field

Indexed keywords

HYDROGEN;

ARTICLE; ATMOSPHERE; CALCULATION; DISSOCIATION; ELECTRON; ENERGY; IONIZATION; MAGNETIC FIELD; MODEL; NEUTRON;

EID: 4143120070     PISSN: 02177323     EISSN: None     Source Type: Journal    
DOI: 10.1142/S0217732304015294     Document Type: Article

References (24)

1. D. Sanwal et al., Ap. J. 574, L61 (2002).
2. C. J. Hailey and K. Mori, Ap. J. 578, L133 (2002); K. Mori and C. J. Hailey, "X-ray spectroscopy of the isolated neutron star 1E1207.4-5209: atmospheric composition and equation of state", astro-ph/0301161.
3. C. J. Hailey and K. Mori, Ap. J. 578, L133 (2002); K. Mori and C. J. Hailey, "X-ray spectroscopy of the isolated neutron star 1E1207.4-5209: atmospheric composition and equation of state", astro-ph/0301161.
4. B. B. Kadomtsev and V. S. Kudryavtsev, Pis'ma ZhETF 13, 15; 61 (1971); Sov. Phys. - JETP Lett. 13, 9; 42 (1971) (English translation); ZhETF 62, 144 (1972); Sov. Phys. - JETP Lett. 35, 76 (1972) (English translation).
5. B. B. Kadomtsev and V. S. Kudryavtsev, Pis'ma ZhETF 13, 15; 61 (1971); Sov. Phys. - JETP Lett. 13, 9; 42 (1971) (English translation); ZhETF 62, 144 (1972); Sov. Phys. - JETP Lett. 35, 76 (1972) (English translation).
6. B. B. Kadomtsev and V. S. Kudryavtsev, Pis'ma ZhETF 13, 15; 61 (1971); Sov. Phys. - JETP Lett. 13, 9; 42 (1971) (English translation); ZhETF 62, 144 (1972); Sov. Phys. - JETP Lett. 35, 76 (1972) (English translation).
7. B. B. Kadomtsev and V. S. Kudryavtsev, Pis'ma ZhETF 13, 15; 61 (1971); Sov. Phys. - JETP Lett. 13, 9; 42 (1971) (English translation); ZhETF 62, 144 (1972); Sov. Phys. - JETP Lett. 35, 76 (1972) (English translation).
8. B. B. Kadomtsev and V. S. Kudryavtsev, Pis'ma ZhETF 13, 15; 61 (1971); Sov. Phys. - JETP Lett. 13, 9; 42 (1971) (English translation); ZhETF 62, 144 (1972); Sov. Phys. - JETP Lett. 35, 76 (1972) (English translation).
9. B. B. Kadomtsev and V. S. Kudryavtsev, Pis'ma ZhETF 13, 15; 61 (1971); Sov. Phys. - JETP Lett. 13, 9; 42 (1971) (English translation); ZhETF 62, 144 (1972); Sov. Phys. - JETP Lett. 35, 76 (1972) (English translation).
10. M. Ruderman, Phys. Rev. Lett. 27, 1306 (1971); in IAU Symp. 53, Physics of Dense Matter, ed. C. J. Hansen (Reidel, 1974), p. 117.
11. M. Ruderman, Phys. Rev. Lett. 27, 1306 (1971); in IAU Symp. 53, Physics of Dense Matter, ed. C. J. Hansen (Reidel, 1974), p. 117.
12. Yu. P. Kravchenko, M. A. Liberman and B. Johansson, Phys. Rev. A54, 287 (1996).
13. A. Y. Potekhin and A. V. Turbiner, Phys. Rev. A63, 065402 (2001).
14. 2+ in a strong magnetic field. Linear configuration, in progress.
15. 2+ in a strong magnetic field. Linear configuration, in progress.
16. 2+ in a strong magnetic field. Linear configuration, in progress.
17. 2+ in a strong magnetic field. Linear configuration, in progress.
18. 2+ in a strong magnetic field. Linear configuration, in progress.
19. 2+ in a strong magnetic field. Linear configuration, in progress.
20. 2+ in a strong magnetic field. Linear configuration, in progress.
21. M. A. Liberman and B. Johansson, Phys. Usp. 38, 117 (1995).
22. D. Lai, Rev. Mod. Phys. 73, 629 (2001).
23. A. Y. Potekhin and G. Chabrier, Ap. J. 600, 317 (2004).
24. G. F. Bignami, P. A. Caraveo, A De Luca and S. Mereghetti, Nature 423, 725 (2003).