scholarly journals Pycnonuclear reactions and nova explosions.

1959 ◽  
Vol 64 ◽  
pp. 325
Author(s):  
A. G. W. Cameron
Keyword(s):  
Pycnonuclear Reactions

scholarly journals PYCNONUCLEAR REACTIONS

1980 ◽  
Vol 41 (C2) ◽  
pp. C2-87-C2-87 ◽  
Author(s):  
A. Alastuey ◽  
B. Jancovici
Keyword(s):  
Pycnonuclear Reactions

Pycnonuclear reactions and the nature of supranuclear matter

2003 ◽  
Vol 43 (56) ◽  
pp. 390-392 ◽  
Author(s):  
D. G. Yakovlev ◽  
K. P. Levenfish
Keyword(s):  
Pycnonuclear Reactions

Enhanced Pycnonuclear Reactions in Ultrahigh-Pressure Metals

1995 ◽  
Vol 64 (7) ◽  
pp. 2270-2273 ◽  
Author(s):  
Setsuo Ichimaru ◽  
Hikaru Kitamura
Keyword(s):  
Ultrahigh Pressure ◽  
Pycnonuclear Reactions

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 Pycnonuclear reactions in dense stellar matter

2005 ◽  
Vol 25 (S1) ◽  
pp. 669-672 ◽  
Author(s):  
D. G. Yakovlev ◽  
K. P. Levenfish ◽  
O. Y. Gnedin
Keyword(s):  
Stellar Matter ◽  
Pycnonuclear Reactions
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