The URCA neutrino loss rate from a hot stellar environment is investigated. The results indicate that the loss rates for URCA type processes from even mass number nuclei are comparable to the rates from odd mass number nuclei at temperatures above about 109 K. Rates are calculated for some typical odd mass isobar pairs and for the even mass isobar fifty-six for temperatures between 5×108 K to 5×1010 K.
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Ashieri, G., Reinieri, M., and Wataghin, G.: 1965,Nuovo Cimento 36, 296.
Beaudet, G., Petrosian, V., and Salpeter, E.: 1967,Astrophys. J. 150, 979.
Chiu, H. Y.: 1961,Ann. Phys. (N.Y.) 15, 1.
Masani, A., Gallino, R., and Silvestro, G.: 1965,Nuovo Cimento 38, 1142.
Pinaev, S.: 1964,Sov. Phys.-JETP. 18, 377.
Stothers, R.: 1970,Phys. Rev. Letters 24, 538.
Tsuruta, S. and Cameron, A.: 1970,Astrophys. Space Sci. 7, 374.
Supported in part by National Science Foundation Grant GP13959.
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McFee, R.W., Schlitt, D.W. The URCA process at high temperatures and densities. Astrophys Space Sci 12, 4–9 (1971). https://doi.org/10.1007/BF00656133
- Loss Rate
- Mass Number
- Type Process
- Number Nucleus
- URCA Process