Home
For authors
Submission status

Current
Archive
Archive (English)
   Volumes 21-40
   Volumes 1-20
   Volumes 41-62
      Volume 62
      Volume 61
      Volume 60
      Volume 59
      Volume 58
      Volume 57
      Volume 56
      Volume 55
      Volume 54
      Volume 53
      Volume 52
      Volume 51
      Volume 50
      Volume 49
      Volume 48
      Volume 47
      Volume 46
      Volume 45
      Volume 44
      Volume 43
      Volume 42
      Volume 41
Search
VOLUME 57 (1993) | ISSUE 5 | PAGE 257
Neutrino luminosity of the bubble phase layer in a hot neutron star
A new mechanism of neutrino emission is suggested for a newly born neutron star cooling. Nucleons emit neutrino pairs due to collisions with bubbles which exist inside the spherical layer of stellar matter from half nuclear to nuclear density. During the earliest stages of the nascent neutron star cooling the νμνμ pair luminosity of this rather thin spherical layer is on the order of 1053 ergs/s.