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 4 | PAGE 195
Measuring the masses of μ and τ neutrinos by detecting neutrinos from collapsing stars with hydrocarbon scintillation detectors
By detecting the neutrino emission from the gravitational collapse of a star by means of low-background underground scintillation detectors one can refine the limit on the ve mass. One can furthermore measure νμ and/or vT by a time-of-flight method or establish ranges on their values at the level of 50-100 eV.