Regularly pulsed neutrinos from supernova SN1987A?

Details Regularly pulsed neutrinos from supernova SN1987A? Regularly pulsed neutrinos from supernova SN1987A?

Aug 1987

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1987natur.328..503h&link_type=abstract

Nature (ISSN 0028-0836), vol. 328, Aug. 6, 1987, p. 503, 504. Research supported by the Alfred P. Sloan Foundation, Alexander vo

Computer Science

10

Neutrinos, Particle Emission, Pulsed Radiation, Stellar Radiation, Supernovae, Anisotropy, Particle Mass

Scientific paper

The neutrino events from SN 1987A observed with the Kamiokande and IMB experiments appear to show evidence of a period (P) of approximately 8.9 milliseconds. While the statistical significance of this period is marginal in each individual experiment, the two sets of data are compatible. The authors remark on a few consequences of interest should the periodicity be confirmed by observations. Interpreting the apparent period P ≈ 8.9 ms as a rotation of a compact object would imply that: (1) neutrino emission is anisotropic; (2) the neutrino mass, averaged over all flavours observed is less than 0.2 eV/(c2.

Affiliated with

Also associated with

No associations

Rating

Regularly pulsed neutrinos from supernova SN1987A? does not yet have a rating. At this time, there are no reviews or comments for this scientific paper.

If you have personal experience with Regularly pulsed neutrinos from supernova SN1987A?, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Regularly pulsed neutrinos from supernova SN1987A? will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1341972