Extragalactic neutrino background from PBHs evaporation

Astronomy and Astrophysics – Astrophysics

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

18pages + 9figures

Scientific paper

We calculated the energy spectra and the fluxes of electron neutrinos in extragalactic space emitted in the process of the evaporation of primordial black holes (PBHs) in the early universe. It was assumed that PBHs are formed by a blue power-law spectrum of primordial density fluctuations. In the calculations of neutrino spectra the spectral index of density fluctuations and the reheating temperature were used as free parameters. The absorption of neutrinos during propagation in the space was taken into account. We obtained the bounds on the spectral index assuming validity of the standard picture of gravitational collapse and using the available data of several experiments with atmospheric and solar neutrinos. The comparison of our results with the previous constraints (which had been obtained using diffuse photon background data) shows that such bounds are quite sensitive to an assumed form of the initial PBH mass function.

No associations

LandOfFree

Say what you really think

Search LandOfFree.com for scientists and scientific papers. Rate them and share your experience with other people.

Rating

Extragalactic neutrino background from PBHs evaporation 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 Extragalactic neutrino background from PBHs evaporation, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Extragalactic neutrino background from PBHs evaporation will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-638980

  Search
All data on this website is collected from public sources. Our data reflects the most accurate information available at the time of publication.