Direct computation of inelastic photon-neutrino processes in the Standard Model

Physics – High Energy Physics – High Energy Physics - Phenomenology

Scientific paper

Rate now

  [ 0.00 ] – not rated yet Voters 0   Comments 0

Details

19 pages, 3 Postscript figures, uses axodraw.sty

Scientific paper

10.1016/S0550-3213(98)00790-1

In this paper, we compute the Standard Model polarized amplitudes and cross sections of the processes $\gamma\nu\to\gamma\gamma \nu$, $\gamma\gamma \to \gamma\nu\bar\nu$ and $\nu\bar\nu \to \gamma\gamma\gamma$, for centre-of-mass energies $\omega$ within the range of validity of the Fermi theory. By using a large electron-mass expansion of the exact result, we also derive the first correction term to the effective, low-energy ($\omega < m_e$) formula for $\gamma\nu\to\gamma\gamma \nu$. Finally, we discuss possible astrophysical implications of our results and provide simple fits to the exact expressions.

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

Direct computation of inelastic photon-neutrino processes in the Standard Model 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 Direct computation of inelastic photon-neutrino processes in the Standard Model, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Direct computation of inelastic photon-neutrino processes in the Standard Model will most certainly appreciate the feedback.

Rate now

     

Profile ID: LFWR-SCP-O-389416

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