Solar neutrino limit on axions and keV-mass bosons

Details Solar neutrino limit on axions and keV-mass bosons Solar neutrino limit on axions and keV-mass bosons

2008-07-18

arxiv.org/abs/0807.2926v3

Phys.Rev.D79:107301,2009

Astronomy and Astrophysics

Astrophysics

4 pages, 1 figure, version accepted by PRD. Results corrected for erroneous axio-electric and Compton cross sections in the li

Scientific paper

10.1103/PhysRevD.79.107301

The all-flavor solar neutrino flux measured by the Sudbury Neutrino Observatory (SNO) constrains nonstandard energy losses to less than about 10% of the Sun's photon luminosity, superseding a helioseismological argument and providing new limits on the interaction strength of low-mass particles. For the axion-photon coupling strength we find g_a\gamma < 7E-10 1/GeV. We also derive explicit limits on the Yukawa coupling to electrons of pseudoscalar, scalar and vector bosons with keV-scale masses.

Affiliated with

Also associated with

No associations

Rating

Solar neutrino limit on axions and keV-mass bosons 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 Solar neutrino limit on axions and keV-mass bosons, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Solar neutrino limit on axions and keV-mass bosons will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-388279