The astrophysical implications of weakly interacting, massive particles

Details The astrophysical implications of weakly interacting, massive particles The astrophysical implications of weakly interacting, massive particles

Sep 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986phdt.........6s&link_type=abstract

Ph.D. Thesis Harvard Univ., Cambridge, MA.

Computer Science

Elastic Scattering, Halos, Thermal Plasmas, Weak Interactions (Field Theory), Energy Transfer, Leptons, Mesons, Photons, Solar Flux Density

Scientific paper

The possibility is explored that most of the universe is composed of weakly interacting non-baryonic particles. These particles comprise most of the mass of the galaxy's halo. Some of these particles were captured by the Sun in elastic scattering off of nuclei of the Sun. Once inside the Sun, they are very effective at energy transport. They alter the thermal profile of the Sun, thus reconciling the predicted solar neutrino flux with observations. If they exist, these particles could be detected by low temperature detectors.

Affiliated with

Also associated with

No associations

Rating

The astrophysical implications of weakly interacting, massive particles 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 The astrophysical implications of weakly interacting, massive particles, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and The astrophysical implications of weakly interacting, massive particles will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1657834