Weakly interacting massive particles and stellar structure

Details Weakly interacting massive particles and stellar structure Weakly interacting massive particles and stellar structure

Sep 1989

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1989a%26a...222..103b&link_type=abstract

Astronomy and Astrophysics (ISSN 0004-6361), vol. 222, no. 1-2, Sept. 1989, p. 103-116.

Astronomy and Astrophysics

Astrophysics

6

Elementary Particle Interactions, Globular Clusters, Milky Way Galaxy, Stellar Structure, Weak Energy Interactions, Dark Matter, Energy Transfer, Halos, Particle Mass, Solar Neutrinos

Scientific paper

The existence of weakly interacting massive particles (WIMPs) may solve both the dark matter problem and the solar neutrino problem. Such particles affect the energy transport in the stellar cores and change the stellar structure. The results of an analytic approximation to compute these effects in a self-consistent way are presented. These results can be applied to many different stars, but the decrease of the B-8 neutrino flux in the case of the sun is emphasized.

Affiliated with

Also associated with

No associations

Rating

Weakly interacting massive particles and stellar structure 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 Weakly interacting massive particles and stellar structure, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Weakly interacting massive particles and stellar structure will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-760278