Observational Evidences of Non-baryonic (non-compact) Microlenses

Details Observational Evidences of Non-baryonic (non-compact) Microlenses Observational Evidences of Non-baryonic (non-compact) Microlenses

Dec 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998tx19.confe.293z&link_type=abstract

Abstracts of the 19th Texas Symposium on Relativistic Astrophysics and Cosmology, held in Paris, France, Dec. 14-18, 1998. Eds.:

Astronomy and Astrophysics

Astrophysics

Scientific paper

It is well-known that most reliable cosmological models need the non-baryonic dark matter existence. The very interesting possibility of the non-baryonic dark matter existence was considered recently by Gurevich et al. They proved that the non-baryonic (non-compact) objects as neutralino stars may be stable during cosmological timescales. The neutralino star radius could be about few Einstein radii. On the other hand, now we have no direct evidences of the fact that microlensing is caused by compact baryonic objects such as brown, red or cold white dwarfs. Using most precise model of a density distribution, I discuss how it could be possible to distinguish the compact (baryonic) and non-compact (non-baryonic) microlensing using light curves, polarization curves etc, therefore, possibly to find the non-baryonic dark matter.

Affiliated with

Also associated with

No associations

Rating

Observational Evidences of Non-baryonic (non-compact) Microlenses 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 Observational Evidences of Non-baryonic (non-compact) Microlenses, we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Observational Evidences of Non-baryonic (non-compact) Microlenses will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-768323