Microkelvin Variations in the Blackbody Radiation of Our Vacuum Space Region to Distinguish Radiation of Stars and Galaxies from that of Remote Regions of Vacuum Space.

Details Microkelvin Variations in the Blackbody Radiation of Our Vacuum Space Region to Distinguish Radiation of Stars and Galaxies from that of Remote Regions of Vacuum Space. Microkelvin Variations in the Blackbody Radiation of Our Vacuum Space Region to Distinguish Radiation of Stars and Galaxies from that of Remote Regions of Vacuum Space.

Apr 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998aps..apr..d308s&link_type=abstract

American Physical Society, APS/AAPT Joint April Meeting, April 18-21, 1998 Columbus, Ohio, abstract #D3.08

Mathematics

Probability

Scientific paper

The probability P of observing a "hot spot" in space is roughly proportional to its volume V. V is proportional to the instrument's "field of view" area A, multiplied by the supposed depth Δ f of the bulk. Clearly, the uncertain value of Δ f increases with distance d to the bulk under observation, and A is roughly proportional to d^2, so that P increases very fast with growing distance d. The number of "hot spots", seen in the field of view, increases therefore very fast with increasing "penetration depth" of the instrument, e.g., of the Hubble telescope. The hot spots are presented to the public (and to NASA) as galaxies and stars, but they may just as well represent hot regions of the electron positron lattice (epola) space.(M.Simhony, The Epola Space, 1990, 160 pp, and The Story of Matter and Space, 1998, 70 pp (available from the author). Also, M.Simhony, Invitation to the Natural Physics of Matter, Space, and Radiation, World Scientific, 1994 (292 pp).) The microK variations in the 3K blackbody radiation are considered as possible means to distinguish radiation of remote extragalaxial hot epola regions from that of real galaxies and stars.

Affiliated with

Also associated with

No associations

Rating

Microkelvin Variations in the Blackbody Radiation of Our Vacuum Space Region to Distinguish Radiation of Stars and Galaxies from that of Remote Regions of Vacuum Space. 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 Microkelvin Variations in the Blackbody Radiation of Our Vacuum Space Region to Distinguish Radiation of Stars and Galaxies from that of Remote Regions of Vacuum Space., we encourage you to share that experience with our LandOfFree.com community. Your opinion is very important and Microkelvin Variations in the Blackbody Radiation of Our Vacuum Space Region to Distinguish Radiation of Stars and Galaxies from that of Remote Regions of Vacuum Space. will most certainly appreciate the feedback.

Rate now

Comments { 0 }

Profile ID: LFWR-SCP-O-1602996