Can Spectroscopy Provide Means to Distinguish the Thermal Radiation of Extended Atomic Bodies from that of "Vacuum Space"?

Details Can Spectroscopy Provide Means to Distinguish the Thermal Radiation of Extended Atomic Bodies from that of "Vacuum Space"? Can Spectroscopy Provide Means to Distinguish the Thermal Radiation of Extended Atomic Bodies from that of "Vacuum Space"?

Mar 1998

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1998aps..mar.i3896s&link_type=abstract

American Physical Society, Annual March Meeting, March 16-20, 1998 Los Angeles, CA, abstract #I38.96

Mathematics

Probability

Scientific paper

Assuming a more or less uniform distribution of mass and energy in "vacuum space", one finds that the probability P of observing a "hot spot" in space should be proportional to the volume V of the bulk of space, onto which our optical instrument is "focused". The volume V is proportional to the "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).) It is therefore imperative to discuss and work out spectroscopic and other means that distinguish between hot epola regions and real galaxies and stars.

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