by M. Reza Tirgan

Created on: July 20, 2011   Last Updated: July 21, 2011

According to HPPH at www.Hparticles.com/, "Dark matter is a form of matter that does not emit light, absorb light, or scatter light. Its only interactions are gravitational"http://www.astro.ucla.edyu/~wright/glossary.html.

The exited H particle-paths due to mass diminution as the subject of, Sec. 5(1)1, Note 5(1)1b, and example 5(1)1,(of the site) may be regarded as dark matter that can produce gravity. "Because dark matter produces gravity, it can produce or enhance the lensing abilities of galaxies or clusters of galaxies in which it resides"[77], Q&A No.154, Note 5(1)2a. According to

http://map.gsfc.nasa.gov/m_uni_101bb2.html

"Dark matter generally refers to exotic non-baryonic matter (WIMPs) that interacts only weakly with ordinary matter. Whereas, no such matter has ever been directly observed in the laboratory, its existence has long been suspected. This form of matter also has no cosmology significant pressure". "WMAP data reveals that Universe contents include 4% atoms, the building blocks of stars and planets. Dark matter comprises 22% of the Universe. This matter, different from atoms, does not emit or absorb light. It has only detected indirectly by its gravity. 74% of the Universe composed of dark energy that acts as assort of an antigravity. This energy distinct from dark matter, is responsible for the present day acceleration of the universe expansion"http://map:gsfc.nasas.gov/m_mm.html, part related to content of the Universe.

Therefore, the ratio of dark energy (related to single direction H particle-paths, Sec. 5(16)7a, Eq. 5(70)8a3 to the sum of dark matter and normal matter [related to counter-current reversible H particle-paths, Sec. 3(1)2, density] is approximately three fold, Remark 5(1)2a, at the present time). Noteworthy, CMB is the single direction H particle-paths moving at c speed individually; whereas, dark matter of configuration from viewpoint of this article is the counter-current H particle-paths at andconfigurations, Sec. 3(1)2, Fig. 3(4) a, b, moving randomly and individually, e.g., super-symmetric models such as neutralinos, Comment 5(1)2b.

 Please refer to Fig. 5(8) of Sec. 5(16)1b, part A, to have an idea in this regards. Therefore, we must seek for dark matter around the macroscopic mass-bodies H system, Remark 5(1)2b, contrary to the CMBR and dark energy, Sec. 5(15)2, that spread all over the Universe and the last two have bosonic H particle-paths nature (Sec. 3(1)2, Fig. 3(4)c, SM configuration).

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