2017
DOI: 10.4236/jmp.2017.82018
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Astrophysics and Dark Matter Theory

Abstract: Space-Time Quantization implies that the cosmic dark matter gas is subjected to pressure effects. We prove this by accounting for the mass-density distribution of dark matter in galactic halos. It can be directly deduced from observed rotation curves and coincides with theoretical predictions for dark matter atmospheres in hydrostatic equilibrium. Through embedding, the pressure of the cosmic dark matter gas prevents also the gravitational collapse of the Oort cloud, globular star clusters and cosmic filaments… Show more

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Cited by 4 publications
(9 citation statements)
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“…Their average kinetic energy would be 3 2 kT w kT mc = . These concepts are confirmed by astrophysical observations [7], which proved that the cosmic DM gas is cold. We mentioned in the introduction that the CDM Λ implies that 1 w = − , but DM particles interact with one another.…”
Section: The Conventional Dm and De Modelsupporting
confidence: 55%
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“…Their average kinetic energy would be 3 2 kT w kT mc = . These concepts are confirmed by astrophysical observations [7], which proved that the cosmic DM gas is cold. We mentioned in the introduction that the CDM Λ implies that 1 w = − , but DM particles interact with one another.…”
Section: The Conventional Dm and De Modelsupporting
confidence: 55%
“…Moreover, it is sufficient that 0 a ≠ , to justify the Standard Model and to complete it in regard to DM particles [5] [6]. Predicted properties of the cosmic DM gas are confirmed by astrophysical observations [7]. Here, we examine other consequences, especially for the accelerated expansion of space and Big Bang processes.…”
Section: Introductionmentioning
confidence: 82%
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“…Because of their mass, DM particles are also subjected to gravitational forces. This accounts for many astrophysical observations [13].…”
Section: Interactions Between Dm Particlesmentioning
confidence: 57%
“…Astrophysical evidence indicates also that interactions between cosmic DM and baryonic matter are negligible and so far, even the most sensitive DM detector did not yield any evidence of interactions between DM particles and nucleons [22]. However, we will show that DM particles can interact with electrons [13].…”
Section: Direct Detection or Productionmentioning
confidence: 62%