Explore the mysterious world of dark matter axions and Bose-Einstein Condensation in this comprehensive outline of dark matter caustics, galaxy clusters, cosmic parameters, and the cosmic puzzle. Discussing the Strong CP Problem and the search for dark matter candidates like the axion and WIMP, delve into the intricacies of axion populations, thermalization, and phase space distribution, shedding light on galactic halos, caustic rings, and their impact on rotation curves. Discover how gravitational interactions drive the formation of Bose-Einstein Condensates in dark matter particles, uncovering the secrets of the universe's hidden energy landscapes.
01 / 66Bose-Einstein Condensation of Dark Matter Axions - Understanding the Hidden Universe Secrets
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Bose-Einstein Condensation of Dark Matter Axions - Understanding the Hidden Universe Secrets
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cluster mass Virial Theorem cluster radius velocities of galaxies in the cluster Using the virial theorem, Zwicky (1933) showed that the Coma cluster contains roughly 100 times more mass than accounted for by the luminous matter in the cluster.
Cosmological Parameters -29 3 Age of the universe 13.7 Gigayear Spatial curvature none Energy density 0.95 10 gr/cm Energy fractions vacuum energy atoms and molecules dark matter
The candidates the axion the WIMP the sterile neutrino others
The Strong CP Problem Because the strong interactions conserve P and CP,. The Standard Model does not provide a reason for to be so tiny, but a relatively small modification of the model does provide a reason …
If a symmetry is assumed, relaxes to zero, and a light neutral pseudoscalar particle is predicted: the axion.
Cold axion properties if decoupled number density velocity dispersion phase space density
Bose-Einstein Condensation if identical bosonic particles are highly condensed in phase space and their total number is conserved and they thermalize then most of them go to the lowest energy available state
why do they do that? by yielding their energy to the non-condensed particles, the total entropy is increased. BEC preBEC
Galactic halos have inner caustics as well as outer caustics. If the initial velocity field is dominated by net overall rotation, the inner caustic is a ‘tricusp ring’. If the initial velocity field is irrotational, the inner caustic has a ‘tent-like’ structure. (Arvind Natarajan and PS, 2005).
Galactic halos have inner caustics as well as outer caustics. If the initial velocity field is dominated by net overall rotation, the inner caustic is a ‘tricusp ring’. If the initial velocity field is irrotational, the inner caustic has a ‘tent-like’ structure. (Arvind Natarajan and PS, 2005).
On the basis of the self-similar infall model(Filmore and Goldreich, Bertschinger) with angular momentum (Tkachev, Wang + PS), the caustic rings were predicted to be in the galactic plane with radii was expected for the Milky Way halo from the effect of angular momentum on the inner rotation curve.
Monoceros Ring of stars H. Newberg et al. 2002; B. Yanny et al., 2003; R.A. Ibata et al., 2003; H.J. Rocha-Pinto et al, 2003; J.D. Crane et al., 2003; N.F. Martin et al., 2005 in the Galactic plane at galactocentric distance appears circular, actually seen for scale height of order 1 kpc velocity dispersion of order 20 km/s may be caused by the n = 2 caustic ring of dark matter (A. Natarajan and P.S. ’07)