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Non-baryonic dark matter

possible research project (KBN application)

Literature Review (original version by Bartek Lew)

primary objectives

  • Observational possibilities of either direct or indirect detection of cold nonbaryonic dark matter (nbCDM) in the Universe
  • Research for composition, nature and physics of nbCDM in terms of currently favored candidates (WIMP's, Axions, super heavy relicts).
  • Galaxy distribution, dynamics, scattering rates and energy deposit in possible interactions of nbCDM for various candidates
  • Possible observational constraints on nature of nbCDM
  • Possible connection (interaction) between nbCDM and dark energy (DE)
  • Current / future possibilities of relevant nbCDM experiments
  • Some knowledge of standard particle physics and supersymmetric extensions of standard model (MSSM)
  • (Super)Symmetry breaking problems in cosmology and particle physics

secondary objectives

  • Friedmann equations solutions for various cosmological models (see cosmological calculator)
  • Equation of state for different components of the Universe (i.e. nbCDM) and it's influence on cosmological parameters evolution
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\begin{math}\displaystyle {\delta(r) \over \delta_{\mbox{crit}}} = {\delta_c \over (r/r_s) (1+ r/r_s)^2}}\end{math}
This is pdfTeX, Version 3.14159265-2.6-1.40.17 (TeX Live 2016/Debian) (preloaded format=latex)
 restricted \write18 enabled.
entering extended mode
LaTeX2e <2017/01/01> patch level 3
Babel <3.9r> and hyphenation patterns for 30 language(s) loaded.
Document Class: article 2014/09/29 v1.4h Standard LaTeX document class
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[1] (./Ga7jjyhFiv.aux) )
(see the transcript file for additional information)
Output written on Ga7jjyhFiv.dvi (1 page, 700 bytes).
Transcript written on Ga7jjyhFiv.log.
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Topic revision: r4 - 26 Jan 2004, BoudRoukema
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