[seminar] Nevenko Bilic, 03. prosinca 2010. (srijeda) u 15:00 c.t., IRB, predavaona I krila

Hrvoje Nikolic hrvoje at thphys.irb.hr
Wed Nov 24 15:25:19 CET 2010



       INSTITUT Ruđer Bošković
       ZAVOD ZA TEORIJSKU FIZIKU
       Bijenička c. 54, Zagreb, Hrvatska


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                      SEMINAR ZAVODA ZA TEORIJSKU  FIZIKU
             (Zajednički seminari Zavoda za teorijsku fiziku i
 		Zavoda za eksperimentalnu fiziku IRB-a i
 		Zavoda za teorijsku fiziku PMF-a)

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  	Nevenko Bilic, Institut Rudjer Boskovic


     "Dark Matter in Galaxies"

       Vrijeme:  03. prosinca 2010. (petak), 15.00, c.t.

       Mjesto:  Institut Rudjer Boskovic, predavaona I krila

       Sazetak:
The distribution of matter in galaxies of different luminosities and
Hubble types, as inferred from observations, plays an important role in
cosmology, extragalactic astrophysics, astroparticle physics, as well as
in a number of issues in high-energy astrophysics, galactic astronomy,
star formation and evolution and general relativity. Notwithstanding the
general successes of the LambdaCDM scenario in explaining the structure
and evolution of the universe, there is a growing conviction that the
structural properties of the dark and luminous components in galaxies
hold important clues about the nature of dark matter and the processes
that are responsible for galaxy formation.
The overall purpose of this seminar is to increase the awareness of the
phenomenology of the mass discrepancy problem in galaxies amongst the
scientists currently working with a theoretical, observational,
experimental and simulation approach on issues involving dark matter or
its alternatives.



      Voditelj seminara:
      Hrvoje Nikolic (hrvoje at thphys.irb.hr)


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