Instruct: Identify the main and secondary category of Arxiv papers based on the titles and abstracts
Query: Cosmological implications of galaxy clusters: best-fit models   The galaxy cluster power spectrum and mass/temperature functions are
currently the most precise observational tools for constraining the theory of
the formation of large scale structure (LSS) in the Universe. Complementing
these tests by the observational data at larger (cosmic microwave backgroud
anisortopy (CMBA)) and smaller (distribution of $Ly_\alpha$ clouds) scales
opens the way to a straightforward determination of the cosmological parameters
in simplest dark matter (DM) models. We argue that such a 'minimal data set' is
free from systematic effects and can indicate quite precisely the parameters of
spatially flat mixed DM model with a positive cosmological constant and no
cosmic gravitational waves.

33
The categories of this paper are: plasm-ph
37
The categories of this paper are: supr-con
4
The categories of this paper are: cond-mat
11
The categories of this paper are: hep-lat
16
The categories of this paper are: stat
7
The categories of this paper are: hep-th
9
The categories of this paper are: nlin
14
The categories of this paper are: math-ph
23
The categories of this paper are: solv-int
21
The categories of this paper are: adap-org
1
The categories of this paper are: cs
15
The categories of this paper are: nucl-ex
32
The categories of this paper are: atom-ph
25
The categories of this paper are: patt-sol
13
The categories of this paper are: quant-ph
35
The categories of this paper are: mtrl-th