Implications of a non-zero cosmological constant on self-gravitating fermionic systems

Details Implications of a non-zero cosmological constant on self-gravitating fermionic systems Implications of a non-zero cosmological constant on self-gravitating fermionic systems

Mar 1986

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=1986phlb..168..223p&link_type=abstract

Physics Letters B, Volume 168, Issue 3, p. 223-225.

Physics

9

Scientific paper

The modified Thomas-Fermi equation of a degenerate self-gravitating
fermion gas in the presence of a non-vanishing cosmological constant is
studied. A restrictive relation between the mass of the bound cluster
and the value of the cosmological constant is obtained for a given
fermion mass.

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