Gravitational lensing effect due to large-scale structure as a probe of dark matter distribution

Details Gravitational lensing effect due to large-scale structure as a probe of dark matter distribution Gravitational lensing effect due to large-scale structure as a probe of dark matter distribution

Nov 2001

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2001asthe..94..541t&link_type=abstract

The Astronomical Herald (ISSN 0374-2466), Vol. 94, No. 11, p. 541 - 549 (2001)

Mathematics

Logic

Gravitational Lensing, Universe: Large-Scale Structure, Dark Matter, Cosmology

Scientific paper

Gravitational lensing effect due to the large-scale structure of the universe can be a unique method for measuring the dark matter distribution. We have recently investigated the weak lensing effects on temperature fluctuations field in the cosmic microwave background and proposed that the effects can be a method for observationally reconstructing the dark matter power spectrum that is an essential quantity in understanding the structure formation. Here, we discuss the methodology and the cosmological meaning.

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