Simulation of cosmological stochastic background in LISA

Details Simulation of cosmological stochastic background in LISA Simulation of cosmological stochastic background in LISA

Mar 2009

adsabs.harvard.edu/cgi-bin/nph-data_query?bibcode=2009jphcs.154a2046b&link_type=abstract

Journal of Physics: Conference Series, Volume 154, Issue 1, pp. 012046 (2009).

Physics

Scientific paper

A pilot study has been carried out to simulate stochastic gravitational wave background originating from first order phase transitions in the early universe. The space based gravitational wave detector LISA will be operational in the range of 10-4 to 0.1 Hz and could be sensitive to the red shifted gravitational waves from cosmological origin. In this study we have modeled the signals from first order phase transitions and we compared the signal both with the expected instrumental noise and realistic simulated foreground signals, originating from the white dwarf population in our galaxy.

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