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Ultra low Frequency Gravitational Waves


tex2html_wrap_inline3922   Each line of sight to a pulsar is analogous to one arm of LIGO, GEO or LISA.

tex2html_wrap_inline3922   Constrain energy density tex2html_wrap_inline16232 of Gravitational Waves of frequency = 1/data span, ie tex2html_wrap_inline16234 Hz.

Assuming tex2html_wrap_inline16236 kms tex2html_wrap_inline16238 Mpc tex2html_wrap_inline16238
tex2html_wrap_inline3922   tex2html_wrap_inline16244 - Kaspi et al 1994

Jon Bell
Thu Dec 19 15:15:11 GMT 1996