next up previous
Next: Constancy of the Chandrasekhar Up: Binary Neutron Stars Previous: Strong v Weak tests

Variations in G

  (Damour, Gibbons & Taylor 1988)

equation863

tex2html_wrap_inline3922   Assuming GR is correct (Taylor 1993)
tex2html_wrap_inline16216 (PSR B1913+16)

tex2html_wrap_inline3922   No Assumptions about GR (Kaspi et al 1994)
tex2html_wrap_inline16220 (PSR B1855+09)

tex2html_wrap_inline3922   Both assume a hard equation of state



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