https://www.selleckchem.com/products/BEZ235.html
If the heavier component of GW190412 is indeed a merger remnant, then its spin magnitude is χ_1=0.56_-0.21^+0.19, which is higher than the value previously reported by the LIGO/Virgo collaboration.On May 21, 2019 at 030229 UTC Advanced LIGO and Advanced Virgo observed a short duration gravitational-wave signal, GW190521, with a three-detector network signal-to-noise ratio of 14.7, and an estimated false-alarm rate of 1 in 4900 yr using a search sensitive to generic transients. If GW190521 is from a quasicircular binary inspiral, then the
Like
Comment
Share
