[ExI] LIGO: RE: Hey, look on the bright side
John Clark
johnkclark at gmail.com
Sat Nov 12 00:14:24 UTC 2016
On Thu, Nov 10, 2016 at 11:28 PM, spike <spike66 at att.net> wrote:
>
> >
> Imagine a neutron star of less than Chandrasekhar’s limit, but big. I
> think two solar masses works for this thought experiment. Now imagine you
> are a photon and you originate very nearby, perhaps from a neutron decay or
> something. You head outbound, you get way red-shifted, but go on your
> way. Now imagine two such neutron stars orbiting each other at some
> distance. If you originate between the two and head outbound along an axis
> perpendicular to the line connecting the two (like the axle on your bike
> tire with the two neutron stars on the rim) then you still get away, but
> even more red shift.
>
> OK now imagine bringing the two neutron stars closer together until
> eventually an event horizon envelopes the both of them.
> [...]
> Afterwards the neutron stars move apart toward aphelion
Once the two Neutron stars get close enough to form a event horizon
they're not getting out again and neither is that photon. A Black Hole will
have been formed
with a non spherical horizon which will then vibrate violently and shed
gravitational waves and become spherical in the process. That will take a
second or two.
Chandrasekhar’s limit is 1.44 solar masses
for a non rotating dead star that has run out of internal energy, like
fusion, to push things out and fight against gravity. A neutron star can be
more massive than what Chandrasekhar
says if it is rotating fast enough.
Theory can't yet pinpoint how massive neutron stars can be because we
aren't sure exactly how strong Neutronium
(the stuff neutron stars are made of) is, and if the star spins too fast it
will fly apart, but we know approximately. The limit is somewhere between
2 and 3.5 solar masses. Any more massive than that and that the neutron
star turns into a Black Hole. And theory matches pretty well with
observation. The most massive neutron star ever observed is 1.97
solar
masses and is spinning at 317 revolutions per second. The least massive
Black Hole ever found is 3.8 solar masses.
John K Clark
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