Naked Science Forum
Non Life Sciences => Physics, Astronomy & Cosmology => Topic started by: syhprum on 01/02/2014 15:15:46
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how quickly would it happen ?, would there be much radiation of photons and neutrinos before the event horizon trapped everything ?.
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A recent supercomputer simulation (http://en.wikipedia.org/wiki/Stellar_collision#Neutron_star_collisions) produced a video of what might happen in a neutron star collision:
- The neutron stars will approach each other as gravitational waves radiate away their angular momentum
- If we had a sensitive-enough gravity-wave telescope, we would see a "chirp" of increasing frequency, as the neutron stars spin around each other, faster and faster.
- The final merger takes around 30ms
- The two neutron stars are distorted as they approach each other; as they touch, they shatter and spray superheated "neutronium" into an accretion disk around them
- Intense magnetic fields can sweep up material from this accretion disk and accelerate it to nearly the speed of light; if we happen to be in line with this jet, we see it as a short gamma ray burst, lasting less than 1 second. It is one of the most intense events in the universe.
- The neutronium in the jet and accretion disk, no longer compressed by the intense gravity of the neutron star will start to decay into protons, electrons and neutrinos; the protons & neutrons will form atomic nuclei, although the temperature will be initially too high to form atoms.
- It is thought that most of the elements heavier than iron are formed in neutron star collisions
- If the combined mass of the two neutron stars exceeds 3-4 times the mass of the Sun, it will collapse into a black hole. Otherwise it will just form a single massive and extremely hot neutron star.
Neutron star collisions will not be a major source of neutrinos, since the majority of matter is already neutrons, and stays in the form of neutrons until it is swallowed by the black hole. Core-collapse supernovae like SN1987a (http://en.wikipedia.org/wiki/SN1987A#Neutrino_emissions) produce more (anti)neutrinos, since a large amount of "normal matter" (protons & electrons) is rapidly crushed into neutrons, releasing an intense blast of antineutrinos.