Want this question answered?
A neutron star is so dense, that apart from a direct collision from another neutron star, the chances are slim to impossible.
No. A neutron star is left behind after a supernova. However, some gamma ray bursts may result from a collision between neutron stars.
It is not actually on any of their cds because it was made specifically for the Twilight: Eclipse Soundtrack.
The neutron is called the neutron because it it electrically neutral, hence the neu- prefix
A neutron does not have a charge -- its neutral
Neutron Star Collision (Love Is Forever) came out on May 17th 2010.
A neutron star is so dense, that apart from a direct collision from another neutron star, the chances are slim to impossible.
aids
neutron star collision (love is forever)
No. A neutron star is left behind after a supernova. However, some gamma ray bursts may result from a collision between neutron stars.
It was released on 17 May 2010.
That would be a collission between two neutron stars. Since many stars are actually double stars, this can happen now and then.
Femi Gamma Ray Telescope
It is not actually on any of their cds because it was made specifically for the Twilight: Eclipse Soundtrack.
No but "Neutron Star Collision (Love Is Forever)", "I Belong to You" and "Supermassive Black Hole" all by Muse are :)
Elastic collision deceleration is the transfer of energy from an accelerated body to another one that results in the deceleration of the first body by some degree. An example might be the elastic collision and deceleration of, say, a neutron in a nuclear reactor. When a fission event occurs, a neutron leaving the scene will be moving like a bullet from a gun. As the neutron doesn't have a charge, it cannot slow by anything other than elastic scattering, a collision with something. It needs to transfer some energy into whatever it hits to slow down. If it slams into the nucleus of, say, an iron atom, that's not so good. (Iron is the major component in steel, which the reactor vessel is made out of.) The iron nucleus is over 50 times as massive, and the neutron can't give it much energy to slow down. That'd be like trying to slow a high speed golf ball down by having it slam into, say, a bowling ball. Not the best thing in the west if we want to slow the golf ball down. (We do need to slow the neutron down in the reactor, by the way.) So what can we use to slow down a neutron? Let's see. We need something near its own size. How about a proton? Like the protons in hydrogen nuclei in water molecules? Oooo, snap! We use water as the heat transfer medium in our reactor and it does double duty as the moderator, or "slower-downer" of neutrons. An elastic scattering deceleration event occurs when a neutron slams into a proton. The proton is knocked across the room and the neutron comes away with less energy. The neutron is said to have decelerated in an elastic scattering event. The slowing neutron is moving to a lower energy state. Toward a state of thermal energy. It is being thermalized. It's slowing down in a thermonuclear reactor. As Paul Harvey would say, and now you know the rest of the story....
nuetron star collision is a song written by muse. it was released in 2010 and was written by Matthew Bellamy, muse frontman, about his ex-girlfriend and how he felt about her when they first got together.