2 body rotating system in GR

In summary, a 2 body rotating system in General Relativity (GR) refers to a system consisting of two massive bodies, such as stars or black holes, that are in orbit around each other and are also rotating around their own axis. In GR, the motion of the two bodies is affected by the curvature of spacetime caused by their masses, leading to effects such as gravitational waves and orbital precession. These systems have been observed and studied by scientists to further our understanding of the effects of gravity and curvature in GR.
  • #1
I_wonder
9
0
In GR, what is the energy of a system of two identical bodies rotating around their center of mass with regular angular frequency? (assuming such a system is possible). Please take into consideration that I don't know GR at all.

Thanks.
 
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  • #2
Pls Ignore my question, it was based on some misunderstanding.
 
  • #3


In general relativity (GR), the energy of a system of two identical bodies rotating around their center of mass with regular angular frequency is described by the Kerr metric. This metric is a solution to Einstein's field equations and describes the gravitational field around a rotating mass.

The energy of such a system is given by the total mass-energy of the two bodies, as well as the angular momentum of the system. The angular momentum is a measure of how much the bodies are rotating around their center of mass. The more they rotate, the larger the angular momentum and the higher the energy of the system.

It is important to note that the energy of the system is not solely dependent on the masses of the bodies, but also on their distribution of mass and how they are rotating. This is a key aspect of general relativity, as it takes into account the curvature of spacetime caused by the distribution of mass and energy.

In GR, the energy of a system of two rotating bodies would also be affected by the presence of any other nearby masses. This is due to the fact that gravity is not just a force between masses, but rather a curvature of spacetime caused by the presence of mass and energy.

Overall, the energy of a two-body rotating system in GR is a complex and dynamic concept that is affected by various factors such as mass, angular momentum, and the curvature of spacetime. It is a fascinating aspect of general relativity that highlights the intricate relationship between mass, energy, and gravity.
 

1. What is a 2 body rotating system in GR?

A 2 body rotating system in General Relativity (GR) refers to a system consisting of two massive bodies, such as stars or black holes, that are in orbit around each other and are also rotating around their own axis. This system is often used to study the effects of gravity and curvature of spacetime in GR.

2. How is the motion of the two bodies affected by GR?

In GR, the motion of the two bodies is affected by the curvature of spacetime caused by their masses. This curvature causes the bodies to follow geodesic paths, which are the shortest and most natural paths through curved spacetime. This leads to effects such as gravitational waves and orbital precession.

3. Can a 2 body rotating system in GR emit gravitational waves?

Yes, a 2 body rotating system in GR can emit gravitational waves. As the two bodies orbit each other, their motion causes ripples in the fabric of spacetime, which are known as gravitational waves. These waves carry away energy and angular momentum, causing the two bodies to slowly spiral towards each other.

4. How does GR explain the precession of the orbit in a 2 body rotating system?

In GR, the precession of the orbit in a 2 body rotating system is explained by the curvature of spacetime caused by the masses of the two bodies. As the bodies move through this curved spacetime, their orbits are affected by the changing curvature, leading to the observed precession.

5. Are there any real-world examples of a 2 body rotating system in GR?

Yes, there are several real-world examples of 2 body rotating systems in GR, such as binary star systems, neutron star binaries, and black hole binaries. These systems have been observed and studied by scientists to further our understanding of the effects of gravity and curvature in GR.

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