Orbital period decay and gravitational waves

In summary: But when it comes to changes that involve a lot of matter moving around, like the binary star system, the gravity wave emission can be quite significant.The basic idea of how gravity waves are produced is this: Imagine you have some configuration of matter. We could be talking about a solar system, or a galaxy, or just an amorphous blob of dust. The specific bit of matter we're considering is irrelevant.Now, this bit of matter undergoes a change, for whatever reason (say, a large collision, such as between two black holes). It is impossible for a change in the configuration of this matter to propagate faster than light, and so the gravitational field away from the bit of
  • #1
Ranku
410
18
We know that the orbital period of binary stars decay due to the emission of gravity waves that carry away energy from the system. What is the form of the energy loss of the system: kinetic energy or potential energy?
 
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  • #2
Ranku said:
We know that the orbital period of binary stars decay due to the emission of gravity waves that carry away energy from the system. What is the form of the energy loss of the system: kinetic energy or potential energy?
It's a combination of the two. The potential energy becomes more negative, while the kinetic energy increases.
 
  • #3
Chalnoth said:
It's a combination of the two. The potential energy becomes more negative, while the kinetic energy increases.

Can we discern potential and kinetic energy components in the gravitational waves themselves?
When gravitational waves impact an object, say a dust sphere, the effect is not gravitational. That would seem to suggest there is no potential energy component in the gravitational waves themselves, even though the energy loss of the source of gravitational waves may well be a combination of potential and kinetic energy.
 
  • #4
Ranku said:
Can we discern potential and kinetic energy components in the gravitational waves themselves?
I'm not sure that question makes a whole lot of sense. The essential thing is that they transport energy away from the binary system, and can, in principle, deposit that energy elsewhere.

Ranku said:
When gravitational waves impact an object, say a dust sphere, the effect is not gravitational.
What do you mean the effect is not gravitational?
 
  • #5
Chalnoth said:
What do you mean the effect is not gravitational?

When gravitational waves impact a dust sphere, it alternately ellipses in perpendicular directions transverse to the direction of the waves. Gravitational waves do not cause gravitational motion of the dust sphere toward the source of the gravity waves.

Indeed not only are gravity waves not gravitational, primordial gravity waves could actually be repulsive! http://arxiv.org/abs/0909.1922v1
 
  • #6
Ranku said:
When gravitational waves impact a dust sphere, it alternately ellipses in perpendicular directions transverse to the direction of the waves. Gravitational waves do not cause gravitational motion of the dust sphere toward the source of the gravity waves.

Indeed not only are gravity waves not gravitational, primordial gravity waves could actually be repulsive! http://arxiv.org/abs/0909.1922v1
That's not a statement that they're not gravitational. I don't think anybody who studied General Relativity would even begin to think that gravity waves should cause matter to be attracted to a source.

Gravity waves are basically ripples in the fabric of space-time. Part of the gravity wave will be space-time that is sort of squeezed, while another part will be sort of stretched. There is no net curvature to a gravity wave. They're still gravitational in the sense that they are gravity acting on matter. It's just not in an overly-simplistic way.

The basic idea of how gravity waves are produced is this:
Imagine you have some configuration of matter. We could be talking about a solar system, or a galaxy, or just an amorphous blob of dust. The specific bit of matter we're considering is irrelevant.

Now, this bit of matter undergoes a change, for whatever reason (say, a large collision, such as between two black holes). It is impossible for a change in the configuration of this matter to propagate faster than light, and so the gravitational field away from the bit of matter cannot respond instantly to the change. What happens is that the effect of the change ripples outward from the source, until the space-time settles down to match the new configuration. But some of those ripples keep going, and become free-flowing gravitational waves.

Granted, it's not quite as simple as this. Space-time has no trouble keeping up with some sorts of changes to the distribution of matter fields. For example, the gravity wave emission from the Earth-Sun system is completely and utterly negligible. The potential well of the Earth basically moves along with the Earth, and isn't left behind just because the Earth is moving.
 

1. How does orbital period decay occur?

Orbital period decay occurs due to the emission of gravitational waves. These waves are produced when massive objects, such as binary star systems, accelerate due to their orbital motion. The emission of these waves causes the objects to lose energy and gradually spiral closer together, resulting in a shorter orbital period.

2. Can orbital period decay be observed?

Yes, orbital period decay can be observed through various methods. One way is through the measurement of pulsar timing. Pulsars are highly magnetized neutron stars that emit regular radio pulses. As the pulsar orbits its companion, the timing of these pulses can be affected by the orbital period decay, allowing scientists to measure the rate of decay.

3. How do gravitational waves affect the universe?

Gravitational waves play a crucial role in shaping the universe. They can cause objects to merge and form larger structures, such as galaxies and galaxy clusters. They also carry information about the events that produce them, such as the merger of black holes or neutron stars, providing a new way to study these phenomena.

4. Can gravitational waves be detected on Earth?

Yes, gravitational waves can be detected on Earth using advanced instruments called interferometers. These devices use laser beams to measure tiny changes in the distance between two objects caused by passing gravitational waves. The first direct detection of gravitational waves was made in 2015 by the Advanced LIGO interferometer.

5. Are there any practical applications of studying orbital period decay and gravitational waves?

Studying orbital period decay and gravitational waves has many practical applications. It allows us to better understand the behavior of celestial objects and can help us refine our understanding of gravity and the laws of physics. Additionally, the detection of gravitational waves has the potential to open up new avenues for astronomy and cosmology, providing a unique way to study the universe and its evolution.

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