How Are Gravitational Waves Produced?

Click For Summary
SUMMARY

Gravitational waves are produced by accelerating masses, specifically through changes in their quadrupole moment. In binary star systems, such as PSR B1913+16, gravitational waves are emitted due to the varying displacement between two orbiting masses. This oscillation creates an alternating gravitational field, which is a fundamental aspect of gravitational wave production. Classical physics principles, including conservation of mass-energy and momentum, dictate the conditions under which these waves can be generated.

PREREQUISITES
  • Understanding of gravitational waves and their properties
  • Familiarity with quadrupole moments in classical physics
  • Knowledge of binary star systems and their dynamics
  • Basic principles of conservation laws in physics
NEXT STEPS
  • Research the mathematical formulation of gravitational wave equations
  • Explore the dynamics of binary star systems and their gravitational interactions
  • Study the differences between monopole, dipole, and quadrupole moments
  • Learn about the detection methods for gravitational waves, such as LIGO
USEFUL FOR

Astronomers, physicists, and students interested in gravitational wave research and the dynamics of celestial bodies.

adm2e
Messages
8
Reaction score
0
This might seem simple...

I'm having a bit of trouble both finding and interpretting information on how a gravitational wave is produced.
I know they are analogous to EM waves, and that they are produced by accelerating masses, but it's more complicated than that, isn't it?

Can anyone explain to me what a quadrupole moment is, in layman's terms preferably?
How does a binary star system (such as PSR B1913+16) emit gravitational waves? How does it produce an alternating gravitational/gravitomagnetic field, since gravity is never repulsive?
If you could explain everything in classical physics, that'd be great too.

Thanks a lot in advance.
 
Last edited:
Physics news on Phys.org
If you made the mass of a star oscillate (monopole moment) the gravitational field elsewhere would also strongly oscillate (gravitational waves), but conservation of mass-energy makes it impossible to do this. (You can't do it for charges either.)

If you shook an isolated star up and down (dipole moment), that would also produce gravitational waves, but conservation of momentum makes it impossible to do this. (You can do this one for electric charges though, since inertia is equal to gravitational rather than electric charge.)

The next weaker term in the mathematical series expansion of the potential gravitational wave equation, namely quadrapole moment, is what results if you vary the displacement between two masses. This is physically possible (they only need orbit each other).
 
Thanks a lot for your help.
With the dipole moment, do you mean that a star will not oscillate up and down, or that this motion won't release waves?
Will the wave made by orbiting masses by transversal or helical?
 

Similar threads

  • · Replies 4 ·
Replies
4
Views
2K
  • · Replies 5 ·
Replies
5
Views
2K
  • · Replies 0 ·
Replies
0
Views
2K
  • · Replies 12 ·
Replies
12
Views
4K
  • · Replies 14 ·
Replies
14
Views
4K
  • · Replies 2 ·
Replies
2
Views
3K
  • · Replies 4 ·
Replies
4
Views
3K
  • · Replies 12 ·
Replies
12
Views
3K
  • · Replies 80 ·
3
Replies
80
Views
11K
  • · Replies 0 ·
Replies
0
Views
2K