Gravitational waves speed in a medium

Click For Summary
SUMMARY

Gravitational waves are predicted to travel at the speed of light (c) in a vacuum, similar to electromagnetic waves. However, their behavior in material mediums remains largely unexplored. According to Ingraham's 1997 paper, "Gravitational waves in matter," the speed of gravitational waves could potentially be less than c when propagating through molecular gas clouds of galactic or intergalactic size, although the effect would be minimal. The recent aLIGO results impose strict limits on any dispersion of gravitational waves.

PREREQUISITES
  • Understanding of gravitational wave physics
  • Familiarity with the stress-energy tensor in general relativity
  • Knowledge of electromagnetic wave propagation
  • Basic concepts of dispersion in wave mechanics
NEXT STEPS
  • Research Ingraham's "Gravitational waves in matter," GRG 29 (1997) 117
  • Explore the implications of aLIGO results on gravitational wave dispersion
  • Investigate the properties of molecular gas clouds in astrophysics
  • Study the effects of mass-energy on wave propagation in various mediums
USEFUL FOR

Astronomers, physicists, and researchers interested in gravitational wave propagation and its interaction with different mediums.

Gerinski
Messages
322
Reaction score
15
Electromagnetic waves are known to travel a c in a vacuum, but at lower speeds in a material medium.
What about gravitational waves? They are also predicted to travel at c in a vacuum, but what about them traveling through material mediums? Do they get slowed down? by which factor?

TX
 
Physics news on Phys.org
I doubt there has been much work done on that. The calculations I have seen regarding gravitational waves have all assumed that outside the source region there is negligible mass-energy, and accordingly assumes the stress-energy tensor outside the source to be zero. Since a medium has mass, the question of speed through a medium would be outside the scope of such calculations.
 
See Ingraham, "Gravitational waves in matter," GRG 29 (1997) 117. Ingraham suggests that the best chance for seeing ##v<c## might be in "gravitational wave propagation through molecular gas clouds of galactic or intergalactic size." Although n−1 would be incredibly small, he suggests that you might be able to see an effect accumulated over thousands or millions of light-years.

Note that the recent aLIGO result puts a very tight upper limit on dispersion.
 

Similar threads

  • · Replies 17 ·
Replies
17
Views
2K
  • · Replies 93 ·
4
Replies
93
Views
6K
  • · Replies 1 ·
Replies
1
Views
1K
  • · Replies 74 ·
3
Replies
74
Views
5K
  • · Replies 13 ·
Replies
13
Views
3K
  • · Replies 7 ·
Replies
7
Views
2K
  • · Replies 37 ·
2
Replies
37
Views
3K
  • · Replies 3 ·
Replies
3
Views
2K
Replies
1
Views
1K
  • · Replies 14 ·
Replies
14
Views
2K