Separation angle between pulsars detecting Gravitational Waves

  • #1
zinn
1
0
TL;DR Summary
How can separation angle alone tell you about the correlation between gravitational wave signals from pulsar timing?
I’m trying to understand the Hellings and Downs curve that is being used to argue for the existence of a gravitational wave background ([NANOGrav article][1]). How can it be that the angle between two pulsars is the only variable that determines if the gravitational waves will interfere constructively (correlated) or destructively (anti-correlated). I would have imagined that distance from the observer would also be a factor.

(Image source: https://astrobites.org/2016/08/10/the-predictor-of-pulsar-timing/)
3EFC2F01-19E9-4450-9E02-914871009C04.png


I imagine that a key part of understanding this concept would be visualising the gravitational waveforms in 3D. Should I be picturing something like this? [youtube video with gravitational wave animations][2]


[1]: https://nanograv.org/15yr/Summary/Background
[2]:
[3]: https://i.stack.imgur.com/w3DSd.png
 

Similar threads

Replies
1
Views
757
  • Astronomy and Astrophysics
Replies
1
Views
1K
Replies
3
Views
1K
  • Special and General Relativity
Replies
12
Views
1K
  • Special and General Relativity
Replies
24
Views
1K
  • Astronomy and Astrophysics
Replies
4
Views
2K
  • Cosmology
Replies
7
Views
2K
Replies
23
Views
13K
  • Quantum Physics
2
Replies
69
Views
4K
  • Beyond the Standard Models
Replies
2
Views
2K
Back
Top