Binary pulsars and general relativity

Click For Summary
Binary pulsars, particularly PSR 1913+16, provide crucial evidence for general relativity, demonstrating strong-field effects and supporting the existence of gravitational waves. Discovered in 1974, this system consists of two neutron stars orbiting a common center of mass, not a black hole, and is notable for its precision in timing, acting as a natural relativistic experiment. The pulsars are not visible optically due to their small size but can be detected through the periodic pulses they emit. The eventual coalescence of these stars, expected in about 300 million years, will produce significant gravitational waves. The discussion highlights the importance of binary pulsars in astrophysics and their role in advancing our understanding of gravitational phenomena.
vladimir69
Messages
124
Reaction score
0
hi
just wondering if anyone knows some interesting things about binary pulsars in relation to general relativity. i have to give a short presentation on the topic and need some ideas on what to talk about

thanks in advance
 
Physics news on Phys.org
Try a google for "binary pulsar general relativity". You should find a lot of articles about PSR 1913+16, and the researchers who got the Nobel prize for their discovery.

Basically this is one of the few strong-field confirmations of GR that we have. A pulsar is a highly accurate clock, so astronomy has blessed us with a naturally occurring relativistic experiment.
 
It was the discovery of the first Binary pulsar in 1974 that strengthened the possibility of the existence of gravitational waves. It also got the dicsoverers one of the few Nobels given for astrophysics.

You can find more information here:http://nobelprize.org/physics/laureates/1993/index.html
 
thanks for the replies
i will be sure to check out that link
 
The two neutrons stars forming PSR 1913+16 are orbiting around the center of mass of the system, but are progressively coming closer together. They will eventually coalesce in about 300 million of years, emiting copious amounts of gravitational waves during the collision
 
i'm just a little unclear about something
is the common mass they orbit around a black hole? and can the pulsars actually be seen or only detected by the pulses they emit periodically?
 
Last edited:
jimbo007 said:
i'm just a little unclear about something
is the common mass they orbit around a black hole? and can the pulsars actually be seen or only detected by the pulses they emit periodically?

The two pulsars orbit around a common centre of mass and not a common mass and, as far as we know, it does not contain a black hole. The concept of centre of mass makes it easier to study a system made up of many particles and it is not necessary for mass to exist and the centre of mass.

Pulsars/Neurton stars are too small to be seen optically. It's surroundings can be detected with optical and x-ray telescopes.
 
As far as I know, only one of the two stars is a pulsar.
 
pervect said:
As far as I know, only one of the two stars is a pulsar.

You're right, but I don't why the system is usually referred to as 'Binary Pulsars'. PSR 1913+16 was the first known binay neutron star system and the only known binary pulsar is J0737–3039.
 

Similar threads

  • · Replies 0 ·
Replies
0
Views
1K
  • · Replies 4 ·
Replies
4
Views
2K
  • · Replies 30 ·
2
Replies
30
Views
1K
Replies
32
Views
3K
  • · Replies 5 ·
Replies
5
Views
2K
Replies
8
Views
2K
  • · Replies 5 ·
Replies
5
Views
2K
  • · Replies 2 ·
Replies
2
Views
2K
  • · Replies 3 ·
Replies
3
Views
936
Replies
45
Views
6K