Understanding 2 Effects of G.R.: Periastron Precession & Pulsation Periods

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In summary: Gravitational time dilation depends on the gravitational potential difference. When they are closest, their combined masses create the lowest gravitational potential.
  • #1
Dyatlov
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Hello, after much thought I decided to ask here about the specifics of 2 of the effects of G.R., which are a bit unclear to me.
The scenario is - one pulsar and one neutron star orbiting their barycenter as you can see from the image below (ignore the binary pulsar title of image, it's just what I have found on web).

bin_puls.gif

One of the effects of G.R. is that the pulsar's (right orbit) periastron will change over time. The change was measured at 4 degrees each year. It's the same as Mercury with it's change of 43 arc seconds every 100 years of it's perihelion.
Why exactly is that? It's due to the perturbations caused by neutron star on the pulsar's orbit ? Or in case of Mercury, of the other outer planets perturbing it's orbit? I know for Mercury that the Schwarzschild radius/ Mercury-Sun radius is the smallest for the entire solar system, that's why we can see this effect at it's best. It has something to do with ripples in space-time sent outward at c by the Sun and perturbing Mercury's orbit? I would like a link with some in-detail explanation of this effect if it's possible.
Now for the second effect: gravitational redshift. I understand this effect pretty well, but in this scenario (neutron-pulsar system) we are talking about pulsation periods. The change in pulsations can be seen from the formula was ΔPp/ P = [ 1+(Vr/c)/ 1-(Vr/c)]-1/2 – 1, Vr being the radial velocity.
Now for the actual question: When both objects are at their periastron (so their distance between is at a minimum), the pulsations from the pulsar will be slowed down (from an observer's point of view, which is located outside their gravitational fields). Why is that? Is it because matter pulls time and the presence of the neutron star's gravitational field makes the time go slower from the observer's p.o.v., therefore the pulsations will come at a slower rate from him?
Any help is greatly appreciated.
Thanks in advance.
 
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  • #2
Dyatlov said:
Why exactly is that? It's due to the perturbations caused by neutron star on the pulsar's orbit ? Or in case of Mercury, of the other outer planets perturbing it's orbit? I know for Mercury that the Schwarzschild radius/ Mercury-Sun radius is the smallest for the entire solar system, that's why we can see this effect at it's best. It has something to do with ripples in space-time sent outward at c by the Sun and perturbing Mercury's orbit?.

The exact solution for 'elliptical' orbits in the Schwarzschild vacuum is in terms of the Weierstrass ##\wp## function which is modular but has two periods.

The precession just happens - it is difficult to assign a specific cause in view of this solution. Also, the effects of other bodies and the sun's oblateness have been factored into the calculation. The remaining (anomolous) precession is a relativistic effect.

G. V. Kraniotis, S. B. Whitehouse,
Precession of Mercury in General Relativity, the Cosmological Constant and Jacobi's Inversion
problem.
Preprint http://128.84.158.119/abs/astro-ph/0305181v3
 
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  • #4
Dyatlov said:
Thanks for the answer. Is this the paper which you are linking? http://arxiv.org/pdf/astro-ph/0305181v4.pdf (yours doesn't work).
Yes. See section 3.1.

[edit]
You could find this relevant to the binary part of your question

Periastron shift in Weyl class spacetimes
Donato Bini, Francesco De Paolis, Andrea Geralico,
Gabriele Ingrosso and Achille Nucita

arXiv:gr-qc/0502062v1 14 Feb 2005
 
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  • #5
Dyatlov said:
It has something to do with ripples in space-time sent outward at c by the Sun and perturbing Mercury's orbit?
If by ripples you mean gravitational waves, then no. The orbit will precess in a static Schwarzschild space time too, due to the spatial geometry. Simple explanation at bottom here:
http://www.physics.ucla.edu/demoweb..._and_general_relativity/curved_spacetime.html

Dyatlov said:
When both objects are at their periastron (so their distance between is at a minimum), the pulsations from the pulsar will be slowed down (from an observer's point of view, which is located outside their gravitational fields). Why is that?
Gravitational time dilation depends on the gravitational potential difference. When they are closest, their combined masses create the lowest gravitational potential.
 
  • #6
Thanks for the answer and link. That cleared my first issue.
A.T. said:
If by ripples you mean gravitational waves, then no. The orbit will precess in a static Schwarzschild space time too, due to the spatial geometry. Simple explanation at bottom here:
http://www.physics.ucla.edu/demoweb..._and_general_relativity/curved_spacetime.html
Gravitational time dilation depends on the gravitational potential difference. When they are closest, their combined masses create the lowest gravitational potential.
The stronger the gravitational potential is(the closer the clock is to the source of gravitation), the slower time should pass, right?
Well in this scenario you said their combined masses create the lowest gravitational potential therefore the pulse periods should be the fastest not slowest. Did you mean the highest gravitational potential maybe? That would explain my case.
 
  • #7
Dyatlov said:
The stronger the gravitational potential is(the closer the clock is to the source of gravitation)
Gravitational potential is lower, closer to the source of gravitation
 
  • #8
A.T. said:
Gravitational potential is lower, closer to the source of gravitation
So clocks that are far from massive bodies (or at higher gravitational potentials) run faster, and clocks close to massive bodies (or at lower gravitational potentials) run slower.
That is why the pulsation periods gets bigger when the two objects are at their periastron.
Thanks a lot for the help.
 
  • #9
Dyatlov said:
So clocks that are far from massive bodies (or at higher gravitational potentials) run faster, and clocks close to massive bodies (or at lower gravitational potentials) run slower.
Yes

Dyatlov said:
That is why the pulsation periods gets bigger when the two objects are at their periastron.
Yes, because the gravitational potential goes even lower, with another big mass nearby.
 

1. What is G.R. and how does it affect periastron precession and pulsation periods?

G.R. stands for General Relativity, which is a theory of gravity proposed by Albert Einstein. It states that gravity is not a force between masses, but rather the curvature of spacetime caused by the presence of mass. This curvature can affect the motion of objects, such as the orbit of a planet around a star, leading to a phenomenon known as periastron precession. G.R. can also affect the period of pulsation of stars, as the mass of the star causes a curvature in spacetime, causing the pulsation to slow down or speed up.

2. What is periastron precession and how is it related to G.R.?

Periastron precession is the gradual rotation of the point of closest approach between two orbiting objects, such as a star and a planet. In the context of G.R., this phenomenon is caused by the curvature of spacetime around the more massive object, which affects the trajectory of the smaller object. This effect is particularly noticeable in binary star systems, where the stars are close enough for G.R. to have a significant impact on their orbits.

3. Can G.R. affect the pulsation period of all stars?

Yes, G.R. can affect the pulsation period of all stars to some degree. However, the magnitude of this effect depends on the mass and size of the star, as well as its distance from other massive objects. In general, the larger and more massive the star, the greater the impact of G.R. on its pulsation period.

4. How do scientists measure the effects of G.R. on periastron precession and pulsation periods?

Scientists use a variety of techniques to measure the effects of G.R. on periastron precession and pulsation periods. For periastron precession, they can use precise measurements of the orbits of binary star systems and compare them to predictions based on G.R. For pulsation periods, they can monitor the brightness of stars over time and look for any changes in their pulsation patterns that can be attributed to G.R.

5. Can G.R. be used to study other astronomical phenomena?

Yes, G.R. has been used to study a wide range of astronomical phenomena, such as gravitational lensing, black holes, and the expansion of the universe. It is a fundamental theory that has revolutionized our understanding of the cosmos and continues to be a crucial tool for scientists studying the universe.

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