Energy & Momentum: The Effects of Photons on Stars

In summary, the momentum vector of a photon changes as it travels towards a star, leading to an increase in both energy and momentum. This implies a potential energy between the photon and star, which can be calculated using the theorem \vec{F}=\nabla E_p. The interaction between the photon and star is equivalent to the photon curving the spacetime around it. However, the speed of light is not actually faster than the speed of light, as there is a delay in the interaction between the photon and star.
  • #1
espen180
834
2
Scenario 1:
A photon is traveling straight towards a star. As it goes deeper in the star's gravitational well, its frequency grows, coresponding to an increase both in energy and momentum.

Scenario 2:
A photon is traveling towards a star, but not head on. As it passes the star, its path changes direction. This corresponds to a chang in momentum.

In both of these scenarioes, the momentum vector of the photon changes. In order for momentum to be conserved, the star will have to gain momentum in the direction of the photon.

This in turn means that there is a net increase in kinetic energy of the system (counting the photon's E=hf as kinetic). Therefore, the photon must have a potential energy with respect to the star, which shouldn't be extremely hard to calculate.

By the theorem [tex]\vec{F}=\nabla E_p[/tex], there is excerted forces between them; gravitational forces. This is equivalent to the photon curving the spacetime around it.

Now back to Scenario 1: Since energy and momentum is conserved, and the photon makes the star accelerate towards itself, does that not imply that the gravitational interaction propagates faster than light?
 
Physics news on Phys.org
  • #2
espen180 said:
Therefore, the photon must have a potential energy with respect to the star, which shouldn't be extremely hard to calculate.

Observations of gravitational effects on photons can be derived from this simple Hamiltonian

[tex] H = Mc^2 + pc - \frac{2GMp}{cR} [/tex]

where M is the star's mass, p is the photon's momentum, G is the gravitational constant, R is the distance between the photon and the center of the star. Star's kinetic energy term [tex] p^2/(2M) [/tex] is negligibly small and ignored.

Eugene.
 
  • #3
espen180 said:
Scenario 1:
A photon is traveling straight towards a star. As it goes deeper in the star's gravitational well, its frequency grows, coresponding to an increase both in energy and momentum.

Scenario 2:
A photon is traveling towards a star, but not head on. As it passes the star, its path changes direction. This corresponds to a chang in momentum.

In both of these scenarioes, the momentum vector of the photon changes. In order for momentum to be conserved, the star will have to gain momentum in the direction of the photon.

This in turn means that there is a net increase in kinetic energy of the system (counting the photon's E=hf as kinetic). Therefore, the photon must have a potential energy with respect to the star, which shouldn't be extremely hard to calculate.

By the theorem [tex]\vec{F}=\nabla E_p[/tex], there is excerted forces between them; gravitational forces. This is equivalent to the photon curving the spacetime around it.

Now back to Scenario 1: Since energy and momentum is conserved, and the photon makes the star accelerate towards itself, does that not imply that the gravitational interaction propagates faster than light?
I'm not an expert on GR but I would say that the photon interacts locally with the field around the star, not with the star itself (or its core).
 
  • #4
Replace the gravitational field with an electric field and the photon with an electron. This argument then proves that the speed of light is faster than the speed of light.
 
  • #5
Looking back, I realize that I have fallen victim to a bare assertion fallacy by not taking the interation delay into account in the first place. :rolleyes:
 

1. How do photons affect the energy and momentum of stars?

Photons, which are particles of light, play a crucial role in the energy and momentum of stars. They are constantly being produced and released by the nuclear reactions happening in the star's core. These photons carry energy and momentum with them as they travel through the star's interior and eventually escape into space. This energy and momentum transfer is essential for maintaining the stability and dynamics of the star.

2. Can photons change the direction of a star's motion?

Yes, photons can indeed change the direction of a star's motion. This is due to the conservation of momentum, which states that the total momentum of a system must remain constant. When photons are emitted or absorbed by a star, they also carry momentum. As a result, the star's momentum changes, causing its direction of motion to shift.

3. How do photons affect the temperature of stars?

Photons play a major role in determining the temperature of a star. As they are released from the core, they carry a significant amount of energy with them. This energy is then absorbed by the surrounding gas and increases its temperature. The more photons are produced and released, the higher the temperature of the star will be.

4. Can the energy and momentum of photons be measured?

Yes, the energy and momentum of photons can be measured. Scientists use specialized instruments, such as spectrometers, to detect and measure the properties of photons. By analyzing the wavelengths and frequencies of photons, scientists can determine their energy and momentum, which provide valuable insights into the behavior of stars.

5. How do photons contribute to a star's lifecycle?

Photons play a crucial role in every stage of a star's lifecycle. They are responsible for initiating the nuclear reactions that power the star and keep it stable. As the star ages, photons continue to play a role in its evolution, affecting its size, temperature, and eventual fate. When a star dies, photons are also released as it explodes in a supernova, spreading its energy and matter throughout the universe.

Similar threads

  • Special and General Relativity
Replies
26
Views
369
  • Special and General Relativity
Replies
21
Views
2K
  • Special and General Relativity
2
Replies
57
Views
6K
  • Special and General Relativity
Replies
30
Views
2K
Replies
1
Views
240
  • Special and General Relativity
2
Replies
53
Views
4K
  • Special and General Relativity
Replies
19
Views
2K
  • Special and General Relativity
Replies
17
Views
1K
Replies
21
Views
1K
  • Special and General Relativity
3
Replies
83
Views
5K
Back
Top