Gravitational Effect of Electromagnetic Radiation

In summary, the conversation discusses the potential impact of electromagnetic radiation from stars on the gravitational coalescence of galaxies. It is estimated that there is a significant amount of energy in the form of photons in the halo surrounding galaxies, but the calculations may overestimate the amount due to the limitations of star energy conversion and the inverse square law for gravitation. The possibility of photons exerting a gravitational effect is also discussed, but it is uncertain and may complicate the combination of quantum mechanics and general relativity.
  • #1
Jon Mel
2
1
Hello PPer's,

I have been considering the effect to which electromagnetic radiation emitted from stars might play in the gravitational coalescence of galaxies. Surrounding every galaxy there must be a halo of electromagnetic radiation streaming outwards at the speed of light which diminishes according to the inverse square rule. From the billions of stars converting their mass into pure energy the gravitational effect of this halo can be estimated. This energy is otherwise largely invisible because it does not have the chance to interact with much as it moves away from the galaxy and into open space. In fact these photons exist as a quantum probability wave which will collapse only when they interact with other galaxies billions of years away. Yet they must exert a real gravitational effect as I will demonstrate with a rough calculation here:

Assuming our Sun to be an average star which will burn for 10 billion years and taking the Milky Way as being 100,000 light years across we can calculate that there is approximately, 1/(10^10 / 10^5) = 1/100,000 solar mass of electromagnetic radiation distributed in a 100,000 light year halo surrounding our galaxy just from our Sun.

Assuming the Milky Way to contain 100 billion stars of which the Sun is average then we have, 10^11 x 10^(-5) = 10^6, or 1 million solar masses of energy in this 100,00 light year halo.

Of course these assumptions take our Sun as losing all of its mass to photons which we know to be untrue, our Sun will lose much of its mass in solar winds when it is a red giant and will hold on to a lot of its mass later as an inert white dwarf. However larger stars burn quicker and more fully convert their mass into photons, leaving behind only supernovae remnants. These stars will therefore have a greater percentage of their total mass as electromagnetic radiation within the 100,000 light year halo at anyone time, for example a 50 solar mass O-type star may have a life span of just 10 million years so that 1% of its mass, or 0.5 solar masses, could be having a gravitational effect from within the halo.

Of course the gravitational influence of this electromagnetic radiation would not stop at the 100,000 light year mark, it would only become more diffuse according to the inverse square rule with distance, so that at 200,000 light years it would have 1/4 of the gravitational effect on stars within, or outlying our Milky Way.

Would this gravitational effect explain, or partly contribute to an explanation, for dark matter?
 
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  • #2
Your computations (a) highly overestimates the amount of energy that can possibly be converted to photons in a star (iron has the largest binding energy per nucleus at about 8 MeV, compared to the proton mass of almost 1 GeV, the effect is less than one percent at most) (b) assumes an inverse square law for gravitation when considering relativistic particles, (c) I am probably missing something else, it is late here.

The answer to your question is simply "no". Also be aware that Physics Forums does not allow personal theories and this thread is already on the very border.
 
  • #3
Power output of the Sun: 4x1026 watts = 4x1026 joules/second x 60 seconds x 60 minutes x 24 hours x 365.25 days x 10 billion years = 1.26x1044 joules.

1.26x1044 joules / 300 million2 (c2)= 1.4x1027 kg radiated away over the course of 10 billion years.

1.4x1027 kg / 1.99×1030 kg (1 solar mass) = 7.05x10-4 solar masses, or 0.000705 solar masses, radiated away over 10 billion years.

Hope my math is right. o_O
 
  • #4
Ok thanks guys, that knocks that idea on the head!

I'd still be interested to know if photons, being at the relativistic velocities they are, can indeed exert a gravitational effect even if it is infinitesimally small. If true, then surely this would negate the possibility of combining quantum mechanics with general relativity since the photon would be in a probability state whilst still interacting with the space-time field. Could the space-time field therefore drain energy from the photon whilst it is traveling long distances thereby causing a redshift effect?
 
  • #5
Jon Mel said:
I'd still be interested to know if photons, being at the relativistic velocities they are, can indeed exert a gravitational effect even if it is infinitesimally small.

Sure. They have energy and therefore will alter the stress-energy tensor, which is where gravitation comes from.

Jon Mel said:
If true, then surely this would negate the possibility of combining quantum mechanics with general relativity since the photon would be in a probability state whilst still interacting with the space-time field. Could the space-time field therefore drain energy from the photon whilst it is traveling long distances thereby causing a redshift effect?

I can't follow this.
 

1. How does electromagnetic radiation affect gravitational fields?

Electromagnetic radiation, also known as light, has no mass and therefore does not directly affect gravitational fields. However, it can indirectly affect them by interacting with charged particles, which can in turn affect the gravitational field.

2. Can electromagnetic radiation produce gravitational waves?

No, only massive objects can produce gravitational waves. However, electromagnetic radiation can cause changes in the distribution of mass and energy, which can indirectly produce gravitational waves.

3. Does the strength of electromagnetic radiation affect its gravitational effect?

Yes, the strength of electromagnetic radiation, or its energy, can affect its gravitational effect. Higher energy radiation can have a stronger effect on charged particles and therefore have a greater impact on the gravitational field.

4. How does the gravitational effect of electromagnetic radiation compare to that of massive objects?

The gravitational effect of electromagnetic radiation is much smaller compared to that of massive objects. This is because electromagnetic radiation has no mass and therefore its gravitational force is significantly weaker.

5. Can the gravitational effect of electromagnetic radiation be measured?

Yes, the gravitational effect of electromagnetic radiation can be measured using sensitive instruments such as gravitational wave detectors. However, the effect is very small and can only be detected in certain situations, such as during extreme events like supernovae or when studying the behavior of very strong electromagnetic fields.

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