How many gravitons are there in the observable universe?

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Discussion Overview

The discussion revolves around the hypothetical number of gravitons in the observable universe, comparing it to known quantities of protons, photons, and neutrinos. Participants explore the implications of these quantities, their origins, and the relationship between them, particularly in the context of cosmic events like the Big Bang and inflation.

Discussion Character

  • Exploratory
  • Debate/contested
  • Technical explanation

Main Points Raised

  • One participant suggests that if there are approximately 10^80 protons and 10^90 photons in the observable universe, the number of gravitons might also be around 10^90, questioning the implications of their temperature.
  • Another participant states that gravitons are hypothetical and suggests that their number is effectively zero until proven otherwise.
  • A participant clarifies that relic photons and neutrinos originate from different eras, with neutrinos forming around 2 seconds after the Big Bang and photons around 380,000 years later, which may affect their comparative numbers.
  • There is a query about whether the numbers of neutrinos and photons are still approximately equal given their different formation times.
  • One participant discusses the dependence of neutrino number on unknown mass and provides a method for estimating neutrino density based on energy density and volume.
  • A question is raised about the velocity range of neutrinos and whether their energies can vary significantly based on their source events.
  • Another participant notes that relic neutrinos were in thermal equilibrium when formed and discusses their expected thermal distribution today, suggesting that their kinetic energy is constrained by the mass of the heaviest neutrino type.
  • There is a request for a more detailed mathematical explanation regarding neutrino density estimation.

Areas of Agreement / Disagreement

Participants express differing views on the existence and number of gravitons, with some asserting they are hypothetical while others explore their potential quantities. The discussion on neutrinos and their relationship to photons also reveals uncertainty and differing interpretations regarding their numbers and origins.

Contextual Notes

Participants acknowledge the unknowns surrounding neutrino mass and the implications for estimating their density. The discussion reflects a range of assumptions and interpretations regarding the thermal history of the universe and the nature of hypothetical particles.

jimgraber
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It is thought that there are approximately 10^80 protons in the observable universe, but there are approximately 10^90 photons in the observable universe. If my googling is correct, there are also approximately 10^90 neutrinos in the observable universe, but their temperature is only 1.9 degrees Kelvin, compared to 2.7 degrees Kelvin for the photons. How many gravitons are there in the observable universe? (And what is their temperature?)

Is this number also approximately equal to 10^90? Why or why not?

The photons and neutrinos are supposedly relics of the big bang.
But we have just (Bicep 2) (indirectly) detected gravitons which are relics of inflation.
Does this make a difference?

Are there photons and neutrinos which are relics of inflation also?
 
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Gravitons are only hyperthetical. So 0, until we can prove otherwise.
 
jimgraber said:
Are there photons and neutrinos which are relics of inflation also?
No, at the end of inflation the universe was so hot that both photons and neutrinos didn't live long enough to "remain intact". The relic neutrinos come from 2 seconds after the big bang, and the photons from ~380 000 years after it.

There are good estimates about the amount of energy in gravitational waves, but I don't know their frequency distribution, so I cannot calculate back to hypothetical gravitons.
 
So, if the relic photons and relic neutrinos come from different eras, is it still true their numbers are approximately equal?
(I had thought they were in quasi -equilibrium and the numbers were related similar to the temperatures.)
If not, how many neutrinos are there?
TIA. Jim Graber
 
This number depends on the unknown neutrino mass, but the current constraints allow a good approximation: take the neutrino energy density, approximate ~10-100 meV of energy per neutrino, and you get the neutrino density. Multiply with whatever volume you want to consider to get the number of neutrinos.
 
approximate ~10-100 meV of energy per neutrino, and you get the neutrino density

Does the standard theory presume that neutrinos all travel within a range of velocities? It would seem that each neutrino would have a velocity determined by the type of event from which the neutrino issued... in which case is it not possible to have extremely large neutrino energies and very small neutrino energies ...just curious where the range estimate came from.
 
The relic neutrinos where in thermal equilibrium at the time they formed, afterwards it just got cooler from the expansion of the universe, so we still expect their thermal distribution now (~2 K, a bit colder than the photon background). With less than 1 meV as corresponding energy, their kinetic energy has to be below the mass of the most massive neutrino type, so at least one of the three types has to be significantly slower than the speed of light now - those 10 to 100 meV are just an estimate for this mass.
 
mfb said:
This number depends on the unknown neutrino mass, but the current constraints allow a good approximation: take the neutrino energy density, approximate ~10-100 meV of energy per neutrino, and you get the neutrino density. Multiply with whatever volume you want to consider to get the number of neutrinos.

May someone post a more complete explanation of this with some maths?
 

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