Why can't we detect neutrino-antineutrino annihilation?

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    Annihilation Neutrinos
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Discussion Overview

The discussion revolves around the detection of neutrino-antineutrino annihilation and the challenges associated with observing the resulting photons. Participants explore the astrophysical processes that produce antineutrinos, the potential outcomes of their interactions, and the implications for understanding neutrino masses.

Discussion Character

  • Exploratory
  • Technical explanation
  • Debate/contested

Main Points Raised

  • Some participants propose that neutrino-antineutrino annihilation should produce detectable infrared photons, but question why these photons are not observed.
  • Others argue that Doppler broadening may obscure any identifiable peaks in the photon spectrum, suggesting that the energy of the annihilation photons is primarily influenced by the kinetic energies of the neutrinos rather than their masses.
  • One participant notes that the cross-section for the annihilation process is extremely small, raising questions about the likelihood of detection compared to other interaction possibilities.
  • Another participant expresses skepticism about the accuracy of estimations regarding the cross-section for neutrino-antineutrino annihilation.
  • Some participants discuss the nature of neutrinos, debating whether they can self-annihilate if they are Majorana particles, with references to existing literature and models.
  • There is a mention of the Z boson decay to neutrinos, suggesting a reverse process that may imply self-annihilation capabilities.
  • One participant corrects a misconception regarding Majorana particles and their ability to self-annihilate, indicating that this characteristic may not apply to leptons.

Areas of Agreement / Disagreement

Participants express differing views on the detectability of neutrino-antineutrino annihilation and the implications of neutrino properties, indicating that the discussion remains unresolved with multiple competing perspectives.

Contextual Notes

Participants highlight limitations in the estimations of cross-sections and the dependence on various theoretical models, including the nature of neutrinos as Majorana or Dirac particles, without reaching a consensus.

bcrowell
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Various astrophysical processes produce antineutrinos, which then fly off into outer space. I assume there are pretty accurate estimates of the production rates. I can imagine three possible fates for such an antineutrino: (1) annihilating with a neutrino, (2) interacting with baryonic matter, (3) ending up as the only particle inside its own cosmological horizon. It seems like we ought to have pretty good estimates of the rate of the neutrino-antineutrino annihilation process. Each such annihilation produces two back-to-back photons. If the neutrino masses are on the order of 0.1 eV, then these are infrared photons with wavelengths on the order of 10^4 nm. Why can't we detect these photons and thereby determine the neutrino mass spectrum? Are the peaks too weak? Too spread out by Doppler broadening?
 
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bcrowell said:
Too spread out by Doppler broadening?

Surely the Doppler broadening is so great that there would be nothing you could call a "peak" in the spectrum? Essentially all neutrinos are relativistic; the energy of the annihilation photons would be almost entirely determined by the neutrinos' kinetic energies and not their masses.
 
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The_Duck said:
Surely the Doppler broadening is so great that there would be nothing you could call a "peak" in the spectrum? Essentially all neutrinos are relativistic; the energy of the annihilation photons would be almost entirely determined by the neutrinos' kinetic energies and not their masses.

Makes sense!
 
The vv → γγ cross-section is truly microsocpic. (zeptoscopic?)

It's got to be photons, because everything else is kinematically blocked. It's got to go through the Z-pole, at 90 GeV when the neutrinos are at 1/40,000 of an eV. It also has to go through a loop which gives additional kinematic reduction, higher powers of the couplings, and a 1/16π2, which in light of the other factors, is almost too small to worry about.
 
Vanadium 50 said:
The vv → γγ cross-section is truly microsocpic. (zeptoscopic?)

It's got to be photons, because everything else is kinematically blocked. It's got to go through the Z-pole, at 90 GeV when the neutrinos are at 1/40,000 of an eV. It also has to go through a loop which gives additional kinematic reduction, higher powers of the couplings, and a 1/16π2, which in light of the other factors, is almost too small to worry about.

The cross-section is small ... compared to what? Is the probability of this fate small compared to both of the other possibilities listed in #1? Negligibly small?
 
I would say "so small that I don't trust the estimation to be done correctly".

If you want a ballpark, I'd estimate that the vv cross-section divided by the vp cross-section is alpha x m(v)/m(p) x [m(v)/m(e)]^4 /16 pi^2.
 
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Thanks Bill. I had acquired the notion that Majorana particles do not self annihilate. Upon further review, I find the consensus is that is only true for bosons, not leptons.
 
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? If neutrinos are majorana they can annihilate - we are supposed to find the Majorana nature by neutrinoless double beta decay.
 
  • #11
Don't we know already that neutrinos can self-annihilate through a Z boson, because we observe that the Z can decay to neutrinos? ( simply the reverse process)
 
  • #12
Thanks Bill. I had acquired the notion that Majorana particles do not self annihilate. Upon further review, I find the consensus is that is only true for bosons, not leptons.

It seems to me that this also isn't true, as two Z bosons ( which are there own antiparticles) can self-annihilate through a higgs boson.
 

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