Is the Proton's Half Life Really 10 to the Power of 32 Years?

In summary, the conversation discusses the stability and possible decay of the proton, with some sources stating it is stable while others claim it has a half life of 10 to the power of 32 years. The only proposed decay for a proton is into a positron and photon, which does not conserve baryon number. The conversation also touches on the concept of proton decay and its relation to the second law of thermodynamics. However, it is mentioned that the proton is considered stable on time scales longer than the age of the universe and experiments have not observed any decay. The conversation then shifts to the possibility of other particles, such as the electron, also being unstable.
  • #71
vanesch said:
Of course one assumes that this symmetry is broken, and that the relevant bosons have a big mass (the "GUT" scale), which decreases this interaction rate. If one estimates this scale (that's where the 3 coupling constants of the standard model should unify) one arrives at something of 10^15 GeV. Using this value, the proton decay rate should be of the order of a life time of 10^31 years, which has been falsified by experiment. So that's where all the hassle came from.

I should add a few things. The GUT scale is in fact already build into the standard model (together with the experimental values of the coupling constants), as we know, at "low" energies what are the coupling constants, and we can calculate how they evolve (running of the coupling constants in renormalization) when we go to higher energies (a few low-order Feynman graphs are sufficient). The nice thing is that they all cross (the electroweak couplings rise, and the strong coupling falls) at about 10^15 GeV. They ALMOST cross, but not really. If they are the results of a broken symmetry, then at the scale of the symmetry, they should become equal to the one and only coupling constant of the grand unifying interaction. And now, the precision on experimental parameters is such that we know that they do not cross exactly at the same point.
Comes in supersymmetry. It is possible to twiddle a bit here, and then one can make the running constants cross exactly. I'm not an expert on this, but apparently, supersymmetry can also "inhibit" proton decay, so that its life time becomes longer than naively estimated. So proponents of supersymmetry say that SUSY can save GUT and that the long proton decay life time is an indirect indication. Others say that this is a bit too artificial twiddling to get out what people wanted to get out.

cheers,
Patrick.
 
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  • #72
kurious said:
The mystery of the asymmetry of matter-antimatter remains to be resolved. At the present time, no such a theory of resolution exist.
We don't know that there is an asymmetry between matter and antimatter, except in this portion of the universe. Most astronomical data is from photons emitted by far away sources. Antiparticles interactions with other antiparticles are the same as particles interactions with other particles. If some region of the universe consists of antimatter, astronomical measurements would not be able to determine that, since there is no matter interacting with it for us to compare it with.
 
  • #73
jtolliver said:
We don't know that there is an asymmetry between matter and antimatter, except in this portion of the universe. Most astronomical data is from photons emitted by far away sources. Antiparticles interactions with other antiparticles are the same as particles interactions with other particles. If some region of the universe consists of antimatter, astronomical measurements would not be able to determine that, since there is no matter interacting with it for us to compare it with.
a) there'd be all kinds of fireworks from a zone of contact ... even the inter-galactic medium isn't empty, and cosmic rays pervade everything (no such fireworks observed); b) while not impossible for there to be regions of matter and regions of anti-matter in both of which there are stars, galaxies etc ... which don't ever get to an opposite region, there will be stars, planets, even galaxies that travel far from their parent cluster (no such megafireworks observed); c) cosmological models with this slight imbalance between matter and anti-matter fit observations well (I'm not sure models in which the matter and anti-matter are equal would fit at all).
 
  • #74
humanino said:
I really don't get it Marlon. The proton is more likely to decay at higher speed !? Usually, at higher speed, decay is just lowered by lorentz contraction of time. Or : the fastest decay should occur in the rest frame !

I could concieve that there is a dynamical process occurring during the acceleration process.




Barionic number conserved through other conservation laws !?
Oh, by the way : is barionic number conservation not much better experimentally tested than the other conservation laws (with regards to proton's lifetime. I have been checking PDG online, and I am not quite sure.) ?

This is the principle of asymptotic freedom coming from renormalization. It states that the strong force gets weaker when the energyscale gets higher. The strong force gets stronger when the energyscale gets lower. This is why quarks are never allone in the QCD-vacuum. Wellcome to the world of Quarkconfinement

marlon
 
  • #75
I don't see how asymptotic freedom could affect the stability of the proton.

Asymptotic freedom tells you that quarks look like free particles at high energy scales. Which scale ? In the context I am working in, Deep Inelastic Scattering (DIS), one typically has an lepton beam incident on an hydrogen target. The lepton exchange a virtual boson with (one of the quarks inside) the target. The energy scale at which one probes the hadronic structure is typically given by the invariant mass of the virtual particle. For instance, the mass of the photon exchanged. Upon selecting highly virtual exchanged bosons, one observes free quarks.

I am not working on experiments involving hadronic beams. However, I am still convinced that the decay of any particle is the fastest in the rest frame.
 
  • #76
Again to nitpick, its possible that the proton can decay, even in the minimal standard model. Its just vanishingly small in principle, and again its only a theoretical argument and never been observed.

It has to do with baryon and Lepton # nonconservation from the electroweak sector first discovered by T'Hooft when he was studying topological effects on gauge theories. Its also really hard to quantify, particularly when you add in GUT interactions (that also imply a proton decay) as you end up with monopole contributions that makes things a nice mess.

Despite many attempts to find a proton decay signature, it has still remained elusive. Perhaps the best indirect evidence that this is true lies in the theory and models of Baryogenesis and the emerging field of Leptogenesis.

But if the world was pure QCD, you would never find a single quark anywhere. The force would grow to infinity the further you pull them apart, and our naive guess would be satisfied.
 
  • #77
Haelfix said:
Again to nitpick, its possible that the proton can decay, even in the minimal standard model... It has to do with baryon and Lepton # nonconservation from the electroweak sector first discovered by T'Hooft when he was studying topological effects on gauge theories. Its also really hard to quantify, particularly when you add in GUT interactions (that also imply a proton decay) as you end up with monopole contributions that makes things a nice mess.
This is new to me; would you care to elaborate? My understanding of the standard electroweak model is that quarks couple only to other quarks and leptons to leptons. How would this break down?
 
  • #78
I couldn't find T' Hoofts remarkable paper on SLAC (its in physical review somewhere) upon cursory browsing..

But I did manage to find a few papers that talk a little about these effects.

Briefly:

http://arxiv.org/PS_cache/hep-ph/pdf/9608/9608456.pdf

For more emphasis on astrophysics:

http://arxiv.org/PS_cache/hep-ph/pdf/9603/9603208.pdf
 
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