How will our world be different if supersymmetry is an unbroken symmetry?

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    Supersymmetry Symmetry
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Discussion Overview

The discussion explores the implications of unbroken supersymmetry on the nature of our world, including the structure of atoms and molecules, the periodic table, and the potential for intelligent life. It encompasses theoretical considerations and speculative scenarios regarding particle interactions and stability.

Discussion Character

  • Exploratory, Technical explanation, Debate/contested

Main Points Raised

  • Some participants propose that if low energy superpartner particles exist, the world would largely resemble our current one, particularly regarding the partners of quarks and leptons.
  • Others argue that the presence of supersymmetric particles could lead to significant changes, such as the potential for atoms composed of selectrons instead of electrons, which would violate the Pauli exclusion principle.
  • A participant notes that if selectrons were stable, the periodic table would not exist as we know it, but questions arise about the stability of these particles.
  • Some contributions suggest that supersymmetric particles would behave as dark matter, while others speculate on the implications of lighter particles having more decay channels, leading to instability in matter.
  • There is a humorous suggestion that truly unbroken supersymmetry would result in a cold, empty world, as non-zero density or temperature would break supersymmetry.
  • Participants discuss the algebraic implications of finite temperature and density breaking Lorentz invariance, which is tied to the breaking of supersymmetry.

Areas of Agreement / Disagreement

Participants express a range of views, with some suggesting the world would remain similar under unbroken supersymmetry, while others contend it would be fundamentally different. The discussion remains unresolved, with multiple competing perspectives on the consequences of supersymmetry.

Contextual Notes

Discussions include assumptions about particle stability, the nature of interactions, and the implications of temperature and density on supersymmetry, which are not fully explored or resolved.

petergreat
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With all kinds of low energy superpartner particles floating around, do we get the same types of atoms and molecules that build up our world? Will the periodic table of elements be larger or smaller? Is this world friendly to the evolution of intelligent life?
 
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petergreat said:
With all kinds of low energy superpartner particles floating around, do we get the same types of atoms and molecules that build up our world? Will the periodic table of elements be larger or smaller? Is this world friendly to the evolution of intelligent life?

More or less the same, at least for the partners of quarks and leptons. The spectrum is full of particles with the same mass charge and spin that the superpartners should have. It is only that they are QCD particles.

A different point is about the partners of gauge bosons, I can not imagine the world with a photino or gauginos.

Which are the interactions of the photino?
 
The world would look rougly the same. The supersymmetric particles would still behave as dark matter. But if there are lighter, normal particles have more decay channels, so various particles are less stable. Probably most matter would break into the lightest supersymmetric particles, which would be fotino, sneutrino and selectron.

A different point is about the partners of gauge bosons, I can not imagine the world with a photino or gauginos.
It's not unlike ours :).
 
The world would look completely different. As one example, you could make atoms with selectrons rather than electrons, and the Pauli principle wouldn't apply. There would be no periodic table to speak of.
 
Vanadium 50 said:
The world would look completely different. As one example, you could make atoms with selectrons rather than electrons, and the Pauli principle wouldn't apply. There would be no periodic table to speak of.
Ok, if selectrons were stable. But if they are not, it is not different from an atom with a pion.

True, with exact supersymmetry, the selectron would be stable. But even a small upwards breaking would do it very different.

But it is good you have grought the selectron example! The electron is the one that does not have a "pionic partner". This is, there are in nature exactly six spin zero, charge minus one, particles:

pion- at 139.5 MeV
kaon- at 493.6 MeV
D- at 1869 MeV
Ds- at 1968 MeV,
B-, at 5279 MeV
Bc-, at 6277 MeV

In the "unbroken supersymmety" scenary, we should get six spin zero, charge minus one, particles: 2 at 105 meV, 2 at 1776 MeV, 2 at 0.510 MeV. The two selectrons are the stable ones in your scenary, and yes it is the difference with the actual world.

It is interesting to note that if the electron were massless and the mass of the muon were exactly the mass of the pion-, the later would be stable at first order.
 
massless charged particles would make EM field short-range.
 
What does that have to do with the OP's question?
 
Just for fun, I suppose the silliest answer would be that our world would be very different because there wouldn't be anything in it. Non-zero density or temperature breaks supersymmetry (basically because bosons are different from fermions). So truly unbroken supersymmetry would require a cold empty world.
 
Physics Monkey said:
Just for fun, I suppose the silliest answer would be that our world would be very different because there wouldn't be anything in it. Non-zero density or temperature breaks supersymmetry (basically because bosons are different from fermions). So truly unbroken supersymmetry would require a cold empty world.

Why does non zero density or temperature break super symmetry?
 
  • #10
Prathyush said:
Why does non zero density or temperature break super symmetry?

There are lots of ways to see that something has to happen. At the algebraic level, finite temperature and density break Lorentz invariance. SUSY inherits this breaking. Physically, a finite density of weakly interacting bosons forms a superfluid while a finite density of weakling interacting fermions forms a Fermi liquid. These things have different heat capacities, for example. Or take the path integral point of view, bosons and fermions get different boundary conditions around the thermal circle leading to different spectra.
 
  • #11
At the algebraic level, finite temperature and density break Lorentz invariance.
Wait, how?
 
  • #12
haael said:
Wait, how?

Let's say either J^{\mu} or T^{\mu \nu} or both may have an expectation value that breaks Lorentz invariance.
 

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