Large Underground Xenon dark matter experiment/LHC LSP neutr

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Discussion Overview

The discussion revolves around the implications of recent null results from the Large Underground Xenon (LUX) dark matter experiment and the Large Hadron Collider (LHC) on the existence of dark matter candidates, specifically neutralinos and the lightest supersymmetric particle (LSP). The conversation explores theoretical interpretations, potential modifications to existing physics, and the nature of dark matter.

Discussion Character

  • Debate/contested
  • Exploratory
  • Technical explanation
  • Conceptual clarification

Main Points Raised

  • Some participants suggest that the lack of detection of WIMPs implies a significant likelihood that LSPs do not exist as dark matter candidates.
  • Others argue that exclusion limits can be adjusted by reducing coupling constants, which may allow particles to remain undetected in current experiments.
  • There is a discussion about the implications of null results from both LHC and LUX, with some proposing that this might necessitate a reevaluation of Newton's laws or the fundamentals of physics.
  • Some participants note that while no dark matter has been found, the search for dark matter-like particles is complex and involves more than just missing energy signatures.
  • There is mention of alternative dark matter theories, including ultra-light scalar field dark matter and axions, which may align better with current exclusion limits.
  • The classification of dark matter as particle-like or wave-like is debated, with one participant stating that both can be described within quantum field theory.
  • Concerns are raised about the challenges of formulating new theories that satisfy existing experimental constraints.

Areas of Agreement / Disagreement

Participants express a range of views on the implications of the experimental results, with no consensus on the existence of LSPs or neutralinos as dark matter candidates. There is ongoing debate about the nature of dark matter and the adequacy of current theoretical frameworks.

Contextual Notes

Limitations include the dependence on definitions of dark matter candidates, the complexity of experimental signatures, and the unresolved nature of theoretical implications based on current exclusion limits.

Who May Find This Useful

This discussion may be of interest to those studying particle physics, cosmology, and theoretical physics, particularly in the context of dark matter research and the implications of experimental findings.

kodama
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Large Underground Xenon dark matter experiment and LHC have reported a null result on searches for dark matter, with new bounds.

What are the implication of these new bounds on neutralinos and LSP?
 
Hi kodama:
Since there been no other replies to your question, I will try to make a useful comment, based on my non-expert interpretation of articles I found by a brief internet search.

Regarding the LSP.
https://en.wikipedia.org/wiki/Lightest_Supersymmetric_Particle
This article says:
The LSP of supersymmetric models is a dark matter candidate and is a Weakly interacting massive particle (WIMP).
The article
http://www.quantumdiaries.org/2014/...-with-the-large-underground-xenon-experiment/
says no WIMPs were found. Therefore one can conclude that no LSPs were found, and that there is a significant likelihood that they do not exist as a kind of DM.

Re neutralinos,
https://en.wikipedia.org/wiki/Neutralino
seems to be saying that neutralinos are not WIMPs. Therefore it seems reasonable to conclude that the XENON based experiment says nothing about the possibility that neutralinos might exist as a kind of DM.

Regards,
Buzz
 
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Buzz Bloom said:
Therefore one can conclude that no LSPs were found, and that there is a significant likelihood that they do not exist as a kind of DM.
Where would such a significant likelihood come from?
The exclusion limits keep improving, but you can always reduce couplings to make the particles invisible to current experiments.
 
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mfb said:
Where would such a significant likelihood come from?
The exclusion limits keep improving, but you can always reduce couplings to make the particles invisible to current experiments.

what about LHC? no neutralinos detected or produced at 8TEV energies.
 
Last edited:
My post applies to both LHC and direct dark matter searches like XENON.
 
mfb said:
My post applies to both LHC and direct dark matter searches like XENON.
lhc is based on finding missing energy. none found.
 
kodama said:
Large Underground Xenon dark matter experiment and LHC have reported a null result on searches for dark matter, with new bounds.

What are the implication of these new bounds on neutralinos and LSP?
I would think that if dark matter isn't found then perhaps we should be tweaking Newton's laws; I mean besides MOND which is only modifying Newton's laws, perhaps a serious shakeup in the fundamentals of physics is due.
 
kodama said:
lhc is based on finding missing energy. none found.
Missing energy is one part of the signature of possible dark matter-like particles, but the searches are more complex than that.

No dark matter found so far: sure. It would be impossible to miss such a discovery.
MathematicalPhysicist said:
I would think that if dark matter isn't found then perhaps we should be tweaking Newton's laws; I mean besides MOND which is only modifying Newton's laws, perhaps a serious shakeup in the fundamentals of physics is due.
Every new theory has to satify constraints from thousands of measurements. That is a huge challenge. If you just start making up hypotheses, they will fail to agree with many of those experimental results.
 
  • #10
mfb said:
Missing energy is one part of the signature of possible dark matter-like particles, but the searches are more complex than that.

No dark matter found so far: sure. It would be impossible to miss such a discovery.Every new theory has to satify constraints from thousands of measurements. That is a huge challenge. If you just start making up hypotheses, they will fail to agree with many of those experimental results.

isnan===
mfb said:
Missing energy is one part of the signature of possible dark matter-like particles, but the searches are more complex than that.

No dark matter found so far: sure. It would be impossible to miss such a discovery.Every new theory has to satify constraints from thousands of measurements. That is a huge challenge. If you just start making up hypotheses, they will fail to agree with many of those experimental results.

i can understand how changing coupling constants can evade bounds of lux, but lhc?

isn't 8 tev enough to create 10-100 gev neutralinos, detected by missing energy?
 
  • #11
Smaller coupling constants reduce the number of events. If the number is small enough, those events get swamped by background events
 
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  • #12
mfb said:
Where would such a significant likelihood come from?
Hi @mfb:

Thank you for pointing out my careless phraseology.

Perhaps I should have said:
"there is a significant possibility that they do not exist as a kind of DM.​
Is this an acceptable statement?

Regards,
Buzz
 
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  • #13
Well, something particle-like is quite likely based on cosmological observations, but it does not have to be a supersymmetric particle, sure. Supersymmetry does not have to exist at all.
 
  • #14
mfb said:
Well, something particle-like is quite likely based on cosmological observations, but it does not have to be a supersymmetric particle, sure. Supersymmetry does not have to exist at all.

what about scalar dark matter? more wave like than particle
 
  • #15
In particle physics such a classification does not make sense. Both "waves" and "particles" are described with the same framework of quantum field theory.
 
  • #16
mfb said:
In particle physics such a classification does not make sense. Both "waves" and "particles" are described with the same framework of quantum field theory.
how adjustable is the coupling for neutralinos and other WIMPS?
 
  • #17
I'm not a theoretician, but in general the phase spaces are usually larger than the exclusion limits experiments can set.
 
  • #18
mfb said:
I'm not a theoretician, but in general the phase spaces are usually larger than the exclusion limits experiments can set.
are you HEP? i ask bc i wonder if ultra-light scalar field dark matter is perhaps the best theory, esp with current exclusion limits from LUX.

i.e no WIMPS, no DM from 1EV-10TEV

DM is ultra-light scalar field dark matter. no cuspy halos. perhaps axions as well around 10 kuev

how would the SM change if they add ultra-light scalar field dark matter ?
 

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