The whole low energy SUSY theory appears to be in trouble. The breaking of 
SUSY as the TeV scale appears not to work. This eliminates the neutralino, 
which is a condensate of supersymmetric partners of the Z particle and 
photon, appears to not exist. This does remove to a fair degree a SUSY 
predicted WIMP particle, the neutralino. 

LC

On Friday, October 29, 2021 at 10:20:20 AM UTC-5 jessem wrote:

> When you say "WIMPs are most likely ruled out" is that related to failure 
> to find supersymmetric particles at LHC? (Correct me if I'm wrong, but my 
> understanding was that many physicists hoped supersymmetry would solve the 
> 'naturalness problem' of the weak energy scale in a way that required 
> supersymmetric particles to have masses in that range, but advocates of the 
> landscape model like Susskind thought there needn't be any 'explanation' 
> for the energy scales of different forces beyond the anthropic principle.) 
> Or are there other reasons to rule them out, like cosmological simulations 
> based on WIMPs being unable to match certain cosmological observations 
> about the real universe?
>
> Jesse
>
> On Fri, Oct 29, 2021 at 7:15 AM Lawrence Crowell <goldenfield...@gmail.com> 
> wrote:
>
>> On Thursday, October 28, 2021 at 9:08:55 PM UTC-5 johnk...@gmail.com 
>> wrote:
>>
>>> Lawrence, any guesses as to what Dark  Matter could be?  Nobody can find 
>>> any evidence of WIMPS and now sterile neutrinos seems to have bit the 
>>> dust. Would you bet your money on Axions, or some modification of General 
>>> Relativity (teleparallel gravity perhaps) or none of the above?
>>>
>>> John K Clark
>>>
>>> ==========
>>>
>>>
>>>
>> I have no commitment to any particular theory. Dark matter might turn out 
>> to be some new physics involving mass-energy in an entirely different form 
>> from what we traditionally know as particles or fields. Dark energy is most 
>> likely some sort of vacuum energy, where the big unknown is how the vacuum 
>> energy is so small compared to what QFT predicts. Dark matter is not 
>> homogeneous and isotropic as is dark energy that is presumed to give the de 
>> Sitter-like expansion curvature. Yet it is still possible that dark energy 
>> is some vacuum type of physics. I have pondered that the large energy 
>> excess we expect for dark energy might in fact be some localized form of 
>> vacuum energy that condensed in the early universe, and this excess remains 
>> as DM. 
>>
>> The phenomenologies proposed so far seem to be falling apart. WIMPs are 
>> mostly likely ruled out. Sterile neutrinos appear to be gone. Axions remain 
>> a possibility, though so far attempts to detect them have come up null. As 
>> a result the most honest thing that can be said is we really have no 
>> certainty about the nature of DM.
>>
>> LC
>>
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