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WIMP in Collider?

  1. Dec 16, 2014 #1
    If we assume that Dark Matter consists (or their fraction) of new particles, WIMPs. Why they aren't detected in colliders?
    I am beginner in a field of DM. Would you recommend some literature?
    Thank you all.
     
  2. jcsd
  3. Dec 16, 2014 #2
    First of all, maybe it would be appropriate to move this thread to the High Energy, Nuclear, Particle Physics subforum.

    Dark matter signals are looked for in collider experiments, such as ATLAS and CMS.

    The role they play in cosmology and astrophysics requires them to be weakly interacting, with no electromagnetic nor strong force/color interactions. Therefore, similar to neutrinos, they are not expected to be detected directly in the detector. However, their presence can be deduced from a momentum imbalance.


    The topic is quite vast.

    Review: http://arxiv.org/pdf/hep-ph/0602187.pdf

    Example of a search and the derived limits: http://arxiv.org/pdf/1210.4491.pdf















     
  4. Dec 16, 2014 #3

    ChrisVer

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    This question is answered simply by experiments. Experiments in colliders have not been able so far to measure "divergencies" from the Standard Model. Also the ways of detection differ by the kind of DM particle you consider.

    First of all, the neutrinos indeed are a part of DM, they consist what we call Hot Dark Matter. The "hot" stands from the fact that these particles decoupled while being relativistic (neutrinos decoupled at temperature [itex]T \approx 0.8~MeV [/itex] so since their masses are small compared to this value, they were relativistic) .

    Now the data we have, if I recall well my value is from Planck's data, the effective number of neutrino species is [itex]N_{eff}=3.3 \pm 0.27[/itex] (here you can find more on these: http://resonaances.blogspot.de). Comparing to the result one obtains by taking into account finite temperature and decoupling effects and Standard Model predictions, [itex]N_{eff}= 3.046[/itex], you can see that in general they are in par. However this also can allow for extra flavors of more massive particles (in case they are fermions, they are called sterile neutrinos). I don't know exactly how can someone look at them in colliders (maybe by looking for new leptonic processes)...

    For example the Supersymmetry gave a candidate for DM, mainly named neutralinos (Lightest supersymmetric particles). For their detection in colliders you get the actual signal and a signal coming from the known Standard Model processes. If you subtract the SM from that signal you can look whether you have an excess of events (coming from new physics) and determine its statistics (whether the excess appears as statistical fluctuations). So far there has not been a detection of such an event excess in the colliders. Mainly we are looking at large missing momenta from the detector, and processes that are not favored in the SM. That is why these particles have not been observed, and the only things you can do is put bounds on the parameter space (the space of the parameters that describe this particle, such as its mass). Reasons for this non-observations vary, they can be much heavier and thus more difficult to create.

    The axionic DM candidates are not searched in a collider. There are several experiments, using their features, that have been conducted to look for them. Especially for the DM axions (cosmological axions), their cold-DM-nature depends a lot on the model itself (and what is the relation between inflation reheating and PQ symmetry breaking temperatures or order) and also allows for a certain window of axionic masses (approximately from [itex]10^{-6} \text{to} 10^{-3} ~eV[/itex]). For that you need more information about inflation (eg BICEP2 and we are also expecting for Planck's data). In particular depending on the order of the Peccei-Quinn symmetry breaking and inflation, you can have domain walls and strings forming as topological deflects or you may have just one vacuum homogenized by the inflation. Now back to searches of axions, ADMX (microwave cavity experiments) is such an experiment and it exploited the axions' property of coupling with the electromagnetic field. So far they haven't been able to observe an axionic signal, and so they have been only able to put boundaries on its couplings/mass. Better resolution experiments are being prepared for the future searches. According to Peccei the next 10 years there will be more dedicated works in looking for that invisible particle [of course that's a personal opinion].
     
  5. Dec 16, 2014 #4

    Chalnoth

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    The short answer is that their interactions with normal matter are weak enough that we can't produce them in large enough quantities in colliders to reliably detect the missing mass (the dark matter would look like a chunk of the reaction energy just disappeared, because we wouldn't actually detect the particle itself). As I understand it, while it is conceivable that the LHC could detect dark matter, it really isn't very likely.
     
  6. Dec 16, 2014 #5
    The latest number combining Planck and Baryon Acoustic Oscillations is Neff =3.04±0.18, in very good agreement with the Standard Model's 3.046, constraining the possibility of additional flavors.
     
  7. Dec 16, 2014 #6
    Thank you all!
    I am enriched.
     
  8. Dec 16, 2014 #7

    Orodruin

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    Let me just add that probably the most smoking gun here would be monojet events. Theoretically, they could happen, e.g., due to quarks annihilating into a dark matter pair with a gluon emitted by one of the initial state quarks. Lots of missing transverse momenta and just one jet to show for it.
     
  9. Dec 17, 2014 #8

    ChrisVer

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    Well thanks for the updating. In fact I looked to find the exact number online, but the data are many... I used this paper:
    http://arxiv.org/pdf/1303.5368v2.pdf
    which dates from 2013. In the introduction he gave the number [itex]N_{eff}=3.30 \pm 0.27[/itex] at [itex]68 \% ~CL[/itex] as a result from the combination of WMAP, Planck, Baryon Acoustic Oscillations and high multipole CMB data . In the conclusions, taking into account the BBN theory, they deduce the bound [itex]N_{eff} <3.56[/itex] at [itex]95 \%~CL[/itex] (all these values they give are taken from a 2013 paper as well, cited [31]).

    If you have any reference for your number, please let me know. Because , since I'm in uni right now, I also checked this (dates April 2014):
    http://iopscience.iop.org/1367-2630/16/6/065002/article
    And I could not find any such small [itex]N_{eff}[/itex]. Except for a small comment on page 17:
    and also for Planck+WP+highL+BAO they give again: [itex] N_{eff}= 3.30^{+0.54}_{-0.51}[/itex] at [itex] 95 \% ~CL[/itex] (in parallel with higher valued results)

    Well yes. It depends on the channel you are looking into. For example there are people looking into the channels of [itex]\tau \tau \rightarrow \text{hadron+hadron~ or~ hadron+lepton}[/itex] decays. Others were looking (I don't remember if they still do) on Flavor changing neutral currents and compare to SM. Intuitevely what you say also seems plausible.
     
    Last edited: Dec 17, 2014
  10. Dec 17, 2014 #9
    My another question was probably said, but generally. Is possible that cold dark matter (I hope I rule out neutrinos) or some of friction is consist of such new particles which can not be created from known particles - SM particles?
     
  11. Dec 17, 2014 #10
    Jester at Resonaances mentioned it-
    http://www.resonaances.blogspot.it/2014/12/planck-whats-new.html

    I assume that he found it in one of the slide presentations at-
    http://www.cosmos.esa.int/web/planck/ferrara2014

    There is a graph, but no number, in the release (in French) at-
    http://www.insu.cnrs.fr/node/5108

    I am downloading the presentations and plan to look through them over the next several days. When I find the one with the number, I'll post a link.

    And, if you haven't seen it, the sum of neutrino masses seems to be constrained to <0.23 eV
     
    Last edited: Dec 17, 2014
  12. Dec 17, 2014 #11

    ChrisVer

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    If you consider SM particles the 3 generations of quarks, the 3 generation of leptons, the 4 vector bosons and the Higgs scalar, then CDM does not contain any of these particles....
     
  13. Dec 17, 2014 #12

    Orodruin

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    I think he means if it is possible that CDM can be created without having a production cross section for any SM particles and I would say yes. In principle there is nothing that demands that it should be possible to create dark matter by colliding SM particles (or at least have a very very very small cross section for such processes). The FIMP (Feebly Interacting Massive Particle) scenario is a scenario where the dark matter has a very small coupling to SM particles. Instead of thermal freeze-out as in the WIMP scenario, dark matter is created through thermal freeze-in in this scenario.
     
  14. Dec 17, 2014 #13

    ChrisVer

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    Well if that's the case... Then I don't know how you would make such a Lagrangian. For example, why would their couplings to SM particles be so suppressed? Also how were they created? as a distinct sector?
    For a practical example, let's say that it is a scalar field, then what doesn't allow it to couple with fermions in a yukawa-interaction? or a pseudoscalar to axial currents?
    In any case you would have to start introducing more symmetries. Extra symmetries is a plausible idea, but after a while, this becomes "boring" (without having an actual observed reason to do so, let's say strong CP-problem).. MOND then would be a more plausible idea (even for me o0)).
     
  15. Dec 17, 2014 #14

    Orodruin

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    I believe it is more common to assume fermions, in which case you can make a singlet out of a fermion bilinear, but have no SM singlet with dimension one to couple it with. Some theories also include additional gauge groups with neutral gauge bosons that mix with the photon, resulting in very weak couplings.

    A relatively nice paper that discusses both the WIMP and FIMP regimes through portal interactions is http://arxiv.org/abs/1112.0493
     
  16. Dec 18, 2014 #15
  17. Dec 18, 2014 #16

    ChrisVer

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    This thing is just crazy o0) All the numbers look pretty low...since it's from Planck 2014, probably I'll have to wait for the Planck's publication in the next days...If that's the case, I'd say that sterile neutrinos seem to get disfavored from the ##N_{eff}## freedom...
     
  18. Dec 19, 2014 #17
    Probably a bit later than the next days. Planck Collaboration now say not December 22 but by end of January, 2015...
    http://www.cosmos.esa.int/web/planck
     
  19. Dec 20, 2014 #18

    ChrisVer

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    And I was expecting it for a presentation in addition to BICEP2....
    :headbang:
     
  20. Dec 20, 2014 #19

    Orodruin

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    To quote Samuel Ting when presenting the AMS-02 results: "Wait!" :rolleyes:
     
  21. Dec 22, 2014 #20
    The Collaboration now says "in early 2015" I'm still hoping for before the end of the Universe.

    And all I wanted for Christmas was the Planck 2014 release and my copy of the new Particle Physics Booklet...
     
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