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Actual Physics behind Mono-X
by Elias Bernreuther, Jan Horak, Tilman Plehn, Anja Butter
This is not the current version.
|As Contributors:||Elias Bernreuther · Tilman Plehn|
|Arxiv Link:||https://arxiv.org/abs/1805.11637v2 (pdf)|
|Date submitted:||2018-06-18 02:00|
|Submitted by:||Plehn, Tilman|
|Submitted to:||SciPost Physics|
Mono-X searches are standard dark matter search strategies at the LHC. First, we show how in the case of initial state radiation they essentially collapse to mono-jet searches. Second, we systematically study mono-X signatures from decays of heavier dark matter states. Direct detection constraints strongly limit our MSSM expectations, but largely vanish for mono-Z and mono-Higgs signals once we include light NMSSM mediators. Finally, the decay topology motivates mono-W-pair and mono-Higgs-pair searches, strengthening and complementing their mono-X counterparts.
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Submission & Refereeing History
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Reports on this Submission
Anonymous Report 2 on 2018-8-1 (Invited Report)
- Cite as: Anonymous, Report on arXiv:1805.11637v2, delivered 2018-08-01, doi: 10.21468/SciPost.Report.546
Serious analysis for collider and astronomical dark matter searches for motivated frameworks beyond the standard model.
Originality: the theoretical frameworks considered in this work have been studied extensively, also for many of the constraints presented here.
This paper considers mono-X signatures arising from non minimal dark sectors. After a review and comparison of mono-X searches from initial state radiation, as it is the case in effective theories for dark matter, the authors describe the theoretical framework in section 3. They consider two cases: the minimal supersymmetric standard model (MSSN) and the next to the minimal supersymmetric standard model (NMSSN). In the same section, they also present the SFITTER framework, which is the setup for the following analysis. The central results are in sections 4 and 5, where the authors combine mono-X searches (with X = Z, W and Higgs) with astrophysical constraints such as relic density and direct and indirect detection. In the former section they study the MSSN, in the latter the NMSSM. Conclusions are given in section 6.
I find this paper clearly written and of good quality. Before recommending its publication, I am asking for two minor revisions. The authors say that direct detection constraints are derived as described in section 3.3. Unless I am missing something, I do not see direct detection discussed in section 3.3. Finally, my last comment is perhaps obvious to the authors, but I think it is important to emphasize this point. It is not fair to treat collider and relic density bounds on an equal footing. As they correctly state in the paper, the lightest stable particle in their framework could be a subdominant contribution to the dark matter and therefore the relic density is just a lower bound on the cross section. More importantly, the relic density calculations performed in this work are based on the assumption of a standard cosmological history. There is no evidence for this, and motivated beyond the standard model frameworks (including moduli in supersymmetric theories) predict deviation from such a simple picture. It is possible to reproduce the observed dark matter relic density for cross sections much larger or much smaller than the WIMP miracle value. While this is a trivial point, I think it is important that the authors state very clearly this caveat.
Report 1 by Tim Tait on 2018-7-4 (Invited Report)
- Cite as: Tim Tait, Report on arXiv:1805.11637v2, delivered 2018-07-03, doi: 10.21468/SciPost.Report.525
1. This article does a comprehensive analysis of the mono-X family of signature, and also applies them to MSSM and NMSSM specific models.
2. The collider analysis is rigorous and well handled and the conclusions are well explained with a mixture of analytical reasoning illustrating numerical results.
3. The results are interesting and suggest some new search strategies such as mono-W-pair which look quite powerful.
1. Throughout, the authors are somewhat guilty of the very common sin of overly fetishizing the freeze-out relic abundance. That is a nice picture for where the amount of WIMP dark matter comes from, but modifications to cosmology or additional particle physics could over-turn it.
In general, this is a valuable contribution to the literature.
1. This is optional, but I would like to see versions of the SFITTER plots without the relic density imposed. (And of course, also to keep the current versions with it imposed).