A 96 GeV scalar tagged to dark matter models

Recently, the CMS Collaboration observed the hint of a resonance decaying to two photons at about 96 GeV with a local significance of 2.8σ. While it is too early to say whether this will stand the test of time, such a resonance can easily be accommodated in many extensions of the Standard Model (SM)...

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Main Authors: Anirban Kundu, Suvam Maharana, Poulami Mondal
Format: Article
Language:English
Published: Elsevier 2020-06-01
Series:Nuclear Physics B
Online Access:http://www.sciencedirect.com/science/article/pii/S0550321320301437
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spelling doaj-fc7da0eca3664adebc0968d595bfd3b72020-11-25T03:22:09ZengElsevierNuclear Physics B0550-32132020-06-01955115057A 96 GeV scalar tagged to dark matter modelsAnirban Kundu0Suvam Maharana1Poulami Mondal2Department of Physics, University of Calcutta, 92 Acharya Prafulla Chandra Road, Kolkata 700009, IndiaDepartment of Physics, University of Calcutta, 92 Acharya Prafulla Chandra Road, Kolkata 700009, IndiaDepartment of Physics, University of Calcutta, 92 Acharya Prafulla Chandra Road, Kolkata 700009, IndiaRecently, the CMS Collaboration observed the hint of a resonance decaying to two photons at about 96 GeV with a local significance of 2.8σ. While it is too early to say whether this will stand the test of time, such a resonance can easily be accommodated in many extensions of the Standard Model (SM). The more challenging part is to tune such an extension so that the required number of diphoton events is reproduced. Assuming that the new resonance is a scalar, we propose that the signal may come either from an ultraviolet complete model with vectorial quarks, or a model involving gluon-scalar and photon-scalar effective operators. We then incorporate this portal to several extensions of the SM that include one or more cold dark matter candidates, and try to investigate how the existence of such a scalar resonance affects the parameter space of such models. As expected, we find that with such a scalar, the parameter space gets more constrained and hence, more tractable. We show how significant constraints can be placed on the parameter space, not only from direct dark matter searches or LHC data but also from theoretical considerations like scattering unitarity or stability of the potential, and discuss some novel features of the allowed parameter space.http://www.sciencedirect.com/science/article/pii/S0550321320301437
collection DOAJ
language English
format Article
sources DOAJ
author Anirban Kundu
Suvam Maharana
Poulami Mondal
spellingShingle Anirban Kundu
Suvam Maharana
Poulami Mondal
A 96 GeV scalar tagged to dark matter models
Nuclear Physics B
author_facet Anirban Kundu
Suvam Maharana
Poulami Mondal
author_sort Anirban Kundu
title A 96 GeV scalar tagged to dark matter models
title_short A 96 GeV scalar tagged to dark matter models
title_full A 96 GeV scalar tagged to dark matter models
title_fullStr A 96 GeV scalar tagged to dark matter models
title_full_unstemmed A 96 GeV scalar tagged to dark matter models
title_sort 96 gev scalar tagged to dark matter models
publisher Elsevier
series Nuclear Physics B
issn 0550-3213
publishDate 2020-06-01
description Recently, the CMS Collaboration observed the hint of a resonance decaying to two photons at about 96 GeV with a local significance of 2.8σ. While it is too early to say whether this will stand the test of time, such a resonance can easily be accommodated in many extensions of the Standard Model (SM). The more challenging part is to tune such an extension so that the required number of diphoton events is reproduced. Assuming that the new resonance is a scalar, we propose that the signal may come either from an ultraviolet complete model with vectorial quarks, or a model involving gluon-scalar and photon-scalar effective operators. We then incorporate this portal to several extensions of the SM that include one or more cold dark matter candidates, and try to investigate how the existence of such a scalar resonance affects the parameter space of such models. As expected, we find that with such a scalar, the parameter space gets more constrained and hence, more tractable. We show how significant constraints can be placed on the parameter space, not only from direct dark matter searches or LHC data but also from theoretical considerations like scattering unitarity or stability of the potential, and discuss some novel features of the allowed parameter space.
url http://www.sciencedirect.com/science/article/pii/S0550321320301437
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