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Kinematically forbidden channels can set the freeze-out dark matter (DM) relic abundance. These channels are described by DM annihilations into heavier states, which vanish at zero temperature limit, but occur at finite temperatures in the…

High Energy Physics - Phenomenology · Physics 2022-11-30 Kwei-Chou Yang

Many models containing particles which are candidates for dark matter, assume the standard model particles and the dark matter candidates are mediated by a spin-0 particle. At the LHC, one can use these models for dark matter searches. One…

High Energy Physics - Experiment · Physics 2019-03-20 Yoav Afik , Eitan Gozani , Yoram Rozen

We consider a complex scalar field as SIMP dark matter in models with gauged $Z_3$ discrete symmetry appearing as a remnant of dark local $U(1)$. Dark matter (DM) annihilates dominantly by the 3-to-2 scattering, due to the DM cubic coupling…

High Energy Physics - Phenomenology · Physics 2015-08-27 Soo-Min Choi , Hyun Min Lee

Dark matter (DM) interacting with the SM fields via a $Z'-$boson ('$Z'$-portal') remains one of the most attractive WIMP scenarios, both from the theoretical and the phenomenological points of view. In order to avoid the strong constraints…

High Energy Physics - Phenomenology · Physics 2019-06-19 S. Caron , J. A. Casas , J. Quilis , R. Ruiz de Austri

We show in this letter how a heavy $(\mathcal{O}(TeV))$ invisible $Z'$ gauge boson that will practically be out of reach of the Large Hadron Collider (LHC), can be discovered at the future muon collider. The new force carrier has a…

High Energy Physics - Phenomenology · Physics 2024-08-27 Anjan Kumar Barik , Santosh Kumar Rai , Aviral Srivastava

Several models of dark matter suggest the existence of dark sectors consisting of SU(3)_C x SU(2)_L x U(1)_Y singlet fields. These sectors of particles do not interact with the ordinary matter directly but could couple to it via gravity. In…

Several string or GUT constructions motivate the existence of a dark U(1)_D gauge boson which interacts with the Standard Model only through its kinetic mixing. We compute the dark matter abundance in such scenario and the constraints in…

High Energy Physics - Phenomenology · Physics 2014-11-21 Y. Mambrini

We revisit the possibility of light scalar dark matter, in the MeV to GeV mass bracket and coupled to electrons through fermion or vector mediators, in light of significant experimental and observational advances that probe new physics…

High Energy Physics - Phenomenology · Physics 2021-04-14 Céline Bœhm , Xiaoyong Chu , Jui-Lin Kuo , Josef Pradler

Tentative evidence for excess GeV-scale gamma rays from the galactic center has been corroborated by several groups, including the Fermi collaboration, on whose data the observation is based. Dark matter annihilation into standard model…

High Energy Physics - Phenomenology · Physics 2016-10-21 James M. Cline , Grace Dupuis , Zuowei Liu , Wei Xue

In gauge-mediated theories supersymmetry breaking originates in a strongly interacting sector and is communicated to the ordinary sparticles via SU(3)$\times$SU(2)$\times$U(1) carrying ``messenger'' particles. Stable baryons of the strongly…

High Energy Physics - Phenomenology · Physics 2009-10-28 S. Dimopoulos , G. F. Giudice , A. Pomarol

This article provides the calculation of an effective vertex function between a nucleon and a $Z^\prime$ boson that couples preferentially to either the top quark or the third generation of fermions, for the purpose of calculating…

High Energy Physics - Phenomenology · Physics 2016-11-11 Frederick S. Sage , Jason N. E. Ho , T. G. Steele , Rainer Dick

Motivated by the growing evidence for lepton flavour universality violation after the first results from Fermilab's muon $(g-2)$ measurement, we revisit one of the most widely studied anomaly free extensions of the standard model namely,…

High Energy Physics - Phenomenology · Physics 2021-09-15 Debasish Borah , Manoranjan Dutta , Satyabrata Mahapatra , Narendra Sahu

If dark matter (DM) interacts with the Standard Model (SM) via the kinetic mixing (KM) portal, it necessitates the existence of massive, likely $\gsim 1$ TeV, enabler portal matter (PM) particles that carry both dark and SM quantum numbers…

High Energy Physics - Phenomenology · Physics 2022-02-18 Thomas G. Rizzo

If fermionic dark matter (DM) is stabilized by dark $U(1)$ gauge symmetry that is spontaneously broken into its subgroup $Z_2$, the particle contents of the model becomes very rich: DM and excited DM, both of them are Majorana fermions, as…

High Energy Physics - Phenomenology · Physics 2020-10-28 Pyungwon Ko , Toshinori Matsui , Yi-Lei Tang

We study direct detection in simplified models of Dark Matter (DM) in which interactions with Standard Model (SM) fermions are mediated by a heavy vector boson. We consider fully general, gauge-invariant couplings between the SM, the…

High Energy Physics - Phenomenology · Physics 2016-08-26 Francesco D'Eramo , Bradley J. Kavanagh , Paolo Panci

We revisit the two real singlet extension of the Standard Model with a $Z_2\times Z_2^\prime$ symmetry. One of the singlet scalars $S_2$, by virtue of an unbroken $Z_2^\prime$ symmetry, plays the role of a stable dark matter candidate. The…

High Energy Physics - Phenomenology · Physics 2021-06-21 Tanushree Basak , Baradhwaj Coleppa , Kousik Loho

Although it is usually thought that a class of weakly interacting massive particle (WIMP) dark matters (DMs), which have the vector coupling with the $Z$ boson, is denied by null results of the direct DM searches, such WIMP DMs are still…

High Energy Physics - Phenomenology · Physics 2021-08-10 Nobuchika Okada , Osamu Seto

Light axion-like particles occur in many theories of beyond-Standard-Model physics, and may make up some or all of the universe's dark matter. One of the ways they can couple to the Standard Model is through the electromagnetic $F_{\mu\nu}…

High Energy Physics - Phenomenology · Physics 2021-04-14 Robert Lasenby

We compute the bounds on the dark matter (DM) annihilation cross section using the most recent Cosmic Microwave Background measurements from WMAP9, SPT'11 and ACT'10. We consider DM with mass in the MeV-TeV range annihilating 100% into…

Cosmology and Nongalactic Astrophysics · Physics 2013-09-13 Laura Lopez-Honorez , Olga Mena , Sergio Palomares-Ruiz , Aaron C. Vincent
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