English
Related papers

Related papers: Higgs production as a probe of Chameleon Dark Ener…

200 papers

Chameleon dark energy models are a popular alternative to the standard cosmological constant model. These models consist of a new light degree of freedom, called chameleon, with a density dependent mass and a non-trivial coupling to both…

High Energy Physics - Phenomenology · Physics 2024-03-28 Tanmoy Kumar , Sourov Roy

The next generation electron-positron colliders are designed for precision studies of the Standard Model and its extensions, in particular in the Higgs sector. We consider the potential for discovery of composite Higgs models in Higgs pair…

High Energy Physics - Phenomenology · Physics 2021-10-14 A. Bharucha , G. Cacciapaglia , A. Deandrea , N. Gaur , D. Harada , F. Mahmoudi , K. Sridhar

Dark energy is frequently modelled as an additional dynamical scalar field component in the Universe, referred to as "quintessence", which drives the late-time acceleration. Furthermore, the quintessence field may be coupled to dark matter…

Cosmology and Nongalactic Astrophysics · Physics 2023-09-12 Daniela Palma , Graeme N. Candlish

We propose that dark energy in the form of a scalar field could effectively couple to dark matter inhomogeneities. Through this coupling energy could be transferred to/from the scalar field, which could possibly enter an accelerated regime.…

Cosmology and Nongalactic Astrophysics · Physics 2016-04-25 Valerio Marra

We explore the possibility that, while the Higgs mechanism provides masses to the weak-gauge bosons at the electroweak scale as in the standard model, fermion masses are generated by an unknown mechanism at a higher energy scale. At low…

High Energy Physics - Phenomenology · Physics 2015-03-17 Emidio Gabrielli , Barbara Mele

Many new physics models contain new particles that interact with the Higgs boson. These particles could be produced at the LHC via gluon-gluon fusion with an off-shell Higgs, as well as via the Drell-Yan process if charged under a gauge…

High Energy Physics - Phenomenology · Physics 2015-05-29 A. G. Hessler , A. Ibarra , E. Molinaro , S. Vogl

Chameleons are scalar fields whose mass depends on the environment, specifically on the ambient matter density. While nearly massless in the cosmos, where the matter density is tiny, their mass is of order of an inverse millimeter on Earth,…

Astrophysics · Physics 2009-11-10 Ph. Brax , C. van de Bruck , A. C. Davis , J. Khoury , A. Weltman

The chameleon scalar field is considered as a possible cause of accelerated expansion of the Universe. The chameleon field induces an interaction potential between a particle and a massive body. Previous experiments with falling cold…

Nuclear Experiment · Physics 2015-06-18 Yu. N. Pokotilovski

The chameleon mechanism is a way to give an effective mass to a light scalar field via field self-interaction and interaction with matter. We study this mechanism in models in which the couplings are field dependent and find that the…

Astrophysics · Physics 2009-11-10 Ph. Brax , C. van de Bruck , A. -C. Davis

The weak boson fusion process for neutral Higgs boson production is investigated with particular attention to the accuracy with which the Higgs boson coupling to weak bosons can be determined at CERN Large Hadron Collider (LHC) energies in…

High Energy Physics - Phenomenology · Physics 2009-02-05 Edmond L. Berger , John Campbell

We introduce a light dark photon $A_\mu^\prime$ to the minimal Higgs portal model, by coupling the Higgs boson to "dark QED" containing fermionic dark matter, which gives rise to rich and interesting collider phenomenology. There are two…

High Energy Physics - Phenomenology · Physics 2020-09-16 Anirudh Krovi , Ian Low , Yue Zhang

In scenarios with sterile (right-handed) neutrinos that are subject to an approximate "lepton-number-like" symmetry, the heavy neutrinos (i.e. the mass eigenstates) can have masses around the electroweak scale and couple to the Higgs boson…

High Energy Physics - Phenomenology · Physics 2016-05-25 Stefan Antusch , Eros Cazzato , Oliver Fischer

We show that a recent constraint on the cosmic birefringence effect due to dark energy can be related to the constraints on the coupling of axion dark matter to photon, by relying on a simple model of two-axion alignment mechanism with…

Cosmology and Nongalactic Astrophysics · Physics 2022-10-11 Ippei Obata

We study the possibility to detect heavy physics effects in the interactions of Higgs bosons and the top quark at future colliders using the effective Lagrangian approach. The modification of the interactions may enhance the production of…

High Energy Physics - Phenomenology · Physics 2009-10-30 J. L. Diaz-Cruz , M. A. Perez , J. J. Toscano

We study how collider data and electroweak precision observables affect the parameter space of models including a new dark force mediated by a massive U(1) gauge boson. It acquires mass via a Higgs mechanism in the dark sector which is…

High Energy Physics - Phenomenology · Physics 2012-05-08 Erich Weihs , Jose Zurita

The left-right twin Higgs model predicts a light stable scalar \hat{S}, which is a candidate for WIMP dark matter. We study its scattering on nucleon and find that the cross section is below the CDMS II upper bound but can reach the…

High Energy Physics - Phenomenology · Physics 2010-05-11 Lei Wang , Jin Min Yang

We analyze the behavior of Higgs to diphoton rate and Higgs gluon-gluon production cross section in minimal extensions of the Standard Model comprising new colored vector-like fermions that do not mix with the ordinary ones. We compare…

High Energy Physics - Phenomenology · Physics 2015-06-11 Enrico Bertuzzo , Pedro A. N. Machado , Renata Zukanovich Funchal

The Large Hadron Collider (LHC) has confirmed the Higgs mechanism to be responsible for generating mass in the Standard Model (SM), making it attractive to also consider spontaneous symmetry breaking as the origin of mass for new particles…

High Energy Physics - Phenomenology · Physics 2024-02-20 Torben Ferber , Alexander Grohsjean , Felix Kahlhoefer

A light scalar field framework of dark energy, sometimes referred to as quintessence, introduces a fifth force between normal matter objects. Screening mechanisms, such as the chameleon model, allow the scalar field to be almost massless on…

Cosmology and Nongalactic Astrophysics · Physics 2022-10-05 J. Betz , J. Manley , E. M. Wright , D. Grin , S. Singh

Light scalar fields are expected to arise in theories of high energy physics (such as string theory), and find phenomenological motivations in dark energy, dark matter, or neutrino physics. However, the coupling of light scalar fields to…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-30 R. Pourhasan , N. Afshordi , R. B. Mann , A. C. Davis