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相关论文: Higgs production as a probe of Chameleon Dark Ener…

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We study models in which a light scalar dark energy particle couples to the gauge fields of the electroweak force, the photon, Z and W bosons. Our analysis applies to a large class of interacting dark energy models, including those in which…

高能物理 - 唯象学 · 物理学 2009-12-08 Philippe Brax , Clare Burrage , Anne-Christine Davis , David Seery , Amanda Weltman

Chameleon dark energy is a matter-coupled scalar field which hides its fifth forces locally by becoming massive. We estimate torsion pendulum constraints on the residual fifth forces due to models with gravitation-strength couplings.…

高能物理 - 唯象学 · 物理学 2012-12-03 Amol Upadhye

Chameleon fields, which are scalar field dark energy candidates, can evade fifth force constraints by becoming massive in high-density regions. However, this property allows chameleon particles to be trapped inside a vacuum chamber with…

高能物理 - 唯象学 · 物理学 2013-05-30 Amol Upadhye , Jason H. Steffen , Aaron S. Chou

We report results from the GammeV Chameleon Afterglow Search---a search for chameleon particles created via photon/chameleon oscillations within a magnetic field. This experiment is sensitive to a wide class of chameleon power-law models…

宇宙学与河外天体物理 · 物理学 2011-01-28 Jason H. Steffen , Amol Upadhye , Al Baumbaugh , Aaron S. Chou , Peter O. Mazur , Ray Tomlin , Amanda Weltman , William Wester

A scalar field dark energy candidate could couple to ordinary matter and photons, enabling its detection in laboratory experiments. Here we study the quantum properties of the chameleon field, one such dark energy candidate, in an…

高能物理 - 唯象学 · 物理学 2015-06-18 Philippe Brax , Amol Upadhye

In chameleon field theories a scalar field can couple to matter with gravitational strength and still evade local gravity constraints due to a combination of self-interactions and the couplings to matter. Originally, these theories were…

宇宙学与河外天体物理 · 物理学 2011-05-02 David F. Mota , Hans A. Winther

The chameleon is a scalar field whose mass depends on the density of its environment. Chameleons are necessarily coupled to matter particles and will excite transitions between atomic energy levels in an analogous manner to photons. When…

高能物理 - 唯象学 · 物理学 2010-12-23 Philippe Brax , Clare Burrage

We propose a low scale leptogenesis scenario in the framework of composite Higgs models supplemented with singlet heavy neutrinos. One of the neutrinos can also be considered as a dark matter candidate whose stability is guaranteed by a…

高能物理 - 唯象学 · 物理学 2021-04-28 M. Ahmadvand

Chameleons are light scalar fields with remarkable properties. Through the interplay of self-interactions and coupling to matter, chameleon particles have a mass that depends on the ambient matter density. The manifestation of the fifth…

宇宙学与河外天体物理 · 物理学 2015-06-16 Justin Khoury

We study the phenomenology of dark matter in the Littlest Higgs model with T-parity after the discovery of Higgs boson. We analyze the relic abundance of dark matter, focusing on the effects of coannihilaitons with T-odd fermions. After…

高能物理 - 唯象学 · 物理学 2015-06-18 Chuan-Ren Chen , Ming-Che Lee , Ho-Chin Tsai

Higgs production in association with a photon at hadron colliders is a rare process, not yet observed at the LHC. We show that this process is sensitive to significant deviations of Higgs couplings to first and second generation SM quarks…

高能物理 - 唯象学 · 物理学 2021-08-16 J. A. Aguilar-Saavedra , J. M. Cano , J. M. No

We report the first results from the GammeV search for chameleon particles, which may be created via photon-photon interactions within a strong magnetic field. Chameleons are hypothesized scalar fields that could explain the dark energy…

Many scenarios beyond the standard model, aiming to solve long-standing cosmological and particle physics problems, suggest that dark matter might experience long-distance interactions mediated by an unbroken dark $U(1)$ gauge symmetry,…

高能物理 - 唯象学 · 物理学 2022-08-02 Sanjoy Biswas , Emidio Gabrielli , Barbara Mele

In this contribution one examines the coupling of dark energy to the gauge fields, to neutrinos, and to the Higgs field. In the first case, one shows how a putative evolution of the fundamental couplings of strong and weak interactions via…

高能物理 - 唯象学 · 物理学 2009-07-24 M. C. Bento , A. E. Bernardini , O. Bertolami

Scalar fields with a "chameleon" property, in which the effective particle mass is a function of its local environment, are common to many theories beyond the standard model and could be responsible for dark energy. If these fields couple…

宇宙学与河外天体物理 · 物理学 2014-11-20 G. Rybka , M. Hotz , L. J Rosenberg , S. J. Asztalos , G. Carosi , C. Hagmann , D. Kinion , K. van Bibber , J. Hoskins , C. Martin , P. Sikivie , D. B. Tanner , R. Bradley , J. Clarke

In view of ongoing measurements of the Higgs-like boson at the LHC and direct searches for dark matter, we explore the possibility of accommodating the potential results in a simple new-physics model with discrete gauge symmetry as well as…

高能物理 - 唯象学 · 物理学 2015-03-20 Cheng-Wei Chiang , Takaaki Nomura , Jusak Tandean

In gauge models with bigger number of Higgs particles their couplings to fermions are more complicated then in the standard model (SM). The influence of the Higgs bosons exchange on the neutrino production cross section in $e^-e^+$…

高能物理 - 唯象学 · 物理学 2011-08-17 J. Gluza , M. Zralek

We explore the collider relevance of a charge-radius coupling among light mesons in composite Higgs models. In particular, we focus of a coupling of the photon to the composite Higgs and a composite singlet, arising from isospin violation…

高能物理 - 唯象学 · 物理学 2022-12-14 G. Cacciapaglia , S. Gascon-Shotkin , A. Lesauvage , N. Manglani , K. Sridhar

Recently, it has been pointed out that two different excesses of events observed at LEP could be interpreted as the CP-even Higgs bosons of the MSSM with masses of approximately 98 and 114 GeV. If this is the case, the entire MSSM Higgs…

高能物理 - 唯象学 · 物理学 2008-11-26 Dan Hooper , Tilman Plehn

We explore a chameleon type of interacting dark matter-dark energy scenario in which a scalar field adiabatically traces the minimum of an effective potential sourced by the dark matter density. We discuss extensively the effect of this…

宇宙学与河外天体物理 · 物理学 2015-08-06 Daniel Boriero , Subinoy Das , Yvonne Y. Y. Wong
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