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Modifications to electrodynamics from physics beyond the Standard Model can be tested to a high accuracy. Here we use two setups to place bounds on hidden photons, an Abelian boson kinetically mixed with the photon. The first setup involves…

High Energy Physics - Phenomenology · Physics 2020-11-16 D. Kroff , P. C. Malta

Atomic interferometry can be used to probe dark energy models coupled to matter. We consider the constraints coming from recent experimental results on models generalising the inverse power law chameleons such as $f(R)$ gravity in the large…

Cosmology and Nongalactic Astrophysics · Physics 2016-12-07 Philippe Brax , Anne-Christine Davis

In general, modified gravity theories are modifications or extensions of Einstein's general relativity. Some of them give rise to additional scalar degrees of freedom in Nature. If these scalar fields exist and are light enough, they should…

General Relativity and Quantum Cosmology · Physics 2019-12-12 Christian Käding

A new scalar particle with generic couplings to the standard-model particles is a possible source for the lepton anomalous magnetic moment and the violation of the weak equivalence principle. Here, one-loop contributions to the lepton…

High Energy Physics - Phenomenology · Physics 2025-09-12 Xitong Mei , Dongfeng Gao , Wei Zhao , Jin Wang , Mingsheng Zhan

Models where the accelerated expansion of our Universe is caused by a quintessence scalar field are reviewed. In the framework of high energy physics, the physical nature of this field is discussed and its interaction with ordinary matter…

Astrophysics · Physics 2009-06-23 Jerome Martin

We consider a noncommutative standard model with a minimal coupling scalar field and a dynamical deformation between the canonical momenta of its scale factor and scalar field, and a chameleon model with a non-minimally coupling scalar…

General Relativity and Quantum Cosmology · Physics 2018-05-25 Nasim Saba , Mehrdad Farhoudi

Atom interferometry experiments are searching for evidence of chameleon scalar fields with ever-increasing precision. As experiments become more precise, so too must theoretical predictions. Previous work has made numerous approximations to…

Cosmology and Nongalactic Astrophysics · Physics 2016-08-31 Benjamin Elder , Justin Khoury , Philipp Haslinger , Matt Jaffe , Holger Müller , Paul Hamilton

Experimental searches for new, "fifth" forces are attracting a lot of attention because they allow to test theoretical extensions to the standard model. Here, we report a new experimental search for possible fifth forces, specifically…

Atomic Physics · Physics 2022-12-13 Kai Wei , Wei Ji , Changbo Fu , Arne Wickenbrock , Jiancheng Fang , Victor Flambaum , Dmitry Budker

We present a cursory overview of chameleon models of dark energy and their laboratory tests with an emphasis on optical and Casimir experiments. Optical experiments measuring the ellipticity of an initially polarised laser beam are…

High Energy Physics - Phenomenology · Physics 2009-11-06 Philippe Brax , Carsten van de Bruck , Anne-Christine Davis , Douglas Shaw

In the paper energy dependence of femtoscopy characteristics of pion emission region at freeze-out is investigated for collisions of various ions and for all experimentally available energies. For the first time the normalized values of…

Nuclear Experiment · Physics 2016-05-17 V. A. Okorokov

We review some of the properties of chameleon theories. Chameleon fields are gravitationally coupled to matter and evade gravitational tests thanks to two fundamental properties. The first one is the density dependence of the chameleon…

Astrophysics · Physics 2007-09-13 Ph. Brax , C. van de Bruck , A. C. Davis

In chameleon gravity, there exists a light scalar field that couples to the trace of the stress-energy tensor in such a way that its mass depends on the ambient matter density, and the field is screened in local, high-density environments.…

Cosmology and Nongalactic Astrophysics · Physics 2016-12-09 Carisa Miller , Adrienne L. Erickcek

We use previously obtained experimental results by neutron interferometry to effectively constrain the parameter space of several prominent dark energy models. This investigation encompasses the environment-dependent dilaton field, a…

High Energy Physics - Phenomenology · Physics 2024-02-23 Hauke Fischer , Christian Käding , Hartmut Lemmel , Stephan Sponar , Mario Pitschmann

We investigate the landscape of constraints on MeV-GeV scale, hidden U(1) forces with nonzero axial-vector couplings to Standard Model fermions. While the purely vector-coupled dark photon, which may arise from kinetic mixing, is a…

High Energy Physics - Phenomenology · Physics 2017-05-24 Yonatan Kahn , Gordan Krnjaic , Siddharth Mishra-Sharma , Tim M. P. Tait

Dark energy models, such as the chameleon, where the acceleration of the expansion of the universe results from the dynamics of a scalar field coupled to matter, suffer from the potential existence of a fifth force. Three known mechanisms…

High Energy Physics - Phenomenology · Physics 2013-05-30 Philippe Brax , Axel Lindner , Konstantin Zioutas

Scalars and pseudoscalars with masses in the MeV to GeV range are of interest in different extensions of the Standard Model. Such particles are often associated with dark matter, the strong CP problem and the $\left(g-2\right)_{\mu}$…

High Energy Physics - Phenomenology · Physics 2024-10-28 Aleksandr Pustyntsev , Marc Vanderhaeghen

Background: The recent disagreement between the proton charge radius extracted from Lamb shift measurements of muonic and electronic hydrogen invites speculation that new physics may be to blame. Several proposals have been made for new…

High Energy Physics - Phenomenology · Physics 2013-05-30 Carl E. Carlson , Benjamin C. Rislow

The stability of scalar quintessence potentials under quantum fluctuations is investigated both for uncoupled models and models with a coupling to fermions. We find that uncoupled models are usually stable in the late universe. However, a…

Astrophysics · Physics 2007-05-23 Michael Doran , Joerg Jaeckel

We consider static, spherically symmetric equilibrium configurations consisting of fermionic dark matter nonminimally coupled to dark energy in the form of a quintessence scalar field. With the scalar field coupling function, the form of…

Solar and Stellar Astrophysics · Physics 2013-09-10 Vladimir Folomeev , Ascar Aringazin , Vladimir Dzhunushaliev

We consider all possible scalar bilinears, which couple to two fermions of the standard model. The various baryon and lepton number violating couplings allowed by these exotic scalars are studied. We then discuss which ones are constrained…

High Energy Physics - Phenomenology · Physics 2014-11-17 H. V. Klapdor-Kleingrothaus , E. Ma , U. Sarkar
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