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相关论文: Detecting Chameleons through Casimir Force Measure…

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We report on a proposal aimed at measuring the Casimir force in a cylinder-plane configuration. The Casimir force is evaluated including corrections due to finite parallelism, conductivity, and temperature. The range of validity of the…

We carry out a realistic, yet simple, calculation of the Casimir-Polder interaction in the presence of a metallic shield in order to aid the design of experiments to test non-Newtonian gravity. In particular, we consider a rubidium atom…

量子物理 · 物理学 2021-02-02 Robert Bennett , D. H. J. O'Dell

A key goal in cosmology in the upcoming decade will be to form a better understanding of the accelerated expansion of the Universe. Upcoming surveys, such as the Vera C. Rubin Observatory's 10-year Legacy Survey of Space and Time (LSST),…

广义相对论与量子宇宙学 · 物理学 2022-11-29 Andrius Tamosiunas , Chad Briddon , Clare Burrage , Alan Cutforth , Adam Moss , Thomas Vincent

The physical origin of the Casimir force is connected with the existence of zero-point and thermal fluctuations. The Casimir effect is very general and finds applications in various fields of physics. This review is limited to the rapid…

其他凝聚态物理 · 物理学 2014-11-18 G. L. Klimchitskaya , U. Mohideen , V. M. Mostepanenko

We investigate the possibility of measuring the thermal Casimir force and its gradient in the configuration of a plate and a microfabricated cylinder attached to a micromachined oscillator. The Lifshitz-type formulas in this configuration…

量子物理 · 物理学 2015-05-20 R. S. Decca , E. Fischbach , G. L. Klimchitskaya , D. E. Krause , D. Lopez , V. M. Mostepanenko

Understanding gravity in the framework of quantum mechanics is one of the great challenges in modern physics. Along this line, a prime question is to find whether gravity is a quantum entity subject to the rules of quantum mechanics. It is…

Modifications of general relativity provide an alternative explanation to dark energy for the observed acceleration of the universe. We review recent developments in modified gravity theories, focusing on higher dimensional approaches and…

宇宙学与河外天体物理 · 物理学 2015-05-18 Bhuvnesh Jain , Justin Khoury

We present a Casimir force setup based on an all-optical ferrule-top sensor. We demonstrate that the instrument can be used to measure the gradient of the Casimir force between a gold coated sphere and a gold coated plate with results that…

量子物理 · 物理学 2011-04-07 P. Zuurbier , S. de Man , G. Gruca , K. Heeck , D. Iannuzzi

We calculate exactly the Casimir force between a spherical particle and a plane, both with arbitrary dielectric properties, in the non-retarded limit. Using a Spectral Representation formalism, we show that the Casimir force of a sphere…

量子物理 · 物理学 2007-05-23 Cecilia Noguea , Carlos E. Roman-Velazquez

We consider the Casimir force including all important corrections to it for the configuration used in a recent experiment employing an atomic force microscope. We calculate the long-range hypothetical forces due to the exchange of light and…

高能物理 - 唯象学 · 物理学 2008-11-26 M. Bordag , B. Geyer , G. L. Klimchitskaya , V. M. Mostepanenko

We investigate the behavior of the fifth force in voids in chameleon models using the spherical collapse method. Contrary to Newtonian gravity, we find the fifth force is repulsive in voids. The strength of the fifth force depends on the…

宇宙学与河外天体物理 · 物理学 2013-05-24 Joseph Clampitt , Yan-Chuan Cai , Baojiu Li

We constrain the Chameleon \textit{screening} mechanism in galaxy clusters, essentially obtaining limits on the coupling strength $\beta$ and the asymptotic value of the field $\phi_{\infty}$. For this purpose, we utilized a collection of…

宇宙学与河外天体物理 · 物理学 2023-08-16 Yacer Boumechta , Balakrishna S. Haridasu , Lorenzo Pizzuti , Minahil Adil Butt , Carlo Baccigalupi , Andrea Lapi

A recent experiment [J.L. Garrett et al., Phys. Rev. Lett {\bf 120}, 040401 (2018)] measured for the first time the gradient of the Casimir force between two gold spheres at room temperature. The theoretical analysis of the data was carried…

量子物理 · 物理学 2018-04-16 Giuseppe Bimonte

The physics of the "dark energy" that drives the current cosmological acceleration remains mysterious, and the dark sector may involve new light dynamical fields. If these light scalars couple to matter, a screening mechanism must prevent…

宇宙学与河外天体物理 · 物理学 2015-06-15 Adrienne L. Erickcek , Neil Barnaby , Clare Burrage , Zhiqi Huang

We compare theoretical expectations for the Casimir force with the results of precise measurements. The force is calculated at finite temperature for multilayered covering of the bodies using the Lifshitz theory. We argue that the…

量子物理 · 物理学 2007-05-23 V. B. Svetovoy , M. V. Lokhanin

The physical origin of the dark energy that causes the accelerated expansion rate of the universe is one of the major open questions of cosmology. One set of theories postulates the existence of a self-interacting scalar field for dark…

宇宙学与河外天体物理 · 物理学 2016-03-23 K. Li , M. Arif , D. G. Cory , R. Haun , B. Heacock , M. G. Huber , J. Nsofini , D. A. Pushin , P. Saggu , D. Sarenac , C. B. Shahi , V. Skavysh , W. M. Snow , A. R. Young

We propose a definitive test of whether plates involved in Casimir experiments should be modeled with ballistic or diffusive electrons--a prominent controversy highlighted by a number of conflicting experiments. The unambiguous test we…

量子物理 · 物理学 2015-06-30 Andrew A. Allocca , Justin H. Wilson , Victor Galitski

Theories of gravity that incorporate new scalar degrees of freedom typically require screening mechanisms to ensure consistency with Solar System tests. One widely-studied mechanism -- the chameleon -- can lead to violations of the…

星系天体物理 · 物理学 2020-11-24 A. P. Naik , N. W. Evans , E. Puchwein , H. Zhao , A. -C. Davis

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…

高能物理 - 唯象学 · 物理学 2024-03-28 Tanmoy Kumar , Sourov Roy

Current acceleration of the cosmic expansion leads to coincidence as well as fine-tuning issues in the framework of general relativity. Dynamical scalar fields have been introduced in response of these problems, some of them invoking…

宇宙学与河外天体物理 · 物理学 2015-12-25 Sandrine Schlogel , Sebastien Clesse , Andre Fuzfa
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