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相关论文: Quintessential Axions from a New Confining Force

200 篇论文

The axion particle may or may not exist, but the axion field can be used, as shown here, in an explicitly local formulation of a chiral U(1) gauge theory with both classical and quantum gauge invariance. Nonabelian analogues of axion…

高能物理 - 唯象学 · 物理学 2022-04-01 P. Mitra

Axions arise in many theoretical extensions of the Standard Model of particle physics, in particular the "string axiverse". If the axion masses, $m_a$, and (effective) decay constants, $f_a$, lie in specific ranges, then axions contribute…

宇宙学与河外天体物理 · 物理学 2017-10-18 Matthew J. Stott , David J. E. Marsh , Chakrit Pongkitivanichkul , Layne C. Price , Bobby S. Acharya

First, we present a simple confining abelian pure gauge theory. Classically, its kinetic term is not positive definite, and it contains a simple UV regularized F^4 interaction. This provoques the formation of a condensate ~ F^2 such that,…

高能物理 - 理论 · 物理学 2011-09-13 U. Ellwanger , N. Wschebor

Constantly accumulating observational data continue to confirm that about 70% of the energy density today consists of dark energy responsible for the accelerated expansion of the Universe. We present recent observational bounds on dark…

宇宙学与河外天体物理 · 物理学 2013-11-12 Shinji Tsujikawa

A new gauge force that acts exclusively on neutrinos is proposed. This new force violates neutrino flavors while masses are diagonal, potentially opening a door for a new field theoretical treatment of the neutrino oscillation. The basic…

高能物理 - 唯象学 · 物理学 2012-10-25 HoSeong La

We provide a generic but physically clear discussion of the clustering properties of dark energy models. We explicitly show that in quintessence-type models the dark energy fluctuations, on scales smaller than the Hubble radius, are of the…

天体物理学 · 物理学 2008-11-26 P. P. Avelino , L. M. G. Beca , C. J. A. P. Martins

A number of proposed and ongoing experiments search for axion dark matter with a mass nearing the limit set by small scale structure (${\cal O} ( 10 ^{ - 21 } {\rm eV} ) $). We consider the late universe cosmology of these models, showing…

高能物理 - 唯象学 · 物理学 2021-01-11 Jeff A. Dror , Jacob M. Leedom

We study four dimensional non-abelian gauge theories with classical moduli. Introducing a chemical potential for a flavor charge causes moduli to become unstable and start condensing. We show that the moduli condensation in the presence of…

高能物理 - 理论 · 物理学 2008-11-26 Alex Buchel , Junji Jia , V. A. Miransky

We review current cosmological constraints on the axion. We describe the basic mechanisms by which axions are created in the early universe, focussing on the standard thermal scenario where the dominant process is through axion radiation by…

天体物理学 · 物理学 2016-08-30 R. A. Battye , E. P. S. Shellard

We look at dark energy from a biology inspired viewpoint by means of the Approximate Bayesian Computation (ABC) and late time cosmological observations. We find that dynamical dark energy comes out on top, or in the ABC language naturally…

宇宙学与河外天体物理 · 物理学 2023-06-27 Reginald Christian Bernardo , Daniela Grandón , Jackson Levi Said , Víctor H. Cárdenas

New physics can be light if it is hidden, coupling very weakly to the Standard Model. In this work we investigate the discovery prospects of Abelian hidden sectors in lower-energy fixed-target and high-precision experiments. We focus on a…

高能物理 - 唯象学 · 物理学 2015-03-31 David E. Morrissey , Andrew Paul Spray

We present a formalism to explicitly construct non-Abelian gauge theories on noncommutative spaces (induced via a star product with aconstant Poisson tensor) from a consistency relation. This results in an expansion of the gauge parameter,…

高能物理 - 理论 · 物理学 2011-09-13 Branislav Jurco , Lutz Möller , Stefan Schraml , Peter Schupp , Julius Wess

Axions solve the Strong CP Problem and are a cold dark matter candidate. The combined constraints from accelerator searches, stellar evolution limits and cosmology suggest that the axion mass is in the range $3 \cdot 10^{-3} > m_a >…

高能物理 - 唯象学 · 物理学 2007-05-23 Pierre Sikivie

In higher dimensional gauge theory, we need energies with higher power terms of field strength in order to realize point-wise monopoles. We consider new models with higher power terms of field strength and extraordinary kinetic term of…

高能物理 - 理论 · 物理学 2009-03-12 Hironobu Kihara

Maximal Abelian gauge has been a particular choice to study dynamical generation of off-diagonal gluon masses in QCD. This gauge is a special case of Abelian projection. Massive off-diagonal gluons are considered a clue to Abelian…

高能物理 - 理论 · 物理学 2015-04-24 Haresh Raval , Urjit A. Yajnik

If dark energy --- which drives the accelerated expansion of the universe --- consists of a light scalar field, it might be detectable as a "fifth force" between normal-matter objects, in potential conflict with precision tests of gravity.…

原子物理 · 物理学 2015-08-24 Paul Hamilton , Matt Jaffe , Philipp Haslinger , Quinn Simmons , Holger Müller , Justin Khoury

In this work, we study a new quintessence model associated with non-Abelian gauge fields, minimally coupled to Einstein gravity. This gauge theory has been recently introduced and studied as an inflationary model, called gauge-flation.…

宇宙学与河外天体物理 · 物理学 2018-09-03 A. Mehrabi , A. Maleknejad , V. Kamali

If a global chiral symmetry is explicitly broken by anomalies in nonabelian gauge theories, a pseudo Nambu-Goldstone boson (axion) associated with a spontaneous breakdown of such a global symmetry acquires a mass through nonperturbative…

高能物理 - 唯象学 · 物理学 2009-09-29 Yasunori Nomura , T. Watari , T. Yanagida

We discuss mechanisms for naturally generating GeV-scale hidden sectors in the context of weak-scale supersymmetry. Such low mass scales can arise when hidden sectors are more weakly coupled to supersymmetry breaking than the visible…

高能物理 - 唯象学 · 物理学 2010-04-15 David E. Morrissey , David Poland , Kathryn M. Zurek

Cosmic acceleration is explained quantitatively, as an apparent effect due to gravitational energy differences that arise in the decoupling of bound systems from the global expansion of the universe. "Dark energy" is a misidentification of…

广义相对论与量子宇宙学 · 物理学 2008-11-26 David L. Wiltshire