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相关论文: Scalar Field Action under 4D Isotropic Cut-off and…

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Scalar fields appear in many theories beyond the Standard Model of particle physics. In the early universe, they are exposed to extreme conditions, including high temperature and rapid cosmic expansion. Understanding their behavior in this…

高能物理 - 唯象学 · 物理学 2015-08-21 Yeuk-Kwan E. Cheung , Marco Drewes , Jin U Kang , Jong Chol Kim

We solve isotropic, homogeneous cosmological models containing a self-interacting scalar field. Calculations are performed in four and two-dimensional spacetimes. We find several exact solutions that have an inflationary regime or has a…

广义相对论与量子宇宙学 · 物理学 2012-08-07 Luis P. Chimento , Adriana E. Cossarini , Alejandro S. Jakubi

We explore the cosmic evolution of a scalar field which is identified with the four dimensional spacetime volume. Given a specific form for the Lagrangian of the scalar field, a new holographic dark energy model is present. The energy…

广义相对论与量子宇宙学 · 物理学 2012-05-22 Changjun Gao

We use action-angle variables to describe the basic physics of coherent scalar field oscillations in the expanding universe. These analytical mechanics methods have some advantages, like the identification of adiabatic invariants. As an…

天体物理学 · 物理学 2016-08-30 Eduard Masso , Francesc Rota , Gabriel Zsembinszki

The important role of scalar field in cosmology was noticed by a number of authors. Due to the fact that the scalar field possesses zero spin, it was basically considered in isotropic cosmological models. If considered in an anisotropic…

广义相对论与量子宇宙学 · 物理学 2015-05-01 Yu. P. Rybakov , G. N. Shikin , Yu. A. Popov , Bijan Saha

We present a model where a non-conventional scalar field may act like dark energy leading to cosmic acceleration. The latter is driven by an appropriate field configuration, which result in an effective cosmological constant. The potential…

高能物理 - 理论 · 物理学 2009-11-11 Alex Kehagias

Cosmological solutions of the equations with scalar interaction are being studied. It is shown, that the scalar field can effectively change the equation of state of statistical system, that leads to series of cosmological consequences.

广义相对论与量子宇宙学 · 物理学 2015-03-17 Yu. G. Ignatyev , R. F. Miftakhov

This article examines the analytic solutions of isotropic spacetime with the minimal coupling of scalar field and matter in the context of energy-momentum squared gravity. The scalar field includes quintessence and phantom dark energy…

广义相对论与量子宇宙学 · 物理学 2023-06-21 M. Sharif , M. Zeeshan Gul

This paper reviews the dynamics of an isotropic and homogeneous cosmological scalar field. A general approach to the solution of the Einstein-Klein-Gordon equations is developed, which does not require slow-roll or other approximations.…

广义相对论与量子宇宙学 · 物理学 2025-04-15 J. W. van Holten

Cosmological models of a scalar field with dynamical equations containing fractional derivatives or derived from the Einstein-Hilbert action of fractional order, are constructed. A number of exact solutions to those equations of fractional…

广义相对论与量子宇宙学 · 物理学 2011-08-22 V. K. Shchigolev

There often appear coherently oscillating scalar fields in particle physics motivated cosmological scenarios, which may have rich phenomenological consequences. Scalar fields should somehow interact with background thermal bath in order to…

高能物理 - 唯象学 · 物理学 2013-04-25 Kyohei Mukaida , Kazunori Nakayama

Cosmological scaling solutions, which give rise to a scalar-field density proportional to a background fluid density during radiation and matter eras, are attractive to alleviate the energy scale problem of dark energy. In the presence of…

广义相对论与量子宇宙学 · 物理学 2010-03-25 Junko Ohashi , Shinji Tsujikawa

Dark energy models and modified gravity theories have been actively studied and the behaviors in the solar system have been also carefully investigated in a part of the models. However, the isotropic solutions of the field equations in the…

广义相对论与量子宇宙学 · 物理学 2018-01-24 Jiro Matsumoto

We give a prescription how high energy physics tools can be used to perform scalar dark matter analysis. We also present the analysis results of scalar dark matter in the context of 6 dimensional Effective Field Theory.

高能物理 - 唯象学 · 物理学 2023-12-11 Ayşe Kuday , Ferhat Özok , Erdinç Ulaş Saka

This paper extends the study of the quantum dissipative effects of a cosmological scalar field by taking into account the cosmic expansion and contraction. Cheung, Drewes, Kang and Kim calculated the effective action and quantum dissipative…

高能物理 - 理论 · 物理学 2024-07-18 Hui Xu , Lei Ming , Yeuk-Kwan E. Cheung

Scalar fields are widely used in cosmology, in particular to emulate dark energy, for example in quintessence models, or to explain dark matter, in particular within the fuzzy dark matter model. In addition many scenarios involving…

宇宙学与河外天体物理 · 物理学 2019-12-09 A. Arbey , J. -F. Coupechoux

A dynamical scalar field represents the simplest generalization of a pure Cosmological Constant as a candidate to explain the recent evidence in favour of the accelerated cosmic expansion. We review the dynamical properties of such a…

天体物理学 · 物理学 2011-07-19 C. Baccigalupi , A. Balbi , S. Matarrese , F. Perrotta , N. Vittorio

We investigate spatially flat isotropic cosmological models which contain a scalar field with an exponential potential and a perfect fluid with a linear equation of state. We include an interaction term, through which the energy of the…

天体物理学 · 物理学 2008-11-26 Andrew P. Billyard , Alan A. Coley

We study the interaction between dark matter and dark energy, with dark energy described by a scalar field having a double exponential effective potential. We discover conditions under which such a scalar field driven solution is a late…

广义相对论与量子宇宙学 · 物理学 2015-08-06 Vartika Gupta , Rakesh Kabir , Amitabha Mukherjee , Daksh Lohiya

A cosmic scalar field evolving very slowly in time can account for the observed dark energy of the Universe. Unlike a cosmological constant, an evolving scalar field also has local spatial gradients due to gravity. If the scalar field has a…

宇宙学与河外天体物理 · 物理学 2013-03-01 Michael V. Romalis , Robert R. Caldwell
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