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We describe a novel duality symmetry of Phi(4)-theory defined on noncommutative Euclidean space and with noncommuting momentum coordinates. This duality acts on the fields by Fourier transformation and scaling. It is an extension, to…

高能物理 - 理论 · 物理学 2008-11-26 Edwin Langmann , Richard J. Szabo

We show that, as a result of non-linear self-interactions, it is feasible, at least in light of the bounds coming from terrestrial tests of gravity, measurements of the Casimir force and those constraints imposed by the physics of compact…

高能物理 - 唯象学 · 物理学 2008-11-26 David F. Mota , Douglas J. Shaw

We study the cosmological evolution of a tachyon scalar field T with a Dirac-Born-Infeld type lagrangian and potential V(T) coupled to a canonically normalized scalar field \phi with an arbitrary interaction term B(T,\phi) in the presence…

高能物理 - 理论 · 物理学 2008-11-26 A. de la Macorra , U. Filobello

The squeezed limit of the primordial curvature bispectrum is an extremely sensitive probe of new physics and encodes information about additional fields active during inflation such as their masses and spins. In the conventional setup,…

高能物理 - 理论 · 物理学 2024-01-23 Ciaran McCulloch , Enrico Pajer , Xi Tong

This study explores the plausibility of an interacting tachyonic scalar, homogeneous in nature, as a promising candidate for dynamic dark energy, offering insights into the observed accelerated expansion of the universe. The…

广义相对论与量子宇宙学 · 物理学 2025-07-16 Tanisha Joshi , S. D Pathak

Cosmological scalar fields coupled to the Standard Model drive temporal variations in the fundamental constants that grow with redshift, positioning the early Universe as a powerful tool to study such models. We investigate the dynamics and…

高能物理 - 唯象学 · 物理学 2025-08-04 Masha Baryakhtar , Olivier Simon , Zachary J. Weiner

Rolling tachyon field models are among the candidates suggested as explanations for the recent acceleration of the Universe. In these models the field is expected to interact with gauge fields and lead to variations of the fine-structure…

宇宙学与河外天体物理 · 物理学 2016-06-28 C. J. A. P. Martins , F. M. O. Moucherek

In this work we study the cosmological evolution of a dark energy model with two scalar fields, i.e. the tachyon and the phantom tachyon. This model enables the equation of state $w$ to change from $w>-1$ to $w<-1$ in the evolution of the…

天体物理学 · 物理学 2009-12-04 Shang-Gang Shi , Yun-Song Piao , Cong-Feng Qiao

We get the same degeneracy relation between $w_0$ and $w_a$ for the tachyon fields as for quintessence and phantom fields. Our results show that the dynamics of scalar fields with different origins becomes indistinguishable when the…

广义相对论与量子宇宙学 · 物理学 2013-09-10 Ximing Chen , Yungui Gong

We study inflation, perturbations, non-gaussinity and late-time cosmological dynamics of a tachyon field both minimally and non-minimally coupled to gravity. By analyzing the parameters space of the model, the viability of the model in…

广义相对论与量子宇宙学 · 物理学 2015-06-16 Kourosh Nozari , Narges Rshidi

The background dynamical evolution of a universe filled with matter and a cosmological scalar field is analyzed employing dynamical system techniques. After the phenomenology of a canonical scalar field with exponential potential is…

广义相对论与量子宇宙学 · 物理学 2014-04-23 Nicola Tamanini

Scalar field dynamics may give rise to a nonzero cosmological variation of fundamental constants. Within different scenarios based on the unification of gauge couplings, the various claimed observations and bounds may be combined in order…

高能物理 - 唯象学 · 物理学 2010-04-21 Thomas Dent , Steffen Stern , Christof Wetterich

The evolution of scalar perturbations is studied for 2-component (non-relativistic matter and dark energy) cosmological models at the linear and non-linear stages. The dark energy is assumed to be the scalar field with either classical or…

天体物理学 · 物理学 2015-05-13 O. Sergijenko , Yu. Kulinich , B. Novosyadlyj , V. Pelykh

We illustrate how form-invariance transformations can be used for constructing phantom cosmologies from standard scalar field universes. First, we discuss how to relate two flat Friedmann-Robertson-Walker cosmologies with different…

广义相对论与量子宇宙学 · 物理学 2009-11-10 L. P. Chimento , Ruth Lazkoz

Scale factor duality, a truncated form of time dependent T-duality, is a symmetry of string effective action in cosmological backgrounds interchanging small and large scale factors. The symmetry suggests a cosmological scenario…

高能物理 - 理论 · 物理学 2009-10-31 Ram Brustein

The relationship between the sources of physical fields and the fields themselves is investigated with regard to the coupling of topological information between them. A class of field theories that we call topological field theories is…

高能物理 - 理论 · 物理学 2007-05-23 David Delphenich

There have been thousands of cosmological models for our early universe proposed in the literature, and many of them claimed to be able to give rise to scale-invariant power spectrum as was favored by the observational data. It is thus…

广义相对论与量子宇宙学 · 物理学 2021-09-15 Jiaming Shi , Zheng Fang , Taotao Qiu

We study the cosmological evolution of a tachyon scalar field T with a Dirac- Born- Infeld type lagrangian and potential V (T) coupled to a canonically normalized scalar field with an arbitrary but factorizeable interaction potential B…

高能物理 - 唯象学 · 物理学 2010-11-11 U. Filobello , A. de la Macorra

The existence of dark energy is essential to explain the cosmic accelerated expansion. We consider a homogenous interacting tachyonic scalar field as a possible candidate for the dynamical dark energy. The interaction between the tachyonic…

广义相对论与量子宇宙学 · 物理学 2023-05-02 V K Ojha , Adithya A Rao , S D Pathak

In this paper, we compare the scalar field dynamics in axion-like and power law potentials for both positive and negative values of the exponents. We find that, for positive exponents, both the potentials exhibit similar scalar field…

宇宙学与河外天体物理 · 物理学 2024-05-10 Md. Wali Hossain , Afaq Maqsood