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Related papers: D-BIonic Screening of Scalar Fields

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We develop a theory of non-linear cosmological perturbations at superhorizon scales for a scalar field with a Lagrangian of the form $P(X,\phi)$, where $X=-\partial^{\mu}\phi\partial_{\mu}\phi$ and $\phi$ is the scalar field. We employ the…

General Relativity and Quantum Cosmology · Physics 2009-01-16 Yu-ichi Takamizu , Shinji Mukohyama

We consider multi-Galileon theory, the most general Galilean invariant theory with $N$ scalar fields linearly coupled to the trace of the stress-energy tensor. We study the behavior of perturbations on a static spherically symmetric…

High Energy Physics - Theory · Physics 2013-05-16 Sebastian Garcia-Saenz

We discuss mimetic gravity theories with direct couplings between the curvature and higher derivatives of the scalar field, up to the quintic order, which were proposed to solve the instability problem for linear perturbations around the…

General Relativity and Quantum Cosmology · Physics 2019-12-18 Alexander Ganz , Nicola Bartolo , Sabino Matarrese

We present a new model of gravity which explicitly breaks Lorentz-invariance by the introduction of a unit time-like vector field, thereby giving rise to an extra (scalar) degree of freedom. We discuss its cosmology, exact solutions and the…

General Relativity and Quantum Cosmology · Physics 2013-01-18 Flavio S. Coelho , Carlos Herdeiro , Shinji Hirano , Yuki Sato

The perturbative treatment of dark matter in structure formation relies on the existence of a well-defined expansion parameter, $k/k_{\rm NL}$, with $k_{\rm NL}$ signalling the onset and ultimately the leading role of non-linearities in the…

Cosmology and Nongalactic Astrophysics · Physics 2019-04-26 Matteo Fasiello , Zvonimir Vlah

We derive scalar effective field theories - Lagrangians, symmetries, and all - from on-shell scattering amplitudes constructed purely from Lorentz invariance, factorization, a fixed power counting order in derivatives, and a fixed order at…

High Energy Physics - Theory · Physics 2015-06-10 Clifford Cheung , Karol Kampf , Jiri Novotny , Jaroslav Trnka

We explore the dynamics of dark energy models based on a Dirac-Born-Infeld (DBI) tachyonic action, studying a range of potentials. We numerically investigate the existence of tracking behaviour and determine the present-day value of the…

Astrophysics · Physics 2009-11-11 Gianluca Calcagni , Andrew R. Liddle

We study Lagrangians with the minimal amount of gauge symmetry required to propagate spin-two particles without ghosts or tachyons. In general, these Lagrangians also have a scalar mode in their spectrum. We find that, in two cases, the…

High Energy Physics - Theory · Physics 2008-11-26 D. Blas

The purpose of this paper is to formulate the Dirac-Born-Infeld (DBI) action in a framework of generalized geometry and clarify its symmetry. A D-brane is defined as a Dirac structure where scalar fields and gauge field are treated on an…

High Energy Physics - Theory · Physics 2013-04-23 Tsuguhiko Asakawa , Shuhei Sasa , Satoshi Watamura

The purpose of this work is to discuss how matter fields are coupled to gravity within the framework of General Relativity. Our particular focus here is on the coupling of scalar field models. In a first step, we suggest a new method for…

General Relativity and Quantum Cosmology · Physics 2026-04-29 Joshua Ritchie

We consider a self-interacting scalar field whose mass saturates the Breitenlohner-Freedman bound, minimally coupled to Einstein gravity with a negative cosmological constant in D \geq 3 dimensions. It is shown that the asymptotic behavior…

High Energy Physics - Theory · Physics 2009-11-10 Marc Henneaux , Cristian Martinez , Ricardo Troncoso , Jorge Zanelli

Galileon fields arise naturally from the decoupling limit of massive gravities, and possess special self-interactions which are protected by a spacetime generalization of Galilean symmetry. We briefly revisit the inflationary phenomenology…

Cosmology and Nongalactic Astrophysics · Physics 2011-10-25 Raquel H. Ribeiro , David Seery

We consider an approach to Brans-Dicke theory of gravity in which the scalar field has a geometrical nature. By postulating the Palatini variation, we find out that the role played by the scalar field consists in turning the space-time…

General Relativity and Quantum Cosmology · Physics 2015-06-18 T. S. Almeida , M. L. Pucheu , C. Romero , J. B. Formiga

The expansion history of the Universe reconstructed from a combination of recent data indicates a preference for a changing Dark Energy (DE) density. Moreover, the DE density appears to be increasing with cosmic time, with its equation of…

Cosmology and Nongalactic Astrophysics · Physics 2020-02-19 Alex Zucca , Levon Pogosian , Alessandra Silvestri , Yuting Wang , Gong-Bo Zhao

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…

High Energy Physics - Phenomenology · Physics 2010-11-11 U. Filobello , A. de la Macorra

Using the superembedding approach, the full supersymmetric effective field theory of the D9-brane, super Born-Infeld theory, is fixed by the so called $\mathcal{F}$-constraint. The odd-odd components of the theory's super field strength,…

High Energy Physics - Theory · Physics 2009-11-07 Sven F. Kerstan

In an Euclidean SU(2) $\otimes$ U(1) gauge theory without fermions, we identify scalar-field variables, functionals of the gauge fields and coming in different representations of isospin, which (i) are of mass dimension one in $d=4$, (ii)…

High Energy Physics - Phenomenology · Physics 2022-01-26 M. Stingl

We present a comprehensive discussion of the consistency of the effective quantum field theory of a single $Z_2$ symmetric scalar field. The theory is constructed from a bare Euclidean action which at a scale much greater than the…

High Energy Physics - Theory · Physics 2009-10-22 R. D. Ball , R. S. Thorne

We study configurations consisting of a gravitating spinor field $\psi$ with a nonlinearity of the type $\lambda\left(\bar\psi\psi\right)^2$. To ensure spherical symmetry of the configurations, we use two spin-$\frac{1}{2}$ fields forming a…

General Relativity and Quantum Cosmology · Physics 2019-04-19 Vladimir Dzhunushaliev , Vladimir Folomeev

The geometric properties of General Relativity are reconsidered as a particular nonlinear interaction of fields on a flat background where the perceived geometry and coordinates are "physical" entities that are interpolated by a patchwork…

Quantum Physics · Physics 2015-01-20 Clifford E. Chafin
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