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相关论文: Effects of Nonlinear Dispersion Relations on Non-G…

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We use the BBGKY hierarchy equations to calculate, perturbatively, the lowest order nonlinear correction to the two point correlation and the pair velocity for Gaussian initial conditions in a critical density matter dominated cosmological…

天体物理学 · 物理学 2009-10-28 Somnath Bharadwaj

We study a particular nonlinear dispersion relation $\omega_p(k_p)$ -- a series expansion in the physical wavenumber $k_p$ -- for modeling first-order corrections in the equation of motion of a test scalar field in a de Sitter spacetime…

广义相对论与量子宇宙学 · 物理学 2009-02-26 S. E. Joras , G. Marozzi

In minisuperspace quantum cosmology, the Lorentzian path integral formulations of the no-boundary and tunneling proposals have recently been analyzed. But it has been pointed out that the wave function of linearized perturbations around a…

广义相对论与量子宇宙学 · 物理学 2023-02-14 Hiroki Matsui , Shinji Mukohyama , Atsushi Naruko

We study field theories on the noncommutative Minkowski space with noncommuting time. The focus lies on dispersion relations in quantized interacting models in the Yang-Feldman formalism. In particular, we compute the two-point correlation…

高能物理 - 理论 · 物理学 2007-07-17 Jochen Zahn

The nonlinear corrections to the Golec-Biernat Wusthoff (GBW) and Bartels- Golec- Kowalski (BGK) models, as discussed by Peredo-Hentschinski [M.A.Peredo and M.Hentschinski, Phys.Rev.D{109}, 014032 (2024)], are analyzed in terms of the gluon…

高能物理 - 唯象学 · 物理学 2025-08-05 G. R. Boroun , B. Rezaei

In Schroedinger picture we study the possible effects of trans-Planckian physics on the quantum evolution of massive non-minimally coupled scalar field in de Sitter space. For the nonlinear Corley-Jacobson type dispersion relations with…

广义相对论与量子宇宙学 · 物理学 2015-09-30 Jung-Jeng Huang

In recent years Planck-scale modifications of the dispersion relation have been attracting increasing interest also from the viewpoint of possible applications in astrophysics and cosmology, where spacetime curvature cannot be neglected.…

高能物理 - 理论 · 物理学 2015-12-30 Giacomo Rosati , Giovanni Amelino-Camelia , Antonino Marciano , Marco Matassa

We derive the expressions for the 1-loop corrections in cosmological, Eulerian, perturbation theory to the matter bispectrum and to the galaxy bispectrum, assuming local galaxy bias, in presence of non-Gaussian initial conditions. We…

宇宙学与河外天体物理 · 物理学 2013-05-29 Emiliano Sefusatti

We study dispersion relations in the noncommutative \phi^3 and Wess-Zumino model in the Yang-Feldman formalism at one-loop order. Nonplanar graphs lead to a distortion of the dispersion relation. We find that the strength of this effect is…

高能物理 - 理论 · 物理学 2009-04-17 Claus Doescher , Jochen Zahn

In the Horndeski's most general scalar-tensor theories, we derive the three-point correlation function of scalar non-Gaussianities generated during single-field inflation in the presence of slow-variation corrections to the leading-order…

高能物理 - 理论 · 物理学 2015-06-12 Antonio De Felice , Shinji Tsujikawa

We investigate the insensitivity of the predictions of inflationary models with respect to modifications of Planck energy physics. The modification we consider consists in replacing the usual dispersion relation by nonlinear ones. This way…

天体物理学 · 物理学 2009-11-06 J. C. Niemeyer , R. Parentani

A feasible mechanism of unitarization of amplitudes of deep inelastic scattering at small values of Bjorken $x$ is the gluon fusion. However, its efficiency depends crucially on the vacuum color screening effect which accompanies the…

高能物理 - 唯象学 · 物理学 2015-06-04 R. Fiore , P. V. Sasorov , V. R. Zoller

We use the results of ultra-precise cold-atom-recoil experiments to constrain the form of the energy-momentum dispersion relation, a structure that is expected to be modified in several quantum-gravity approaches. Our strategy of analysis…

广义相对论与量子宇宙学 · 物理学 2009-11-07 Giovanni Amelino-Camelia , Claus Laemmerzahl , Flavio Mercati , Guglielmo M. Tino

A quantum linear Boltzmann equation is proposed, constructed in terms of the operator-valued dynamic structure factor of the macroscopic system the test particle is interacting with. Due to this operator structure it is a non-Abelian linear…

量子物理 · 物理学 2009-11-07 Bassano Vacchini

Gravitational clustering is an intrinsically non-linear process that generates significant non-Gaussian signatures in the density field. We consider how these affect power spectrum determinations from galaxy and weak-lensing surveys.…

天体物理学 · 物理学 2008-11-26 Roman Scoccimarro , Matias Zaldarriaga , Lam Hui

Dispersion relations are nonperturbative formulas that relate the ultraviolet and infrared behavior of an observable with wide-ranging applications applications in linear response theory, quantum field theory scattering amplitudes, and…

高能物理 - 理论 · 物理学 2025-11-19 Dean Carmi , Javier Moreno , Shimon Sukholuski

We show that the relativistic effects are negligibly small in the non-linear density and velocity bispectra. Although the non-linearities of Einstein equation introduce additional non-linear terms to the Newtonian fluid equations, the…

宇宙学与河外天体物理 · 物理学 2014-05-28 Sang Gyu Biern , Jinn-Ouk Gong , Donghui Jeong

The possibility that the scale-invariant inflationary spectrum may be modified due to the hidden assumptions about the Planck scale physics -- dubbed as trans-Planckian inflation -- has received considerable attention. To mimic the possible…

高能物理 - 理论 · 物理学 2009-11-11 S. Shankaranarayanan , Musongela Lubo

In this Letter we study the dependence of the spectrum of fluctuations in inflationary cosmology on possible effects of trans-Planckian physics, using the Corley/Jacobson dispersion relations as an example. We compare the methods used in…

高能物理 - 理论 · 物理学 2009-11-07 Jerome Martin , Robert H. Brandenberger

Inflationary models predicting abundant primordial black holes (PBHs) and large amplitude of scalar-induced gravitational waves (SIGWs) often rely on amplified fluctuations over limited scales, typically driven by phase transitions,…

宇宙学与河外天体物理 · 物理学 2025-12-15 Mohammad Hossein Namjoo , Bahar Nikbakht
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