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Scattering amplitudes in $d+2$ dimensions can be recast as correlators of conformal primary operators in a putative holographic CFT$_d$ by working in a basis of boost eigenstates instead of momentum eigenstates. It has been shown previously…

高能物理 - 理论 · 物理学 2024-02-15 Prahar Mitra

The standard cosmological model does not determine the spatial topology of the universe. This article revisits the signature of a non-trivial topology on the properties of the cosmic microwave background anisotropies. We show that the…

宇宙学与河外天体物理 · 物理学 2015-08-19 Ophélia Fabre , Simon Prunet , Jean-Philippe Uzan

Cosmological correlators encode rich information about physics at the Hubble scale and may exhibit characteristic oscillatory signals due to the exchange of massive particles. Although many 1-loop processes, especially those that break de…

高能物理 - 理论 · 物理学 2025-04-22 Zhehan Qin

The AdS/CFT correspondence conjectures a holographic duality between gravity in a bulk space and a critical quantum field theory on its boundary. Tensor networks have come to provide toy models to understand such bulk-boundary…

量子物理 · 物理学 2019-08-13 Alexander Jahn , Marek Gluza , Fernando Pastawski , Jens Eisert

In celestial conformal field theory, gluons are represented by primary fields with dimensions $\Delta=1+i\lambda$, $\lambda\in\mathbb{R}$ and spin $J=\pm 1$, in the adjoint representation of the gauge group. All two- and three-point…

高能物理 - 理论 · 物理学 2023-01-11 Wei Fan , Angelos Fotopoulos , Stephan Stieberger , Tomasz R. Taylor , Bin Zhu

Cosmological correlators encode statistical properties of the initial conditions of our universe. Mathematically, they can often be written as Mellin integrals of a certain rational function associated to graphs, namely the flat space…

A holographic duality is proposed relating quantum gravity on dS_D (D-dimensional de Sitter space) to conformal field theory on a single S^{D-1} ((D-1)-sphere), in which bulk de Sitter correlators with points on the boundary are related to…

高能物理 - 理论 · 物理学 2009-11-07 Andrew Strominger

Physical constants and cosmological parameters could vary with position. On the largest scales such variations would manifest themselves as gradients across our Hubble volume, leading to dipole-modulation of the cosmic microwave…

宇宙学与河外天体物理 · 物理学 2011-08-12 Adam Moss , Douglas Scott , James P. Zibin , Richard Battye

A large fraction of the dwarf satellites orbiting the Andromeda galaxy are surprisingly aligned in a thin, extended and apparently kinematically coherent planar structure. Such a structure is not easily found in simulations based on the…

星系天体物理 · 物理学 2016-06-01 Tobias Buck , Aaron A. Dutton , Andrea V. Macciò

A new, improved version of a cosmic crystallography method for constraining cosmic topology is introduced. Like the circles-in-the-sky method using CMB data, we work in a thin, shell-like region containing plenty of objects. Two pairs of…

宇宙学与河外天体物理 · 物理学 2011-04-19 Hirokazu Fujii , Yuzuru Yoshii

We define the 7D Randall-Sundrum (RS) background and construct the corresponding 6D theory via AdS/CFT duality. In simple approximations, the Friedmann equation derived from 7D RS cosmology and the brane view-point results exactly match.…

高能物理 - 理论 · 物理学 2008-11-26 Liuba Mazzanti

It is proposed that the mathematical formalism that is most appropriate for the study of spatially non-integrable cosmological models is the transverse geometry of a one-dimensional foliation (congruence) defined by a physical observer. By…

广义相对论与量子宇宙学 · 物理学 2007-11-14 David Delphenich

Spiral galaxies are axi-symmetric objects showing 2D-chirality when projected onto a plane. Features in common with tetrahedral molecules are pointed out, in particular the existence of a preferred chiral modality for genetic galaxies as in…

化学物理 · 物理学 2008-11-26 Salvatore Capozziello , Alessandra Lattanzi

The holographic correspondence creates an interface between classical gravitational physics and the dynamics of strongly interacting quantum field theories. This chapter will relate the physics of charged, asymptotically Anti-de Sitter…

高能物理 - 理论 · 物理学 2011-07-11 Sean A. Hartnoll

We derive in this paper expressions for the covariance matrix of the cosmic shear two-point correlation functions which are readily applied to any survey geometry. Furthermore, we consider the more special case of a simple survey geometry…

天体物理学 · 物理学 2009-11-07 Peter Schneider , Ludovic van Waerbeke , Martin Kilbinger , Yannick Mellier

We present a method that uses observations of galaxies to simultaneously constrain cosmological parameters and the galaxy-dark matter connection (aka halo occupation statistics). The latter describes how galaxies are distributed over dark…

宇宙学与河外天体物理 · 物理学 2012-04-05 Surhud More , Frank van den Bosch , Marcello Cacciato , Anupreeta More , Houjun Mo , Xiaohu Yang

The basic observables in cosmology are known as in-in correlators. Recent calculations have revealed that in-in correlators in four dimensional de Sitter space exhibit hidden simplicity stemming from a close relation to scattering…

高能物理 - 理论 · 物理学 2026-03-12 Chandramouli Chowdhury , Arthur Lipstein , Joe Marshall , Jiajie Mei , Ivo Sachs

Homogeneous gravitational wave backgrounds arise as infinite momentum limits of many geometries with a well-understood holographic description. General global aspects of these geometries are discussed. Using exact CFT techniques, strings in…

高能物理 - 理论 · 物理学 2009-11-07 E. Kiritsis , B. Pioline

In many astronomical works, the structure of vector fields is analyzed, such as the differences in the celestial object coordinates in catalogs or the celestial object velocities, by decomposition into vector spherical harmonics (VSH). This…

天体物理仪器与方法 · 物理学 2024-10-10 Zinovy Malkin

Stellar halos around galaxies retain fundamental evidence of the processes which lead to their build up. Sophisticated models of galaxy formation in a cosmological context yield quantitative predictions about various observable…

星系天体物理 · 物理学 2016-09-07 Laura Greggio , Renato Falomo , Michela Uslenghi
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