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Warped conformal field theories (WCFTs) are two-dimensional non-relativistic systems, with a chiral scaling and shift symmetry. We present a detailed derivation of the near-extremal limit for their torus partition function. This limit…

高能物理 - 理论 · 物理学 2023-08-02 Ankit Aggarwal , Alejandra Castro , Stéphane Detournay , Beatrix Mühlmann

We propose and implement a fast, universally applicable method for extracting the angular power spectrum C_l from CMB temperature maps by first estimating the correlation function \xi(\theta). Our procedure recovers the C_l's using N^2 (but…

天体物理学 · 物理学 2007-05-23 Istvan Szapudi , Simon Prunet , Dmitry Pogosyan , Alexander S. Szalay , J. Richard Bond

The recent three-year WMAP data have confirmed the anomaly concerning the low quadrupole amplitude compared to the best-fit \Lambda CDM prediction. We show that, allowing the large-scale spatial geometry of our universe to be…

天体物理学 · 物理学 2008-12-18 L. Campanelli , P. Cea , L. Tedesco

This paper proposes a new method to analyze the spatial structure of urban systems using ideas from fractals. Regarding a system of cities as a set of "particles" distributed randomly on a triangular lattice, we construct a spatial…

物理与社会 · 物理学 2016-06-15 Yanguang Chen , Shiguo Jiang

Various aspects of the connection between cloud cover (CC) and cosmic rays (CR) are analysed. Many features of this connection indicate that there is no direct causal connection between low cloud cover (LCC) and CR in spite of the evident…

地球与行星天体物理 · 物理学 2015-05-13 A. D. Erlykin , G. Gyalai , K. Kudela , T. Sloan , A. W. Wolfendale

Since the publication of the results of the Planck satellite mission in 2013, the local and early universes have been considered to be in tension in respect of the determination of amplitude of the matter density spatial fluctuations…

宇宙学与河外天体物理 · 物理学 2017-11-30 G. Hurier , P. Singh , C. Hernández-Monteagudo

In a tomographic approach, we measure the cross-correlation between the CMB lensing reconstructed from the Planck satellite and the galaxies of the photometric redshift catalogue based on the combination of the South Galactic Cap u-band Sky…

宇宙学与河外天体物理 · 物理学 2020-06-24 Gabriela A. Marques , Armando Bernui

We consider a cosmological model with two scalar fields minimally coupled to gravity which have a mixed kinetic term. Hence, Chiral cosmology is included in our analysis. The coupling function and the potential function, which depend on one…

广义相对论与量子宇宙学 · 物理学 2019-09-04 N. Dimakis , A. Paliathanasis , Petros A. Terzis , T. Christodoulakis

We provide a first principle definition of cosmological correlation functions for a large class of scalar toy models in arbitrary FRW cosmologies, in terms of novel geometries we name {\it weighted cosmological polytopes}. Each of these…

高能物理 - 理论 · 物理学 2025-03-26 Paolo Benincasa , Gabriele Dian

In this article we propose a novel test for statistical anisotropy of the CMB. The test is based on the fact, that the Galactic foregrounds have a remarcably strong symmetry with respect to their antipodal points and with respect to the…

宇宙学与河外天体物理 · 物理学 2015-05-28 P. Naselsky , M. Hansen , J. Kim

The cross-correlation between cosmic microwave background (CMB) gravitational lensing and large-scale structure tracers will be an important cosmological probe in the coming years. Quadratic estimators provide a simple and powerful (if…

宇宙学与河外天体物理 · 物理学 2023-07-10 Giulio Fabbian , Antony Lewis , Dominic Beck

We reconsider the inference of spatial power spectra from angular clustering data and show how to include correlations in both the angular correlation function and the spatial power spectrum. Inclusion of the full covariance matrices…

天体物理学 · 物理学 2009-10-31 Daniel J. Eisenstein , Matias Zaldarriaga

We study the effect of global topology of the spatial geometry on the cosmic microwave background (CMB) for closed flat and closed hyperbolic models in which the spatial hypersurface is multiply connected. If the CMB temperature…

天体物理学 · 物理学 2013-09-06 Kaiki Taro Inoue

The usual formulas for the correlation functions in orthogonal and symplectic matrix models express them as quaternion determinants. From this representation one can deduce formulas for spacing probabilities in terms of Fredholm…

solv-int · 物理学 2009-07-11 Craig A. Tracy , Harold Widom

Galaxy surveys probe both structure formation and the expansion rate, making them promising avenues for understanding the dark universe. Photometric surveys accurately map the 2D distribution of galaxy positions and shapes in a given…

宇宙学与河外天体物理 · 物理学 2017-06-19 Samuel Passaglia , Alessandro Manzotti , Scott Dodelson

Cosmological correlators encode invaluable information about the wavefunction of the primordial universe. In this letter we present a duality between correlators and wavefunction coefficients that is valid to all orders in the loop…

高能物理 - 理论 · 物理学 2025-01-07 David Stefanyszyn , Xi Tong , Yuhang Zhu

Chiral random matrix theory makes very detailed predictions for the spectral correlations of the QCD Dirac operator, both in the bulk of the spectrum and near zero virtuality. These predictions have been successfully tested in lattice QCD…

高能物理 - 格点 · 物理学 2007-05-23 Tilo Wettig

This work examines a relativistic model for the observed inhomogeneities of the large scale structure where the hypothesis that this structure can be described as being a self-similar fractal system is advanced. The concept of hierarchical…

天体物理学 · 物理学 2011-02-11 Marcelo B. Ribeiro

We investigate some of the asymmetries reported in the CMB temperature angular distribution considering the {\Lambda}CDM model in the 3, 5 and 7 year WMAP data. We aim to analyze the 4 quadrants of the ILC CMB maps using 3 Galactic cuts:…

宇宙学与河外天体物理 · 物理学 2012-07-03 Larissa Santos , Thyrso Villela , Carlos Alexandre Wuensche