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相关论文: The Odd-Parity Galaxy Bispectrum

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The observed acceleration of the universe, explained through dark energy, could alternatively be explained through a modification of gravity that would also induce modifications in the evolution of cosmological perturbations. We use new…

宇宙学与河外天体物理 · 物理学 2011-09-16 Ismael Tereno , Elisabetta Semboloni , Tim Schrabback

We show that dynamical Chern-Simons (dCS) gravity imprints a parity-violating signal in primordial scalar perturbations. Specifically, we find that, after dCS amplifies one graviton helicity due to a tachyonic instability, the…

宇宙学与河外天体物理 · 物理学 2023-03-10 Cyril Creque-Sarbinowski , Stephon Alexander , Marc Kamionkowski , Oliver Philcox

Cosmic voids as typical under-density regions in the large scale Universe are known for their hyperbolic properties as an ability to deviate the photon beams. The under-density then is acting as the negative curvature in the hyperbolic…

广义相对论与量子宇宙学 · 物理学 2021-04-07 M. Samsonyan , A. A. Kocharyan , A. Stepanian , V. G. Gurzadyan

Anomalous redshifts of some galactic objects such as binary stars, early-type stars in the solar neighborhood, and O stars in a star clusters are discussed. It is shown that all these phenomena have a common characteristic, that is, the…

综合物理 · 物理学 2013-10-02 Yi-Jia Zheng

The theoretical framework of cosmology is mainly defined by gravity, of which general relativity is the current model. Recent tests of general relativity within the \Lambda Cold Dark Matter (CDM) model have found a concordance between…

宇宙学与河外天体物理 · 物理学 2011-09-30 Radoslaw Wojtak , Steen H. Hansen , Jens Hjorth

The asymmetry in the large-scale distribution of the directions towards spiral galaxies rotate has been observed by multiple telescopes, all show a consistent asymmetry in the distribution of galaxy spin directions as observed from Earth.…

宇宙学与河外天体物理 · 物理学 2024-10-22 Lior Shamir

The origin of the extragalactic gamma-ray background is a pressing cosmological mystery. The Fermi Gamma-Ray Space Telescope has recently measured the intensity and spectrum of this background; both are substantially different from previous…

宇宙学与河外天体物理 · 物理学 2010-11-16 Brian D. Fields , Vasiliki Pavlidou , Tijana Prodanovic

As a generalization of our previous work [Phys. Rev. D 95 043528 (2017)], in which an analytic model for the galaxy bispectrum in redshift space was developed on the basis of the halo approach, we here investigate its higher multipoles that…

宇宙学与河外天体物理 · 物理学 2018-07-31 Yue Nan , Kazuhiro Yamamoto , Chiaki Hikage

The Universe could be spatially flat, positively curved or negatively curved. Each option has been popular at various times, partly affected by an understanding that models tend to evolve away from flatness. The curvature of the Universe is…

天体物理学 · 物理学 2009-08-18 Elena Pierpaoli , Douglas Scott , Martin White

Although cosmological observations suggest that the fluctuations of seed fields are almost Gaussian, the possibility of a small deviation of their fields from Gaussianity is widely discussed. Theoretically, there exist numerous inflationary…

宇宙学与河外天体物理 · 物理学 2022-09-21 Maresuke Shiraishi

It has been recently recognized that the observational relativistic effects, mainly arising from the light propagation in an inhomogeneous universe, induce the dipole asymmetry in the cross-correlation function of galaxies. In particular,…

宇宙学与河外天体物理 · 物理学 2022-07-06 Shohei Saga , Atsushi Taruya , Michel-Andrès Breton , Yann Rasera

Recent theoretical work determines the correct coupling constant of a scalar field to the Ricci curvature of spacetime in general relativity. The periodicity in the redshift distribution of galaxies observed by Broadhurst {\em et al.}, if…

广义相对论与量子宇宙学 · 物理学 2010-11-30 Valerio Faraoni

Recent searches for parity breaking in the galaxy four-point correlation function, as well as the prospects for greatly improved sensitivity to parity breaking in forthcoming surveys, motivate the search for physical mechanisms that could…

宇宙学与河外天体物理 · 物理学 2025-02-07 Keisuke Inomata , Leah Jenks , Marc Kamionkowski

Next-generation galaxy surveys will increasingly rely on the galaxy bispectrum to improve cosmological constraints, especially on primordial non-Gaussianity. A key theoretical requirement that remains to be developed is the analysis of…

宇宙学与河外天体物理 · 物理学 2017-03-22 Obinna Umeh , Sheean Jolicoeur , Roy Maartens , Chris Clarkson

We analyze the science reach of a next generation galaxy redshift survey such as BigBOSS to fit simultaneously for time varying dark energy equation of state and time- and scale-dependent gravity. The simultaneous fit avoids potential bias…

宇宙学与河外天体物理 · 物理学 2013-02-06 Scott F. Daniel , Eric V. Linder

The recent measurement of the gravitational redshifts of galaxies in galaxy clusters by Wojtak et al. has opened a new observational window on dark matter and modified gravity. By stacking clusters this determination effectively used the…

宇宙学与河外天体物理 · 物理学 2015-06-15 Rupert A. C. Croft

The James Webb Space Telescope has recently detected massive, fully formed, galaxies at redshifts corresponding to few hundred million years after the Big-Bang. However, our current cosmological model cannot produce such massive systems so…

广义相对论与量子宇宙学 · 物理学 2025-11-26 Christos G. Tsagas

Clusters of galaxies have been used to measure a subtle effect predicted by Einstein: gravitational redshift. This signal encodes pristine information about our Universe, since it is sensitive to the depth of the clusters' gravitational…

宇宙学与河外天体物理 · 物理学 2026-01-28 Enea Di Dio , Sveva Castello , Camille Bonvin

A generic prediction of the standard cosmology, based on general relativity (GR), dark matter and the cosmological constant (and more generally, smooth dark energy), is that, the two gravitational potentials describing the spatial and…

天体物理学 · 物理学 2008-09-18 Pengjie Zhang , Rachel Bean , Michele Liguori , Scott Dodelson

Galaxy cluster peculiar velocities can be inferred from high-sensitivity, high-resolution multiple-frequency observations in the 30 to 400 GHz range. While galaxy cluster counts and power spectra are sensitive to the growth factor, peculiar…

天体物理学 · 物理学 2009-11-07 A. Peel , L. Knox