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When coupled to electromagnetism via a Chern-Simons interaction, axion-like particles (ALP) produce a rotation of the plane of linear polarization of photons known as cosmic birefringence. Recent measurements of cosmic birefringence…

宇宙学与河外天体物理 · 物理学 2023-04-10 P. Diego-Palazuelos

We investigate the point-parity and mirror-parity handedness of the large angle anisotropy in the cosmic microwave background (CMB). In particular we consider whether the observed low CMB quadrupole could more generally signal odd…

天体物理学 · 物理学 2015-06-24 Kate Land , Joao Magueijo

We propose using the upcoming Cosmic Microwave Background (CMB) ground based experiments to detect the signal of ALPs (Axion like particles) interacting with magnetic fields in galaxy clusters. The conversion between CMB photons and ALPs in…

宇宙学与河外天体物理 · 物理学 2020-03-02 Suvodip Mukherjee , David N. Spergel , Rishi Khatri , Benjamin D. Wandelt

Considering high-energy modifications of Einstein gravity during inflation is an interesting issue. We can constrain the strength of the new gravitational terms through observations of inflationary imprints in the actual universe. In this…

宇宙学与河外天体物理 · 物理学 2017-07-26 Nicola Bartolo , Giorgio Orlando

A detection of the primordial gravitational wave background is considered to be the ``smoking-gun '' evidence for inflation. While super-horizon waves are probed with cosmic microwave background (CMB) polarization, the relic background will…

天体物理学 · 物理学 2011-05-12 Tristan L. Smith , Hiranya V. Peiris , Asantha Cooray

We study the imprint of a coupling of scalar dark energy to photon on the cosmic microwave background (CMB) polarization. The time-evolving field value as well as the perturbation of the scalar generically induce $B$-mode polarization.…

宇宙学与河外天体物理 · 物理学 2014-03-26 Seokcheon Lee , Guo-Chin Liu , Kin-Wang Ng

In this paper we generalise previous work on tensor perturbations in a de Sitter background in terms of Ashtekar variables to cover all complex values of the Immirzi parameter gamma (previous work was restricted to imaginary gamma).…

广义相对论与量子宇宙学 · 物理学 2015-05-30 Laura Bethke , Joao Magueijo

Polarizations of electromagnetic waves from distant galaxies are known to be correlated with the source orientations. These quantities have been used to search for signals of cosmological birefringence. We review and classify transformation…

天体物理学 · 物理学 2009-10-30 John P. Ralston , Pankaj Jain

A B-mode polarization signal in the cosmic microwave background (CMB) is widely regarded as smoking gun evidence for gravitational waves produced during inflation. Here, we demonstrate that tensor perturbations sourced during…

宇宙学与河外天体物理 · 物理学 2026-04-22 Kylar Greene , Aurora Ireland , Gordan Krnjaic , Yuhsin Tsai

We show that in theories with a nontrivial kinetic term the contribution of the gravitational waves to the CMB fluctuations can be substantially larger than that is naively expected in simple inflationary models. This increase of the…

天体物理学 · 物理学 2014-10-13 V. Mukhanov , A. Vikman

We study the possible contribution of a stochastic gravitational wave background to the anisotropy of the cosmic microwave background (CMB) in cold and mixed dark matter (CDM and MDM) models. We test this contribution against recent…

天体物理学 · 物理学 2009-10-31 A. Melchiorri , M. V. Sazhin , V. V. Shulga , N. Vittorio

Inflation generates gravitational waves, which may be observable in the low multipoles of the cosmic microwave background (cmb) anisotropy but only if the inflaton field variation is at least of order the Planck scale. Such a large…

高能物理 - 唯象学 · 物理学 2009-10-28 David H. Lyth

The inflationary paradigm is extremely successful regarding predictions of temperature anisotropies in the CMB. However, inflation also makes predictions for a CMB B-mode polarization, which has not been detected. Moreover, the standard…

广义相对论与量子宇宙学 · 物理学 2018-07-24 Gabriel León , Abhishek Majhi , Elias Okon , Daniel Sudarsky

We compute analytically the tidal field and polarizations of an exact gravitational wave generated by a cylindrical beam of null matter of finite width and length in quadratic curvature gravity. We propose that this wave can represent the…

广义相对论与量子宇宙学 · 物理学 2009-11-10 E. C. de Rey Neto , J. C. N. de Araujo , O. D. Aguiar

When a cosmic microwave background (CMB) photon travels from the surface of last scatter through spacetime metric perturbations, the polarization vector may rotate about its direction of propagation. This gravitational rotation is distinct…

宇宙学与河外天体物理 · 物理学 2014-01-31 Liang Dai

While many aspects of general relativity have been tested, and general principles of quantum dynamics demand its quantization, there is no direct evidence for that. It has been argued that development of detectors sensitive to individual…

高能物理 - 理论 · 物理学 2014-03-04 Lawrence M. Krauss , Frank Wilczek

We study the auto-correlation function of CMB polarization anisotropies and their cross correlation with temperature fluctuations as probe of the causal structure of the universe. Because polarization is generated at the last scattering…

天体物理学 · 物理学 2016-08-30 David N. Spergel , Matias Zaldarriaga

The impact of the existence of gravitons with non-vanishing masses on the B modes of the Cosmic Microwave Background (CMB) is investigated. We also focus on putative modifications to the speed of the gravitational waves. We find that a…

宇宙学与河外天体物理 · 物理学 2018-03-21 Philippe Brax , Sebastian Cespedes , Anne-Christine Davis

Bipolar spherical harmonics (BiPoSHs) provide a general formalism for quantifying departures in the cosmic microwave background (CMB) from statistical isotropy (SI) and from Gaussianity. However, prior work has focused only on BiPoSHs with…

宇宙学与河外天体物理 · 物理学 2013-05-30 Laura G. Book , Marc Kamionkowski , Tarun Souradeep

Measurements of CMB anisotropy and, more recently, polarization have played a very important role in cosmology. Besides precise determination of various parameters of the `standard' cosmological model, observations have also established…

宇宙学与河外天体物理 · 物理学 2011-06-02 Tarun Souradeep