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Related papers: Detecting rotation from lensing in the CMB

200 papers

We present a first internal delensing of CMB maps, both in temperature and polarization, using the public foreground-cleaned (SMICA) Planck 2015 maps. After forming quadratic estimates of the lensing potential, we use the corresponding…

Cosmology and Nongalactic Astrophysics · Physics 2017-05-24 Julien Carron , Antony Lewis , Anthony Challinor

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…

Cosmology and Nongalactic Astrophysics · Physics 2014-01-31 Liang Dai

Impacts of observational systematic errors on the lensing analysis of the cosmic microwave background (CMB) polarization are investigated by numerical simulations. We model errors of gain, angle, and pointing in observation of the CMB…

Cosmology and Nongalactic Astrophysics · Physics 2021-06-10 Ryo Nagata , Toshiya Namikawa

Lensing of the CMB is affected by post-Born lensing, producing corrections to the convergence power spectrum and introducing field rotation. We show numerically that the lensing convergence power spectrum is affected at the $\lesssim 0.2\%$…

Cosmology and Nongalactic Astrophysics · Physics 2024-06-03 Geraint Pratten , Antony Lewis

The next-generation CMB experiments are expected to constrain the tensor-to-scalar ratio $r$ with high precision. Delensing is an important process as the observed CMB $B$-mode polarization that contains the primordial tensor perturbation…

Cosmology and Nongalactic Astrophysics · Physics 2022-10-17 Chen Heinrich , Trey Driskell , Chris Heinrich

The primordial B-modes component of the cosmic microwave background (CMB) polarization is a promising experimental dataset to probe the inflationary paradigm. B-modes are indeed a direct consequence of the presence of gravitational waves in…

Cosmology and Nongalactic Astrophysics · Physics 2018-02-28 Alessandro Manzotti

We investigate the performance of a simple Bayesian fitting approach to correct the cosmic microwave background (CMB) B-mode polarization for gravitational lensing effects in the recovered probability distribution of the tensor-to-scalar…

Cosmology and Nongalactic Astrophysics · Physics 2017-11-28 M. Remazeilles , C. Dickinson , H. K. Eriksen , I. K. Wehus

Polarization data will soon provide the best avenue for measurements of the CMB lensing potential, although it is potentially sensitive to several instrumental effects including beam asymmetry, polarization angle uncertainties, sky…

Cosmology and Nongalactic Astrophysics · Physics 2019-06-10 Toshiya Namikawa , Ryuichi Takahashi

As confusion with lensing B-modes begins to limit experiments that search for primordial B-mode polarization, robust methods for delensing the CMB polarization sky are becoming increasingly important. We investigate in detail the…

Cosmology and Nongalactic Astrophysics · Physics 2015-08-19 Blake D. Sherwin , Marcel Schmittfull

Cosmological Birefringence (CB), a rotation of the polarization plane of radiation coming to us from distant astrophysical sources, may reveal parity violation in either the electromagnetic or gravitational sectors of the fundamental…

Cosmology and Nongalactic Astrophysics · Physics 2013-05-30 Amit P. S. Yadav , Meir Shimon , Brian G. Keating

CMB (Cosmic Microwave Background) polarization observations test many aspects of cosmological models. Effective pseudoscalar-photon interaction(s) would induce a rotation of linear polarization of electromagnetic wave propagating with…

Cosmology and Nongalactic Astrophysics · Physics 2009-08-20 Wei-Tou Ni

Large-scale $B$-mode polarization of the cosmic microwave background (CMB) is a prime target for current and future experiments in search of primordial gravitational waves (PGW). With increasingly sensitive instruments being deployed,…

We present efficient algorithms for CMB lensing simulation and power spectrum es- timation for flat-sky CMB polarization maps. We build a pure B-mode estimator to remedy E to B leakage due to partial sky coverage. We show that our…

Cosmology and Nongalactic Astrophysics · Physics 2013-11-14 Thibaut Louis , Sigurd Næss , Sudeep Das , Joanna Dunkley , Blake Sherwin

The cosmic microwave background (CMB) lensing power spectrum is a powerful probe of the late-time universe, encoding valuable information about cosmological parameters such as the sum of neutrino masses and dark energy equation of state.…

Cosmology and Nongalactic Astrophysics · Physics 2024-10-11 Hongbo Cai , Yilun Guan , Toshiya Namikawa , Arthur Kosowsky

The effect of weak gravitational lensing on the cosmic microwave background (CMB) temperature anisotropies and polarization will provide access to cosmological information that cannot be obtained from the primary anisotropies alone. We…

Astrophysics · Physics 2007-05-23 Sarah Smith , Anthony Challinor , Graca Rocha

The B-mode of polarization of the CMB is a uniquely powerful probe of gravitational waves produced in the very early Universe. But searches for primordial B-mode anisotropies must contend with gravitational lensing, which induces late-time…

Cosmology and Nongalactic Astrophysics · Physics 2026-02-27 Shengzhu Wang , Antón Baleato Lizancos , José Luis Bernal

Gravitational lensing rotation of images is predicted to be negligible at linear order in density perturbations, but can be produced by the post-Born lens-lens coupling at second order. This rotation is somewhat enhanced for Cosmic…

Cosmology and Nongalactic Astrophysics · Physics 2025-01-28 Mathew Robertson , Antony Lewis

We report the first detection of gravitational lensing due to galaxy clusters using only the polarization of the cosmic microwave background (CMB). The lensing signal is obtained using a new estimator that extracts the lensing dipole…

Cosmology and Nongalactic Astrophysics · Physics 2019-11-06 S. Raghunathan , S. Patil , E. Baxter , B. A. Benson , L. E. Bleem , T. M. Crawford , G. P. Holder , T. McClintock , C. L. Reichardt , T. N. Varga , N. Whitehorn , P. A. R. Ade , S. Allam , A. J. Anderson , J. E. Austermann , S. Avila , J. S. Avva , D. Bacon , J. A. Beall , A. N. Bender , F. Bianchini , S. Bocquet , D. Brooks , D. L. Burke , J. E. Carlstrom , J. Carretero , F. J. Castander , C. L. Chang , H. C. Chiang , R. Citron , M. Costanzi , A. T. Crites , L. N. da Costa , S. Desai , H. T. Diehl , J. P. Dietrich , M. A. Dobbs , P. Doel , S. Everett , A. E. Evrard , C. Feng , B. Flaugher , P. Fosalba , J. Frieman , J. Gallicchio , J. García-Bellido , E. Gaztanaga , E. M. George , T. Giannantonio , A. Gilbert , R. A. Gruendl , J. Gschwend , N. Gupta , G. Gutierrez , T. de Haan , N. W. Halverson , N. Harrington , J. W. Henning , G. C. Hilton , D. L. Hollowood , W. L. Holzapfel , K. Honscheid , J. D. Hrubes , N. Huang , J. Hubmayr , K. D. Irwin , T. Jeltema , M. Carrasco Kind , L. Knox , N. Kuropatkin , O. Lahav , A. T. Lee , D. Li , M. Lima , A. Lowitz , M. A. G. Maia , J. L. Marshall , J. J. McMahon , P. Melchior , F. Menanteau , S. S. Meyer , R. Miquel , L. M. Mocanu , J. J. Mohr , J. Montgomery , C. Corbett Moran , A. Nadolski , T. Natoli , J. P. Nibarger , G. Noble , V. Novosad , R. L. C. Ogando , S. Padin , A. A. Plazas , C. Pryke , D. Rapetti , A. K. Romer , A. Roodman , A. Carnero Rosell , E. Rozo , J. E. Ruhl , E. S. Rykoff , B. R. Saliwanchik , E. Sanchez , J. T. Sayre , V. Scarpine , K. K. Schaffer , M. Schubnell , S. Serrano , I. Sevilla-Noarbe , C. Sievers , G. Smecher , M. Smith , M. Soares-Santos , A. A. Stark , K. T. Story , E. Suchyta , M. E. C. Swanson , G. Tarle , C. Tucker , K. Vanderlinde , T. Veach , J. De Vicente , J. D. Vieira , V. Vikram , G. Wang , W. L. K. Wu , V. Yefremenko , Y. Zhang

Detailed measurements of the CMB lensing signal are an important scientific goal of ongoing ground-based CMB polarization experiments, which are mapping the CMB at high resolution over small patches of the sky. In this work we simulate CMB…

Cosmology and Nongalactic Astrophysics · Physics 2014-07-30 Ruth Pearson , Blake Sherwin , Antony Lewis