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Recognizing the impact of contamination from weak gravitational lensing B-modes induced by Large Scale Structure, we examine delensing methods to enhance sensitivity to the tensor-to-scalar ratio $r$ in primordial B-mode detection…

Cosmology and Nongalactic Astrophysics · Physics 2025-11-27 Wen-Zheng Chen , Yang Liu , Siyu Li , Bin Hu , Hong Li

The search for primordial gravitational waves in the Cosmic Microwave Background (CMB) will soon be limited by our ability to remove the lensing contamination to $B$-mode polarization. The often-used quadratic estimator for lensing is known…

Cosmology and Nongalactic Astrophysics · Physics 2021-01-04 Marius Millea , Ethan Anderes , Benjamin D. Wandelt

A detection of excess cosmic microwave background (CMB) B-mode polarization on large scales allows the possibility of measuring not only the amplitude of these fluctuations but also their scale dependence, which can be parametrized as the…

Cosmology and Nongalactic Astrophysics · Physics 2015-08-06 Gabrielle Simard , Duncan Hanson , Gil Holder

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 explore the potential use of the Radio Continuum (RC) survey conducted by the Square Kilometre Array (SKA) to remove (delens) the lensing-induced B-mode polarization and thus enhance future cosmic microwave background (CMB) searches for…

Cosmology and Nongalactic Astrophysics · Physics 2016-03-02 Toshiya Namikawa , Daisuke Yamauchi , Blake Sherwin , Ryo Nagata

We present a constraint on the tensor-to-scalar ratio, $r$, derived from measurements of cosmic microwave background (CMB) polarization $B$-modes with "delensing," whereby the uncertainty on $r$ contributed by the sample variance of the…

Cosmology and Nongalactic Astrophysics · Physics 2021-02-02 BICEP/Keck , SPTpol Collaborations , : , P. A. R. Ade , Z. Ahmed , M. Amiri , A. J. Anderson , J. E. Austermann , J. S. Avva , D. Barkats , R. Basu Thakur , J. A. Beall , A. N. Bender , B. A. Benson , F. Bianchini , C. A. Bischoff , L. E. Bleem , J. J. Bock , H. Boenish , E. Bullock , V. Buza , J. E. Carlstrom , C. L. Chang , J. R. Cheshire , H. C. Chiang , T-L. Chou , R. Citron , J. Connors , C. Corbett Moran , J. Cornelison , T. M. Crawford , A. T. Crites , M. Crumrine , A. Cukierman , T. de Haan , M. Dierickx , M. A. Dobbs , L. Duband , W. Everett , S. Fatigoni , J. P. Filippini , S. Fliescher , J. Gallicchio , E. M. George , T. St. Germaine , N. Goeckner-Wald , D. C. Goldfinger , J. Grayson , N. Gupta , G. Hall , M. Halpern , N. W. Halverson , S. Harrison , S. Henderson , J. W. Henning , S. R. Hildebrandt , G. C. Hilton , G. P. Holder , W. L. Holzapfel , J. D. Hrubes , N. Huang , J. Hubmayr , H. Hui , K. D. Irwin , J. Kang , K. S. Karkare , E. Karpel , S. Kefeli , S. A. Kernasovskiy , L. Knox , J. M. Kovac , C. L. Kuo , K. Lau , A. T. Lee , E. M. Leitch , D. Li , A. Lowitz , A. Manzotti , J. J. McMahon , K. G. Megerian , S. S. Meyer , M. Millea , L. M. Mocanu , L. Moncelsi , J. Montgomery , A. Nadolski , T. Namikawa , T. Natoli , C. B. Netterfield , H. T. Nguyen , J. P. Nibarger , G. Noble , V. Novosad , R. O'Brient , R. W. Ogburn , Y. Omori , S. Padin , S. Palladino , S. Patil , T. Prouve , C. Pryke , B. Racine , C. L. Reichardt , C. D. Reintsema , S. Richter , J. E. Ruhl , B. R. Saliwanchik , K. K. Schaffer , A. Schillaci , B. L. Schmitt , R. Schwarz , C. D. Sheehy , C. Sievers , G. Smecher , A. Soliman , A. A. Stark , B. Steinbach , R. V. Sudiwala , G. P. Teply , K. L. Thompson , J. E. Tolan , C. Tucker , A. D. Turner , C. Umiltà , T. Veach , J. D. Vieira , A. G. Vieregg , A. Wandui , G. Wang , A. C. Weber , N. Whitehorn , D. V. Wiebe , J. Willmert , C. L. Wong , W. L. K. Wu , H. Yang , V. Yefremenko , K. W. Yoon , E. Young , C. Yu , L. Zeng , C. Zhang

The delensing of cosmic microwave background (CMB) maps will be increasingly valuable for extracting as much information as possible from future CMB surveys. Delensing provides many general benefits, including sharpening of the acoustic…

Cosmology and Nongalactic Astrophysics · Physics 2024-09-20 Cynthia Trendafilova , Selim C. Hotinli , Joel Meyers

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

We present a new method for delensing $B$ modes of the cosmic microwave background (CMB) using a lensing potential reconstructed from the same realization of the CMB polarization (CMB internal delensing). The $B$-mode delensing is required…

Cosmology and Nongalactic Astrophysics · Physics 2017-05-31 Toshiya Namikawa

We estimate the efficiency of mitigating the lensing $B$-mode polarization, the so-called delensing, for the $LiteBIRD$ experiment with multiple external data sets of lensing-mass tracers. The current best bound on the tensor-to-scalar…

Cosmology and Nongalactic Astrophysics · Physics 2024-12-30 T. Namikawa , A. I. Lonappan , C. Baccigalupi , N. Bartolo , D. Beck , K. Benabed , A. Challinor , P. Diego-Palazuelos , J. Errard , S. Farrens , A. Gruppuso , N. Krachmalnicoff , M. Migliaccio , E. Martínez-González , V. Pettorino , G. Piccirilli , M. Ruiz-Granda , B. Sherwin , J. Starck , P. Vielva , R. Akizawa , A. Anand , J. Aumont , R. Aurlien , S. Azzoni , M. Ballardini , A. J. Banday , R. B. Barreiro , M. Bersanelli , D. Blinov , M. Bortolami , T. Brinckmann , E. Calabrese , P. Campeti , A. Carones , F. Carralot , F. J. Casas , K. Cheung , L. Clermont , F. Columbro , G. Conenna , A. Coppolecchia , F. Cuttaia , G. D'Alessandro , P. de Bernardis , T. de Haan , M. De Petris , S. Della Torre , E. Di Giorgi , H. K. Eriksen , F. Finelli , C. Franceschet , U. Fuskeland , G. Galloni , M. Galloway , M. Georges , M. Gerbino , M. Gervasi , T. Ghigna , S. Giardiello , C. Gimeno-Amo , E. Gjerløw , M. Hazumi , S. Henrot-Versillé , L. T. Hergt , E. Hivon , K. Kohri , E. Komatsu , L. Lamagna , M. Lattanzi , C. Leloup , M. Lembo , M. López-Caniego , G. Luzzi , B. Maffei , S. Masi , M. Massa , S. Matarrese , T. Matsumura , S. Micheli , A. Moggi , M. Monelli , L. Montier , G. Morgante , B. Mot , L. Mousset , R. Nagata , P. Natoli , A. Novelli , I. Obata , A. Occhiuzzi , L. Pagano , A. Paiella , D. Paoletti , G. Pascual-Cisneros , V. Pavlidou , F. Piacentini , M. Pinchera , G. Pisano , G. Polenta , G. Puglisi , M. Remazeilles , A. Ritacco , A. Rizzieri , J. Rubino-Martin , Y. Sakurai , D. Scott , M. Shiraishi , G. Signorelli , S. L. Stever , Y. Takase , H. Tanimura , A. Tartari , K. Tassis , L. Terenzi , M. Tristram , L. Vacher , B. van Tent , I. K. Wehus , G. Weymann-Despres , M. Zannoni , Y. Zhou

The Simons Observatory (SO), due to start full science operations in early 2025, aims to set tight constraints on inflationary physics by inferring the tensor-to-scalar ratio $r$ from measurements of CMB polarization $B$-modes. Its nominal…

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

The Simons Observatory (SO), a next-generation ground-based CMB experiment in its final stages of construction, will target primordial $B$-modes with unprecedented sensitivity to set tight bounds on the amplitude of inflationary…

Cosmology and Nongalactic Astrophysics · Physics 2024-05-24 Emilie Hertig , Kevin Wolz , Toshiya Namikawa , Antón Baleato Lizancos , Susanna Azzoni , Anthony Challinor

Primordial B-mode detection is one of the main goals of next-generation cosmic microwave background (CMB) experiments. Primordial B-modes are a unique signature of primordial gravitational waves (PGWs). However, the gravitational…

Cosmology and Nongalactic Astrophysics · Physics 2023-07-05 Ye-Peng Yan , Guo-Jian Wang , Si-Yu Li , Jun-Qing Xia

The search for primordial $B$-mode polarization of the CMB is limited by the sample variance of $B$-modes produced at later times by gravitational lensing. Constraints can be improved by `delensing': using some proxy of the matter…

Cosmology and Nongalactic Astrophysics · Physics 2023-01-24 Antón Baleato Lizancos , Simone Ferraro

One of the primary scientific targets of current and future CMB polarization experiments is the search for a stochastic background of gravity waves in the early universe. As instrumental sensitivity improves, the limiting factor will…

Cosmology and Nongalactic Astrophysics · Physics 2015-05-20 Kendrick M. Smith , Duncan Hanson , Marilena LoVerde , Christopher M. Hirata , Oliver Zahn

Efforts to detect a primordial $B$-mode of CMB polarization generated by inflationary gravitational waves ought to mitigate the large variance associated with the $B$-modes produced by gravitational lensing, a process known as delensing. A…

Cosmology and Nongalactic Astrophysics · Physics 2021-01-13 Antón Baleato Lizancos , Anthony Challinor , Julien Carron

The most promising avenue for detecting primordial gravitational waves from cosmic inflation is through measurements of degree-scale CMB $B$-mode polarisation. This approach must face the challenge posed by gravitational lensing of the CMB,…

Cosmology and Nongalactic Astrophysics · Physics 2022-07-20 Antón Baleato Lizancos , Anthony Challinor , Blake D. Sherwin , Toshiya Namikawa

We analyze the possibility of delensing CMB polarization maps using foreground weak lensing (WL) information. We build an estimator of the CMB lensing potential out of optimally combined projected potential estimators to different source…

Astrophysics · Physics 2008-11-26 Laura Marian , Gary M. Bernstein
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