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Future observations of cosmic microwave background (CMB) polarisation have the potential to answer some of the most fundamental questions of modern physics and cosmology. In this paper, we list the requirements for a future CMB polarisation…

Instrumentation and Methods for Astrophysics · Physics 2019-08-13 J. Delabrouille , P. de Bernardis , F. R. Bouchet , A. Achúcarro , P. A. R. Ade , R. Allison , F. Arroja , E. Artal , M. Ashdown , C. Baccigalupi , M. Ballardini , A. J. Banday , R. Banerji , D. Barbosa , J. Bartlett , N. Bartolo , S. Basak , J. J. A. Baselmans , K. Basu , E. S. Battistelli , R. Battye , D. Baumann , A. Benoît , M. Bersanelli , A. Bideaud , M. Biesiada , M. Bilicki , A. Bonaldi , M. Bonato , J. Borrill , F. Boulanger , T. Brinckmann , M. L. Brown , M. Bucher , C. Burigana , A. Buzzelli , G. Cabass , Z. -Y. Cai , M. Calvo , A. Caputo , C. -S. Carvalho , F. J. Casas , G. Castellano , A. Catalano , A. Challinor , I. Charles , J. Chluba , D. L. Clements , S. Clesse , S. Colafrancesco , I. Colantoni , D. Contreras , A. Coppolecchia , M. Crook , G. D'Alessandro , G. D'Amico , A. da Silva , M. de Avillez , G. de Gasperis , M. De Petris , G. de Zotti , L. Danese , F. -X. Désert , V. Desjacques , E. Di Valentino , C. Dickinson , J. M. Diego , S. Doyle , R. Durrer , C. Dvorkin , H. -K. Eriksen , J. Errard , S. Feeney , R. Fernández-Cobos , F. Finelli , F. Forastieri , C. Franceschet , U. Fuskeland , S. Galli , R. T. Génova-Santos , M. Gerbino , E. Giusarma , A. Gomez , J. González-Nuevo , S. Grandis , J. Greenslade , J. Goupy , S. Hagstotz , S. Hanany , W. Handley , S. Henrot-Versillé , C. Hernández-Monteagudo , C. Hervias-Caimapo , M. Hills , M. Hindmarsh , E. Hivon , D. T. Hoang , D. C. Hooper , B. Hu , E. Keihänen , R. Keskitalo , K. Kiiveri , T. Kisner , T. Kitching , M. Kunz , H. Kurki-Suonio , G. Lagache , L. Lamagna , A. Lapi , A. Lasenby , M. Lattanzi , A. M. C. Le Brun , J. Lesgourgues , M. Liguori , V. Lindholm , J. Lizarraga , G. Luzzi , J. F. Macìas-Pérez , B. Maffei , N. Mandolesi , S. Martin , E. Martinez-Gonzalez , C. J. A. P. Martins , S. Masi , M. Massardi , S. Matarrese , P. Mazzotta , D. McCarthy , A. Melchiorri , J. -B. Melin , A. Mennella , J. Mohr , D. Molinari , A. Monfardini , L. Montier , P. Natoli , M. Negrello , A. Notari , F. Noviello , F. Oppizzi , C. O'Sullivan , L. Pagano , A. Paiella , E. Pajer , D. Paoletti , S. Paradiso , R. B. Partridge , G. Patanchon , S. P. Patil , O. Perdereau , F. Piacentini , M. Piat , G. Pisano , L. Polastri , G. Polenta , A. Pollo , N. Ponthieu , V. Poulin , D. Prêle , M. Quartin , A. Ravenni , M. Remazeilles , A. Renzi , C. Ringeval , D. Roest , M. Roman , B. F. Roukema , J. -A. Rubino-Martin , L. Salvati , D. Scott , S. Serjeant , G. Signorelli , A. A. Starobinsky , R. Sunyaev , C. Y. Tan , A. Tartari , G. Tasinato , L. Toffolatti , M. Tomasi , J. Torrado , D. Tramonte , N. Trappe , S. Triqueneaux , M. Tristram , T. Trombetti , M. Tucci , C. Tucker , J. Urrestilla , J. Väliviita , R. Van de Weygaert , B. Van Tent , V. Vennin , L. Verde , G. Vermeulen , P. Vielva , N. Vittorio , F. Voisin , C. Wallis , B. Wandelt , I. Wehus , J. Weller , K. Young , M. Zannoni

South Pole Station offers a unique combination of high, dry, stable conditions and well-developed support facilities. Over the past 20 years, a sequence of increasingly sophisticated CMB experiments at Pole have built on the experience of…

Astrophysics · Physics 2007-07-10 J. M. Kovac , D. Barkats

We present a pedagogical and phenomenological introduction to the study of cosmic microwave background (CMB) polarization to build intuition about the prospects and challenges facing its detection. Thomson scattering of temperature…

Astrophysics · Physics 2009-08-18 Wayne Hu , Martin White

CMB-S4, the next-generation ground-based cosmic microwave background (CMB) observatory, will provide detailed maps of the CMB at millimeter wavelengths to dramatically advance our understanding of the origin and evolution of the universe.…

This Science White Paper, prepared in response to the ESA Voyage 2050 call for long-term mission planning, aims to describe the various science possibilities that can be realized with an L-class space observatory that is dedicated to the…

The polarization of the Cosmic Microwave Background (CMB)is a powerful observational tool at hand for modern cosmology. It allows to break the degeneracy of fundamental cosmological parameters one cannot obtain using only anisotropy data…

Astrophysics · Physics 2009-11-07 M. V. Sazhin , G. Sironi , O. S. Khovanskaya

We review the theory of the temperature anisotropy and polarization of the cosmic microwave background (CMB) radiation, and describe what we have learned from current CMB observations. In particular, we discuss how the CMB is being used to…

Cosmology and Nongalactic Astrophysics · Physics 2010-02-22 Anthony Challinor , Hiranya Peiris

The Cosmic Microwave Background (CMB) is a fundamental observational tool in modern cosmology. The linear polarization of the CMB provides a crucial observational tool for exploring new physics, including the inflationary paradigm and…

Cosmology and Nongalactic Astrophysics · Physics 2025-03-12 Vyoma Muralidhara

For 40 years, the cosmic microwave background (CMB) has been the most important source of information about the geometry and contents of the Universe. Even so, only a small fraction of the information available in the CMB has been extracted…

Astrophysics · Physics 2012-08-27 The Planck Collaboration

Rapid progress has been made in observations of the temperature anisotropies of the Cosmic Microwave Background (CMB). These observations have enabled cosmologists to characterize the state of the universe at recombination, and…

Astrophysics · Physics 2009-11-07 Tanmay Vachaspati , Arthur Lue

Observations of the polarization of the cosmic microwave backround (CMB) have the potential to place much tighter constraints on cosmological parameters than observations of the fluctuations in temperature alone. We discuss using CMB…

Astrophysics · Physics 2009-10-30 William H. Kinney

I briefly review some of the most common map-making strategies for experiments targeting the polarization of the Cosmic Microwave Background (CMB), in light of the anticipated volumes of data collected by next generation observatories such…

Cosmology and Nongalactic Astrophysics · Physics 2024-06-25 Simon Biquard

One of the most spectacular scientific breakthroughs in past decades was using measurements of the fluctuations in the cosmic microwave background (CMB) to test precisely our understanding of the history and composition of the Universe.…

The next generation of instruments designed to measure the polarization of the cosmic microwave background (CMB) will provide a historic opportunity to open the gravitational wave window to the primordial Universe. Through high sensitivity…

The Universe is the grandest conceivable scale on which the human mind can strive to understand nature. The amazing aspect of cosmology, the branch of science that attempts to understand the origin and evolution of the Universe, is that it…

Cosmology and Nongalactic Astrophysics · Physics 2011-04-19 Tarun Souradeep

The cosmic microwave background (CMB) experiments have reached an era of unprecedented precision and complexity. Aiming to detect the primordial B-mode polarization signal, these experiments will soon be equipped with $10^{4}$ to $10^{5}$…

Cosmology and Nongalactic Astrophysics · Physics 2025-11-05 Avinash Anand , Giuseppe Puglisi

This is a solicited whitepaper for the Snowmass 2021 community planning exercise. The paper focuses on measurements and science with the Cosmic Microwave Background (CMB). The CMB is foundational to our understanding of modern physics and…

Cosmology and Nongalactic Astrophysics · Physics 2022-03-16 Clarence L. Chang , Kevin M. Huffenberger , Bradford A. Benson , Federico Bianchini , Jens Chluba , Jacques Delabrouille , Raphael Flauger , Shaul Hanany , William C. Jones , Alan J. Kogut , Jeffrey J. McMahon , Joel Meyers , Neelima Sehgal , Sara M. Simon , Caterina Umilta , Kevork N. Abazajian , Zeeshan Ahmed , Yashar Akrami , Adam J. Anderson , Behzad Ansarinejad , Jason Austermann , Carlo Baccigalupi , Denis Barkats , Darcy Barron , Peter S. Barry , Nicholas Battaglia , Eric Baxter , Dominic Beck , Amy N. Bender , Charles Bennett , Benjamin Beringue , Colin Bischoff , Lindsey Bleem , James Bock , Boris Bolliet , J Richard Bond , Julian Borrill , Thejs Brinckmann , Michael L. Brown , Erminia Calabrese , John Carlstrom , Anthony Challinor , Chihway Chang , Yuji Chinone , Susan E. Clark , William Coulton , Ari Cukierman , Francis-Yan Cyr-Racine , Shannon M. Duff , Cora Dvorkin , Alexander van Engelen , Josquin Errard , Johannes R. Eskilt , Thomas Essinger-Hileman , Giulio Fabbian , Chang Feng , Simone Ferraro , Jeffrey Filippini , Katherine Freese , Nicholas Galitzki , Eric Gawiser , Daniel Grin , Daniel Grin , Evan Grohs , Alessandro Gruppuso , Jon E. Gudmundsson , Nils W. Halverson , Jean-Christophe Hamilton , Kathleen Harrington , Sophie Henrot-Versillé , Brandon Hensley , J. Colin Hill , Adam D. Hincks , Renee Hlozek , William Holzapfel , Selim C. Hotinli , Howard Hui , Ayodeji Ibitoye , Matthew Johnson , Bradley R. Johnson , Jae Hwan Kang , Kirit S. Karkare , Lloyd Knox , John Kovac , Kenny Lau , Louis Legrand , Marilena Loverde , Philip Lubin , Yin-Zhe Ma , Tony Mroczkowski , Suvodip Mukherjee , Moritz Münchmeyer , Daisuke Nagai , Johanna Nagy , Michael Niemack , Valentine Novosad , Yuuki Omori , Giorgio Orlando , Zhaodi Pan , Laurence Perotto , Matthew A. Petroff , Levon Pogosian , Clem Pryke , Alexandra Rahlin , Marco Raveri , Christian L. Reichardt , Mathieu Remazeilles , Yoel Rephaeli , John Ruhl , Emmanuel Schaan , Sarah Shandera , Meir Shimon , Ahmed Soliman , Antony A. Stark , Glenn D. Starkman , Radek Stompor , Ritoban Basu Thakur , Cynthia Trendafilova , Matthieu Tristram , Pranjal Trivedi , Gregory Tucker , Eleonora Di Valentino , Joaquin Vieira , Abigail Vieregg , Gensheng Wang , Scott Watson , Lukas Wenzl , Edward J. Wollack , W. L. Kimmy Wu , Zhilei Xu , David Zegeye , Cheng Zhang

With polarization of the cosmic microwave background (CMB) now detected, and confirmed by several independent experiments, the next goal is to characterise accurately its statistical properties. In these lecture notes we review the physical…

Astrophysics · Physics 2018-05-02 Anthony Challinor

The cosmic microwave background (CMB) contains perturbations that are close to Gaussian and isotropic. This means that its information content, in the sense of the ability to constrain cosmological models, is closely related to the number…

Cosmology and Nongalactic Astrophysics · Physics 2016-07-06 Douglas Scott , Dagoberto Contreras , Ali Narimani , Yin-Zhe Ma