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相关论文: PICO: Probe of Inflation and Cosmic Origins

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The Probe of Inflation and Cosmic Origins (PICO) is an imaging polarimeter that will scan the sky for 5 years in 21 frequency bands spread between 21 and 799 GHz. It will produce full-sky surveys of intensity and polarization with a final…

The Probe of Inflation and Cosmic Origins (PICO) is a NASA-funded study of a Probe-class mission concept. The top-level science objectives are to probe the physics of the Big Bang by measuring or constraining the energy scale of inflation,…

The Probe of Inflation and Cosmic Origins (PICO) is a probe-class mission concept currently under study by NASA. PICO will probe the physics of the Big Bang and the energy scale of inflation, constrain the sum of neutrino masses, measure…

This is the Phase 1 Report on the Experimental Probe of Inflationary Cosmology (EPIC), a mission concept study for NASA's Einstein Inflation Probe. When we began our study we sought to answer five fundamental implementation questions: 1)…

The Primordial Inflation Explorer (PIXIE) is an Explorer-class mission concept to measure the energy spectrum and linear polarization of the cosmic microwave background (CMB). A single cryogenic Fourier transform spectrometer compares the…

The Primordial Inflation Polarization ExploreR (PIPER) is a balloon-borne telescope designed to measure the polarization of the Cosmic Microwave Background on large angular scales. PIPER will map 85% of the sky at 200, 270, 350, and 600 GHz…

The Primordial Inflation Explorer (PIXIE) is an Explorer-class mission to measure the gravity-wave signature of primordial inflation through its distinctive imprint on the linear polarization of the cosmic microwave background. The…

宇宙学与河外天体物理 · 物理学 2015-05-28 A. Kogut , D. J. Fixsen , D. T. Chuss , J. Dotson , E. Dwek , M. Halpern , G. F. Hinshaw , S. M. Meyer , S. H. Moseley , M. D. Seiffert , D. N. Spergel , E. J. Wollack

Measurements of Cosmic Microwave Background (CMB) anisotropy have served as the best experimental probe of the early universe to date. The inflationary paradigm, inspired in part by the extreme isotropy of the CMB, is now a cornerstone in…

Cosmic microwave background experiments have experienced an exponential increase in complexity, data size and sensitivity. One of the goals of current and future experiments is to characterize the B-mode power spectrum, which would be…

天体物理仪器与方法 · 物理学 2020-07-07 P. Fluxá , M. K. Brewer , R. Dünner

We forecast the scientific capabilities to improve our understanding of cosmic inflation of CORE, a proposed CMB space satellite submitted in response to the ESA fifth call for a medium-size mission opportunity. The CORE satellite will map…

宇宙学与河外天体物理 · 物理学 2018-04-25 CORE Collaboration , Fabio Finelli , Martin Bucher , Ana Achúcarro , Mario Ballardini , Nicola Bartolo , Daniel Baumann , Sébastien Clesse , Josquin Errard , Will Handley , Mark Hindmarsh , Kimmo Kiiveri , Martin Kunz , Anthony Lasenby , Michele Liguori , Daniela Paoletti , Christophe Ringeval , Jussi Väliviita , Bartjan van Tent , Vincent Vennin , Rupert Allison , Frederico Arroja , Marc Ashdown , A. J. Banday , Ranajoy Banerji , James G. Bartlett , Soumen Basak , Jochem Baselmans , Paolo de Bernardis , Marco Bersanelli , Anna Bonaldi , Julian Borril , François R. Bouchet , François Boulanger , Thejs Brinckmann , Carlo Burigana , Alessandro Buzzelli , Zhen-Yi Cai , Martino Calvo , Carla Sofia Carvalho , Gabriella Castellano , Anthony Challinor , Jens Chluba , Ivan Colantoni , Martin Crook , Giuseppe D'Alessandro , Guido D'Amico , Jacques Delabrouille , Vincent Desjacques , Gianfranco De Zotti , Jose Maria Diego , Eleonora Di Valentino , Stephen Feeney , James R. Fergusson , Raul Fernandez-Cobos , Simone Ferraro , Francesco Forastieri , Silvia Galli , Juan García-Bellido , Giancarlo de Gasperis , Ricardo T. Génova-Santos , Martina Gerbino , Joaquin González-Nuevo , Sebastian Grandis , Josh Greenslade , Steffen Hagstotz , Shaul Hanany , Dhiraj K. Hazra , Carlos Hernández-Monteagudo , Carlos Hervias-Caimapo , Matthew Hills , Eric Hivon , Bin Hu , Ted Kisner , Thomas Kitching , Ely D. Kovetz , Hannu Kurki-Suonio , Luca Lamagna , Massimiliano Lattanzi , Julien Lesgourgues , Antony Lewis , Valtteri Lindholm , Joanes Lizarraga , Marcos López-Caniego , Gemma Luzzi , Bruno Maffei , Nazzareno Mandolesi , Enrique Martínez-González , Carlos J. A. P. Martins , Silvia Masi , Darragh McCarthy , Sabino Matarrese , Alessandro Melchiorri , Jean-Baptiste Melin , Diego Molinari , Alessandro Monfardini , Paolo Natoli , Mattia Negrello , Alessio Notari , Filippo Oppizzi , Alessandro Paiella , Enrico Pajer , Guillaume Patanchon , Subodh P. Patil , Michael Piat , Giampaolo Pisano , Linda Polastri , Gianluca Polenta , Agnieszka Pollo , Vivian Poulin , Miguel Quartin , Andrea Ravenni , Mathieu Remazeilles , Alessandro Renzi , Diederik Roest , Matthieu Roman , Jose Alberto Rubiño-Martin , Laura Salvati , Alexei A. Starobinsky , Andrea Tartari , Gianmassimo Tasinato , Maurizio Tomasi , Jesús Torrado , Neil Trappe , Tiziana Trombetti , Carole Tucker , Marco Tucci , Jon Urrestilla , Rien van de Weygaert , Patricio Vielva , Nicola Vittorio , Karl Young

PICO is a concept for a NASA probe-scale mission aiming to detect or constrain the tensor to scalar ratio $r$, a parameter that quantifies the amplitude of inflationary gravity waves. We carry out map-based component separation on…

The Primordial Inflation Polarization Explorer (PIPER) is a balloon-borne cosmic microwave background (CMB) polarimeter designed to search for evidence of inflation by measuring the large-angular scale CMB polarization signal. BICEP2…

The Primordial Inflation Explorer (PIXIE) is an Explorer-class mission concept designed to measure the polarization and absolute intensity of the cosmic microwave background. In the following, we report on the design, fabrication, and…

The Primordial Inflation Explorer (PIXIE) is an Explorer-class mission concept to measure cosmological signals from both linear polarization of the cosmic microwave background and spectral distortions from a perfect blackbody. The targeted…

天体物理仪器与方法 · 物理学 2021-03-08 A. Kogut , D. J. Fixsen

We propose an inflationary primordial feature model that can explain both the large and small-scale anomalies in the currently measured cosmic microwave background (CMB) anisotropy spectra, revealing a clip of adventurous history of the…

宇宙学与河外天体物理 · 物理学 2022-06-15 Matteo Braglia , Xingang Chen , Dhiraj Kumar Hazra

Inflation is the leading theory of the first instant of the universe. Inflation, which postulates that the universe underwent a period of rapid expansion an instant after its birth, provides convincing explanation for cosmological…

天体物理仪器与方法 · 物理学 2018-06-13 A. Suzuki , P. A. R. Ade , Y. Akiba , D. Alonso , K. Arnold , J. Aumont , C. Baccigalupi , D. Barron , S. Basak , S. Beckman , J. Borrill , F. Boulanger , M. Bucher , E. Calabrese , Y. Chinone , H-M. Cho , A. Cukierman , D. W. Curtis , T. de Haan , M. Dobbs , A. Dominjon , T. Dotani , L. Duband , A. Ducout , J. Dunkley , J. M. Duval , T. Elleflot , H. K. Eriksen , J. Errard , J. Fischer , T. Fujino , T. Funaki , U. Fuskeland , K. Ganga , N. Goeckner-Wald , J. Grain , N. W. Halverson , T. Hamada , T. Hasebe , M. Hasegawa , K. Hattori , M. Hattori , L. Hayes , M. Hazumi , N. Hidehira , C. A. Hill , G. Hilton , J. Hubmayr , K. Ichiki , T. Iida , H. Imada , M. Inoue , Y. Inoue , K. D. , H. Ishino , O. Jeong , H. Kanai , D. Kaneko , S. Kashima , N. Katayama , T. Kawasaki , S. A. Kernasovskiy , R. Keskitalo , A. Kibayashi , Y. Kida , K. Kimura , T. Kisner , K. Kohri , E. Komatsu , K. Komatsu , C. L. Kuo , N. A. Kurinsky , A. Kusaka , A. Lazarian , A. T. Lee , D. Li , E. Linder , B. Maffei , A. Mangilli , M. Maki , T. Matsumura , S. Matsuura , D. Meilhan , S. Mima , Y. Minami , K. Mitsuda , L. Montier , M. Nagai , T. Nagasaki , R. Nagata , M. Nakajima , S. Nakamura , T. Namikawa , M. Naruse , H. Nishino , T. Nitta , T. Noguchi , H. Ogawa , S. Oguri , N. Okada , A. Okamoto , T. Okamura , C. Otani , G. Patanchon , G. Pisano , G. Rebeiz , M. Remazeilles , P. L. Richards , S. Sakai , Y. Sakurai , Y. Sato , N. Sato , M. Sawada , Y. Segawa , Y. Sekimoto , U. Seljak , B. D. Sherwin , T. Shimizu , K. Shinozaki , R. Stompor , H. Sugai , H. Sugita , J. Suzuki , O. Tajima , S. Takada , R. Takaku , S. Takakura , S. Takatori , D. Tanabe , E. Taylor , K. L. Thompson , B. Thorne , T. Tomaru , T. Tomida , N. Tomita , M. Tristram , C. Tucker , P. Turin , M. Tsujimoto , S. Uozumi , S. Utsunomiya , Y. Uzawa , F. Vansyngel , I. K. Wehus , B. Westbrook , M. Willer , N. Whitehorn , Y. Yamada , R. Yamamoto , N. Yamasaki , T. Yamashita , M. Yoshida

We consider a novel model of cosmic inflation. In our model one does not need any specific matter field to drive inflation, but inflation stems from the microscopic, Planck scale structure of spacetime, thus being of quantum gravitational…

广义相对论与量子宇宙学 · 物理学 2014-08-28 Jarmo Mäkelä

We describe a space-borne, multi-band, multi-beam polarimeter aiming at a precise and accurate measurement of the polarization of the Cosmic Microwave Background. The instrument is optimized to be compatible with the strict budget…

天体物理仪器与方法 · 物理学 2019-08-13 P. de Bernardis , P. A. R. Ade , J. J. A. Baselmans , E. S. Battistelli , A. Benoit , M. Bersanelli , A. Bideaud , M. Calvo , F. J. Casas , G. Castellano , A. Catalano , I. Charles , I. Colantoni , F. Columbro , A. Coppolecchia , M. Crook , G. D'Alessandro , M. De Petris , J. Delabrouille , S. Doyle , C. Franceschet , A. Gomez , J. Goupy , S. Hanany , M. Hills , L. Lamagna , J. Macias-Perez , B. Maffei , S. Martin , E. Martinez-Gonzalez , S. Masi , D. McCarthy , A. Mennella , A. Monfardini , F. Noviello , A. Paiella , F. Piacentini , M. Piat , G. Pisano , G. Signorelli , C. Y. Tan , A. Tartari , N. Trappe , S. Triqueneaux , C. Tucker , G. Vermeulen , K. Young , M. Zannoni , A. Achúcarro , R. Allison , M. Ashdown , M. Ballardini , A. J. Banday , R. Banerji , J. Bartlett , N. Bartolo , S. Basak , A. Bonaldi , M. Bonato , J. Borrill , F. Bouchet , F. Boulanger , T. Brinckmann , M. Bucher , C. Burigana , A. Buzzelli , Z. Y. Cai , C. S. Carvalho , A. Challinor , J. Chluba , S. Clesse , G. De Gasperis , G. De Zotti , E. Di Valentino , J. M. Diego , J. Errard , S. Feeney , R. Fernandez-Cobos , F. Finelli , F. Forastieri , S. Galli , R. Génova-Santos , M. Gerbino , J. González-Nuevo , S. Hagstotz , J. Greenslade , W. Handley , C. Hernández-Monteagudo , C. Hervias-Caimapo , E. Hivon , K. Kiiveri , T. Kisner , T. Kitching , M. Kunz , H. Kurki-Suonio , A. Lasenby , M. Lattanzi , J. Lesgourgues , A. Lewis , M. Liguori , V. Lindholm , G. Luzzi , C. J. A. P. Martins , A. Melchiorri , J. B. Melin , D. Molinari , P. Natoli , M. Negrello , A. Notari , D. Paoletti , G. Patanchon , L. Polastri , G. Polenta , A. Pollo , V. Poulin , M. Quartin , M. Remazeilles , M. Roman , J. A. Rubiño-Martín , L. Salvati , M. Tomasi , D. Tramonte , T. Trombetti , J. Väliviita , R. Van de Weijgaert , B. van Tent , V. Vennin , P. Vielva , N. Vittorio

The upcoming satellite missions MAP and Planck will measure the spectrum of fluctuations in the Cosmic Microwave Background with unprecedented accuracy. We discuss the prospect of using these observations to distinguish among proposed…

天体物理学 · 物理学 2007-05-23 William H. Kinney , Scott Dodelson , Edward W. Kolb
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