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Measuring spectral distortions (SDs) of the cosmic microwave background (CMB) will provide new constraints on previously unexplored scales of the primordial power spectrum, allowing us to extend the probed parameter space by several orders…

宇宙学与河外天体物理 · 物理学 2021-05-03 Nils Schöneberg , Matteo Lucca , Deanna C. Hooper

Cosmic microwave background (CMB) photons are deflected by large-scale structure through gravitational lensing. This secondary effect introduces higher-order correlations in CMB anisotropies, which are used to reconstruct lensing…

宇宙学与河外天体物理 · 物理学 2025-11-26 M. Ruiz-Granda , P. Diego-Palazuelos , C. Gimeno-Amo , P. Vielva , A. I. Lonappan , T. Namikawa , R. T. Génova-Santos , M. Lembo , R. Nagata , M. Remazeilles , D. Adak , E. Allys , A. Anand , J. Aumont , C. Baccigalupi , M. Ballardini , A. J. Banday , R. B. Barreiro , N. Bartolo , S. Basak , M. Bersanelli , A. Besnard , D. Blinov , M. Bortolami , F. Bouchet , T. Brinckmann , F. Cacciotti , E. Calabrese , P. Campeti , A. Carones , F. J. Casas , K. Cheung , M. Citran , L. Clermont , F. Columbro , A. Coppolecchia , P. de Bernardis , T. de Haan , E. de la Hoz , M. De Lucia , S. Della Torre , E. Di Giorgi , H. K. Eriksen , F. Finelli , C. Franceschet , U. Fuskeland , G. Galloni , M. Galloway , M. Gervasi , T. Ghigna , S. Giardiello , A. Gruppuso , M. Hazumi , L. T. Hergt , E. Hivon , K. Ichiki , H. Jiang , B. Jost , K. Kohri , L. Lamagna , M. Lattanzi , C. Leloup , F. Levrier , M. López-Caniego , G. Luzzi , J. Macias-Perez , V. Maranchery , E. Martínez-González , S. Masi , S. Matarrese , T. Matsumura , S. Micheli , M. Monelli , L. Montier , G. Morgante , M. Najafi , A. Novelli , F. Noviello , I. Obata , A. Occhiuzzi , A. Paiella , D. Paoletti , G. Pascual-Cisneros , F. Piacentini , G. Piccirilli , G. Polenta , L. Porcelli , N. Raffuzzi , A. Rizzieri , J. A. Rubiño-Martín , Y. Sakurai , J. Sanghavi , D. Scott , M. Shiraishi , G. Signorelli , R. M. Sullivan , Y. Takase , L. Terenzi , M. Tomasi , M. Tristram , L. Vacher , B. van Tent , I. K. Wehus , G. Weymann-Despres , Y. Zhou

Future Cosmic Microwave Background (CMB) experiments will deliver extremely accurate measurements of the E-modes pattern of the CMB polarization field. Given the sharpness of the E-modes transfer functions, such surveys make for a powerful…

宇宙学与河外天体物理 · 物理学 2023-03-15 Matteo Braglia , Xingang Chen , Dhiraj Kumar Hazra , Lucas Pinol

Using a set of cosmological hydro-dynamical simulations, we constrained the properties of primordial magnetic fields by studying their impact on the formation and evolution of dwarf galaxies. We performed a large set of simulations (8 dark…

星系天体物理 · 物理学 2020-11-04 Mahsa Sanati , Yves Revaz , Jennifer Schober , Kerstin E. Kunze , Pascale Jablonka

Magnetic fields are everywhere in nature and they play an important role in every astronomical environment which involves the formation of plasma and currents. It is natural therefore to suppose that magnetic fields could be present in the…

宇宙学与河外天体物理 · 物理学 2011-12-22 Dai G. Yamazaki , Kiyotomo Ichiki , Toshitaka Kajino , Grant J. Mathew

A primordial magnetic field in the early universe will cause Faraday rotation of the linear polarization of the cosmic microwave background generated via Compton scattering at the surface of last scattering. This rotation induces a non-zero…

天体物理学 · 物理学 2009-08-11 Tina Kahniashvili , Yurii Maravin , Arthur Kosowsky

We study how the next generation of Cosmic Microwave Background (CMB) measurement missions (such as EPIC, LiteBIRD, PRISM and COrE) will be able to constrain the inflationary landscape in the hardest to disambiguate situation in which…

宇宙学与河外天体物理 · 物理学 2014-10-30 Jerome Martin , Christophe Ringeval , Vincent Vennin

LiteBIRD, a forthcoming satellite mission, aims to measure the polarization of the Cosmic Microwave Background (CMB) across the entire sky. The experiment will employ three telescopes, Transition-Edge Sensor (TES) bolometers and rotating…

After the precise observations of the Cosmic Microwave Background (CMB) anisotropy power spectrum, attention is now being focused on the higher order statistics of the CMB anisotropies. Since linear evolution preserves the statistical…

天体物理学 · 物理学 2009-11-10 Daniel Babich , Matias Zaldarriaga

We present the first results from SPHINX-MHD, a suite of cosmological radiation-magnetohydrodynamics simulations designed to study the impact of primordial magnetic fields (PMFs) on galaxy formation and the evolution of the intergalactic…

The search for primordial gravitational waves through the $B$-mode polarization pattern in the CMB is one of the major goals of current and future CMB experiments. Besides foregrounds, a potential hurdle in this search is the anisotropic…

宇宙学与河外天体物理 · 物理学 2021-01-06 Anirban Roy , Girish Kulkarni , P. Daniel Meerburg , Anthony Challinor , Carlo Baccigalupi , Andrea Lapi , Martin G. Haehnelt

Recent developments of transition-edge sensors (TESs), based on extensive experience in ground-based experiments, have been making the sensor techniques mature enough for their application on future satellite CMB polarization experiments.…

天体物理仪器与方法 · 物理学 2021-04-06 H. Sugai , P. A. R. Ade , Y. Akiba , D. Alonso , K. Arnold , J. Aumont , J. Austermann , C. Baccigalupi , A. J. Banday , R. Banerji , R. B. Barreiro , S. Basak , J. Beall , S. Beckman , M. Bersanelli , J. Borrill , F. Boulanger , M. L. Brown , M. Bucher , A. Buzzelli , E. Calabrese , F. J. Casas , A. Challinor , V. Chan , Y. Chinone , J. -F. Cliche , F. Columbro , A. Cukierman , D. Curtis , P. Danto , P. de Bernardis , T. de Haan , M. De Petris , C. Dickinson , M. Dobbs , T. Dotani , L. Duband , A. Ducout , S. Duff , A. Duivenvoorden , J. -M. Duval , K. Ebisawa , T. Elleflot , H. Enokida , H. K. Eriksen , J. Errard , T. Essinger-Hileman , F. Finelli , R. Flauger , C. Franceschet , U. Fuskeland , K. Ganga , J. -R. Gao , R. Génova-Santos , T. Ghigna , A. Gomez , M. L. Gradziel , J. Grain , F. Grupp , A. Gruppuso , J. E. Gudmundsson , N. W. Halverson , P. Hargrave , T. Hasebe , M. Hasegawa , M. Hattori , M. Hazumi , S. Henrot-Versille , D. Herranz , C. Hill , G. Hilton , Y. Hirota , E. Hivon , R. Hlozek , D. -T. Hoang , J. Hubmayr , K. Ichiki , T. Iida , H. Imada , K. Ishimura , H. Ishino , G. C. Jaehnig , M. Jones , T. Kaga , S. Kashima , Y. Kataoka , N. Katayama , T. Kawasaki , R. Keskitalo , A. Kibayashi , T. Kikuchi , K. Kimura , T. Kisner , Y. Kobayashi , N. Kogiso , A. Kogut , K. Kohri , E. Komatsu , K. Komatsu , K. Konishi , N. Krachmalnicoff , C. L. Kuo , N. Kurinsky , A. Kushino , M. Kuwata-Gonokami , L. Lamagna , M. Lattanzi , A. T. Lee , E. Linder , B. Maffei , D. Maino , M. Maki , A. Mangilli , E. Martínez-González , S. Masi , R. Mathon , T. Matsumura , A. Mennella , M. Migliaccio , Y. Minami , K. Mistuda , D. Molinari , L. Montier , G. Morgante , B. Mot , Y. Murata , J. A. Murphy , M. Nagai , R. Nagata , S. Nakamura , T. Namikawa , P. Natoli , S. Nerva , T. Nishibori , H. Nishino , Y. Nomura , F. Noviello , C. O'Sullivan , H. Ochi , H. Ogawa , H. Ogawa , H. Ohsaki , I. Ohta , N. Okada , N. Okada , L. Pagano , A. Paiella , D. Paoletti , G. Patanchon , F. Piacentini , G. Pisano , G. Polenta , D. Poletti , T. Prouvé , G. Puglisi , D. Rambaud , C. Raum , S. Realini , M. Remazeilles , G. Roudil , J. A. Rubiño-Martín , M. Russell , H. Sakurai , Y. Sakurai , M. Sandri , G. Savini , D. Scott , Y. Sekimoto , B. D. Sherwin , K. Shinozaki , M. Shiraishi , P. Shirron , G. Signorelli , G. Smecher , P. Spizzi , S. L. Stever , R. Stompor , S. Sugiyama , A. Suzuki , J. Suzuki , E. Switzer , R. Takaku , H. Takakura , S. Takakura , Y. Takeda , A. Taylor , E. Taylor , Y. Terao , K. L. Thompson , B. Thorne , M. Tomasi , H. Tomida , N. Trappe , M. Tristram , M. Tsuji , M. Tsujimoto , C. Tucker , J. Ullom , S. Uozumi , S. Utsunomiya , J. Van Lanen , G. Vermeulen , P. Vielva , F. Villa , M. Vissers , N. Vittorio , F. Voisin , I. Walker , N. Watanabe , I. Wehus , J. Weller , B. Westbrook , B. Winter , E. Wollack , R. Yamamoto , N. Y. Yamasaki , M. Yanagisawa , T. Yoshida , J. Yumoto , M. Zannoni , A. Zonca

Various so-called anomalies have been found in both the WMAP and Planck cosmic microwave background (CMB) temperature data that exert a mild tension against the highly successful best-fit 6 parameter cosmological model, potentially…

宇宙学与河外天体物理 · 物理学 2025-08-25 A. J. Banday , C. Gimeno-Amo , P. Diego-Palazuelos , E. de la Hoz , A. Gruppuso , N. Raffuzzi , E. Martínez-González , P. Vielva , R. B. Barreiro , M. Bortolami , C. Chiocchetta , G. Galloni , D. Scott , R. M. Sullivan , D. Adak , E. Allys , A. Anand , J. Aumont , C. Baccigalupi , M. Ballardini , N. Bartolo , S. Basak , M. Bersanelli , A. Besnard , D. Blinov , F. Bouchet , T. Brinckmann , F. Cacciotti , E. Calabrese , P. Campeti , A. Carones , F. J. Casas , K. Cheung , M. Citran , L. Clermont , F. Columbro , A. Coppolecchia , P. de Bernardis , M. De Lucia , S. Della Torre , E. Di Giorgi , H. K. Eriksen , F. Finelli , C. Franceschet , U. Fuskeland , M. Galloway , M. Gervasi , R. T. Génova-Santos , T. Ghigna , S. Giardiello , M. Hazumi , L. T. Hergt , E. Hivon , K. Ichiki , H. Ishino , B. Jost , K. Kohri , L. Lamagna , M. Lattanzi , C. Leloup , F. Levrier , A. I. Lonappan , M. López-Caniego , G. Luzzi , J. Macias-Perez , V. Maranchery , S. Masi , S. Matarrese , T. Matsumura , S. Micheli , M. Migliaccio , M. Monelli , L. Montier , G. Morgante , M. Najafi , T. Namikawa , A. Novelli , I. Obata , A. Occhiuzzi , A. Paiella , D. Paoletti , G. Pascual-Cisneros , F. Piacentini , G. Piccirilli , G. Polenta , L. Porcelli , M. Remazeilles , A. Rizzieri , J. A. Rubiño-Martín , M. Ruiz-Granda , Y. Sakurai , J. Sanghavi , M. Shiraishi , G. Signorelli , Y. Takase , L. Terenzi , M. Tomasi , M. Tristram , L. Vacher , B. van Tent , I. K. Wehus , G. Weymann-Despres , E. J. Wollack , Y. Zhou

Primordial magnetic fields will generate non-Gaussian signals in the cosmic microwave background (CMB) as magnetic stresses and the temperature anisotropy they induce depend quadratically on the magnetic field. We compute a new measure of…

宇宙学与河外天体物理 · 物理学 2012-06-15 Pranjal Trivedi , T. R. Seshadri , Kandaswamy Subramanian

We derive updated Cosmic Microwave Background (CMB) constraints on annihilating dark matter, and present forecasts for upcoming CMB surveys. We show that the addition of recent temperature, polarization, and lensing data from ground-based…

宇宙学与河外天体物理 · 物理学 2025-12-12 Charlotte Myers , Dominic Agius , Daniele Gaggero , Angelo Ricciardone

Cosmic microwave background polarization encodes information not only on the early universe but also dark energy, neutrino mass, and gravity in the late universe through CMB lensing. Ground based surveys such as ACTpol, PolarBear, SPTpol…

宇宙学与河外天体物理 · 物理学 2012-10-02 Sudeep Das , Eric V. Linder

We investigate the impact of a hypothesized delayed initiation of inflation, characterized by a cutoff k_min to the primordial power spectrum in the cosmic microwave background (CMB). This cutoff affects both the scalar and tensor spectra,…

宇宙学与河外天体物理 · 物理学 2025-07-28 Jingwei Liu , Fulvio Melia

Cosmic birefringence$-$the rotation of the polarization plane of light as it traverses the universe$-$offers a direct observational window into parity-violating physics beyond the Standard Model. In this work, we revisit the anisotropic…

宇宙学与河外天体物理 · 物理学 2025-06-27 A. I. Lonappan , B. Keating , K. Arnold

We study the impact of a stochastic background of primordial magnetic fields on the scalar contribution of CMB anisotropies and on the matter power spectrum. We give the correct initial conditions for cosmological perturbations and the…

天体物理学 · 物理学 2008-12-18 Fabio Finelli , Francesco Paci , Daniela Paoletti

Measurements of the cosmic microwave background (CMB) allow high precision observation of the cosmic plasma at redshift z~1100. After the success of the NASA satellite COBE, that in 1992 provided the first detection of the CMB anisotropy,…