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Recent observations of the cosmic microwave background (CMB) have extended the measured power spectrum to higher multipoles $l\gtrsim$1000, and there appears to be possible evidence for excess power on small angular scales. The primordial…

天体物理学 · 物理学 2009-02-19 D. Yamazaki , K. Ichiki , T. Kajino , G. J. Mathews

Cosmic birefringence (CB) is the rotation of the photons' linear polarisation plane during propagation. Such an effect is a tracer of parity-violating extensions of standard electromagnetism and would probe the existence of a new…

宇宙学与河外天体物理 · 物理学 2025-06-24 E. de la Hoz , P. Diego-Palazuelos , J. Errard , A. Gruppuso , B. Jost , R. M. Sullivan , M. Bortolami , Y. Chinone , L. T. Hergt , E. Komatsu , Y. Minami , I. Obata , D. Paoletti , D. Scott , P. Vielva , D. Adak , R. Akizawa , A. Anand , J. Aumont , C. Baccigalupi , A. J. Banday , R. B. Barreiro , N. Bartolo , S. Basak , A. Basyrov , M. Bersanelli , T. Brinckmann , F. Cacciotti , E. Calabrese , P. Campeti , E. Carinos , A. Carones , F. Carralot , F. J. Casas , M. Citran , L. Clermont , F. Columbro , G. Coppi , A. Coppolecchia , F. Cuttaia , P. de Bernardis , M. De Lucia , M. De Petris , S. Della Torre , E. Di Giorgi , H. K. Eriksen , E. Ferreira , F. Finelli , C. Franceschet , U. Fuskeland , G. Galloni , M. Galloway , M. Gerbino , M. Gervasi , R. T. Génova-Santos , T. Ghigna , S. Giardiello , C. Gimeno-Amo , E. Gjerløw , M. Hazumi , S. Henrot-Versillé , E. Hivon , H. Ishino , K. Kohri , L. Lamagna , M. Lattanzi , C. Leloup , M. Lembo , F. Levrier , M. López-Caniego , G. Luzzi , E. Martínez-González , S. Masi , S. Matarrese , S. Micheli , M. Migliaccio , M. Monelli , L. Montier , G. Morgante , R. Nagata , T. Namikawa , P. Natoli , A. Occhiuzzi , L. Pagano , A. Paiella , G. Pascual-Cisneros , V. Pavlidou , V. Pelgrims , F. Piacentini , G. Piccirilli , G. Polenta , L. Porcelli , N. Raffuzzi , M. Remazeilles , A. Ritacco , A. Rizzieri , J. A. Rubiño-Martín , M. Ruiz-Granda , Y. Sakurai , J. Sanghavi , M. Shiraishi , S. L. Stever , Y. Takase , K. Tassis , L. Terenzi , M. Tomasi , M. Tristram , L. Vacher , B. van Tent , D. Watts , I. K. Wehus , G. Weymann-Despres , B. Winter , E. J. Wollack , Y. Zhou

We investigate bounds on the strength of the primordial magnetic field (PMF) from the cosmic microwave background (CMB) bispectra of the intensity (temperature) modes induced from the auto- and cross-correlated bispectra of the scalar and…

宇宙学与河外天体物理 · 物理学 2012-04-02 Maresuke Shiraishi , Daisuke Nitta , Shuichiro Yokoyama , Kiyotomo Ichiki

Several missions following Planck are currently under development, which will provide high-precision measurements of the Cosmic Microwave Background (CMB) anisotropies. Specifically, measurements of the E modes will become nearly limited by…

宇宙学与河外天体物理 · 物理学 2025-07-01 Catherine Petretti , Matteo Braglia , Xingang Chen , Dhiraj Kumar Hazra , Sonia Paban

The LiteBIRD satellite is planned to be launched by JAXA in the late 2020s. Its main purpose is to observe the large-scale B-mode polarization in the Cosmic Microwave Background (CMB) anticipated from the Inflation theory. LiteBIRD will…

天体物理仪器与方法 · 物理学 2021-01-22 Mayu Tominaga , Masahiro Tsujimoto , Samantha Lynn Stever , Tommaso Ghigna , Hirokazu Ishino , Ken Ebisawa

Primordial magnetic fields (PMFs) may significantly influence 21-cm physics via two mechanisms: (i) magnetic heating of the intergalactic medium (IGM) through ambipolar diffusion (AD) and decaying magnetohydrodynamic turbulence (DT), (ii)…

宇宙学与河外天体物理 · 物理学 2025-01-27 Arko Bhaumik , Debarun Paul , Supratik Pal

The primordial magnetic fields (PMFs) produced in the early universe are expected to be the origin of the large-scale cosmic magnetic fields. The PMFs are considered to leave a footprint on the cosmic microwave background (CMB) anisotropies…

宇宙学与河外天体物理 · 物理学 2021-05-17 Teppei Minoda , Kiyotomo Ichiki , Hiroyuki Tashiro

We constrain a stochastic background of primordial magnetic field (PMF) by its contribution to the angular power spectrum of cosmic microwave background anisotropies. We parametrize such stochastic background by a power-law spectrum with…

宇宙学与河外天体物理 · 物理学 2015-05-18 Daniela Paoletti , Fabio Finelli

We show that the new precise measurements of Cosmic Microwave Background (CMB) temperature and polarization anisotropies made by the Planck satellite significantly improves previous constraints on the cosmic gravitational waves background…

宇宙学与河外天体物理 · 物理学 2016-10-17 Luca Pagano , Laura Salvati , Alessandro Melchiorri

Multi-field inflation models and non-Bunch-Davies vacuum initial conditions both predict sizeable non-Gaussian primordial perturbations and anisotropic $\mu$-type spectral distortions of the cosmic microwave background (CMB) blackbody.…

宇宙学与河外天体物理 · 物理学 2022-02-23 Mathieu Remazeilles , Andrea Ravenni , Jens Chluba

Faraday Rotation (FR) of CMB polarization, as measured through mode-coupling correlations of E and B modes, can be a promising probe of a stochastic primordial magnetic field (PMF). While the existence of a PMF is still hypothetical, there…

宇宙学与河外天体物理 · 物理学 2013-10-02 Soma De , Levon Pogosian , Tanmay Vachaspati

Primordial magnetic fields lead to non-Gaussian signals in the cosmic microwave background (CMB) even at the lowest order, as magnetic stresses and the temperature anisotropy they induce depend quadratically on the magnetic field. In…

宇宙学与河外天体物理 · 物理学 2011-01-17 Pranjal Trivedi , Kandaswamy Subramanian , T. R. Seshadri

In this work we investigate the effects of the primordial magnetic fields on cosmic microwave background anisotropies (CMB). Based on cosmological magnetohydrodynamic (MHD) simulations we calculate the CMB anisotropy spectra and…

天体物理学 · 物理学 2009-11-13 Hiroyuki Tashiro , Naoshi Sugiyama , Robi Banerjee

The primordial magnetic field (PMF) can strongly affect the cosmic microwave background (CMB) power spectrum and the formation of large scale structure. In this presentation, we calculate the CMB temperature anisotropies generated by…

天体物理学 · 物理学 2008-11-26 Dai G. Yamazaki , Kiyotomo Ichiki , Toshitaka Kajino , Grant J. Mathews

Primordial magnetic fields (PMFs), which were generated in the early Universe before recombination, affect the motion of plasma and then the cosmic microwave background and the matter power spectrum. We consider constraints on PMFs with a…

宇宙学与河外天体物理 · 物理学 2013-12-03 Dai G. Yamazaki , Kiyotomo Ichiki , Keitaro Takahashi

We update and extend our previous CMB anisotropy constraints on primordial magnetic fields through their dissipation by ambipolar diffusion and MHD decaying turbulence effects on the post-recombination ionization history. We derive the…

宇宙学与河外天体物理 · 物理学 2022-10-26 D. Paoletti , J. Chluba , F. Finelli , J. A. Rubiño-Martin

LiteBIRD is the Cosmic Microwave Background (CMB) radiation polarization satellite mission led by ISAS/JAXA. The main scientific goal is to search for primordial gravitational wave signals generated from the inflation epoch of the Universe.…

Tangled, primordial cosmic magnetic fields create small rotational velocity perturbations on the last scattering surface (LSS) of the cosmic microwave background radiation (CMBR). Such perturbations can contribute significantly to the CMBR…

天体物理学 · 物理学 2009-11-07 Kandaswamy Subramanian , T. R. Seshadri , John. D. Barrow

The absence of large-angle correlations in the temperature of the cosmic microwave background (CMB), confirmed by three independent satellite missions, creates significant tension with the standard model of cosmology. Previous work has…

宇宙学与河外天体物理 · 物理学 2024-04-15 Jingwei Liu , Fulvio Melia

Cosmic Microwave Background (CMB) polarization B-modes induced by Faraday Rotation (FR) can provide a distinctive signature of primordial magnetic fields because of their characteristic frequency dependence and because they are only weakly…

宇宙学与河外天体物理 · 物理学 2013-06-11 Levon Pogosian , Tanmay Vachaspati , Amit Yadav