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相关论文: New Constraints on the Primordial Magnetic Field

200 篇论文

We study primordial magnetic field effects on the matter perturbations in the Universe. We assume magnetic field generation prior to the big bang nucleosynthesis (BBN), i.e. during the radiation dominated epoch of the Universe expansion,…

宇宙学与河外天体物理 · 物理学 2015-06-12 Tina Kahniashvili , Yurii Maravin , Aravind Natarajan , Nicholas Battaglia , Alexander G. Tevzadze

Primordial magnetic fields (PMFs) can enhance matter power spectrum on small scales ($\lesssim$ Mpc) and still agree with bounds from cosmic microwave background (CMB) and Faraday rotation measurements. As modes on scales smaller than Mpc…

宇宙学与河外天体物理 · 物理学 2024-07-19 Pranjal Ralegankar , Mak Pavičević , Matteo Viel

The cosmological magnetic field is one of the important physical quantities which affect strongly the cosmic microwave background (CMB) power spectrum. Recent CMB observations have been extended to higher multipoles $l\gtrsim$1000, and they…

天体物理学 · 物理学 2009-11-10 D. G. Yamazaki , K. Ichiki , T. Kajino

Cosmic magnetic fields are observed to be coherent on large scales and could have a primordial origin. Non-Gaussian signals in the cosmic microwave background (CMB) are generated by primordial magnetic fields as the magnetic stresses and…

宇宙学与河外天体物理 · 物理学 2014-03-05 Pranjal Trivedi , Kandaswamy Subramanian , T. R. Seshadri

Measuring the primordial matter power spectrum is our primary means of probing unknown physics in the very early universe. We allow the primordial power spectrum to be an arbitrary function, and parametrize it in terms of wavelet band…

天体物理学 · 物理学 2009-11-07 Pia Mukherjee , Yun Wang

Since the energy momentum tensor of a magnetic field always contains a spin-2 component in its anisotropic stress, stochastic primordial magnetic field (PMF) in the early universe must generate stochastic gravitational wave (GW) background.…

天体物理学 · 物理学 2010-01-27 Shuang Wang

Primordial magnetic fields (PMFs) offer a compelling explanation for the origin of observed magnetic fields, especially on extragalactic scales. Such PMFs give rise to excess of power in small scale matter perturbations that could strongly…

宇宙学与河外天体物理 · 物理学 2023-06-22 Tal Adi , Sarah Libanore , Hector Afonso G. Cruz , Ely D. Kovetz

We constrain a stochastic background of primordial magnetic fields (PMF) by its contribution to the cosmic microwave background (CMB) anisotropy angular power spectrum with the combination of WMAP 7 year and South Pole Telescope (SPT) data.…

宇宙学与河外天体物理 · 物理学 2013-10-23 Daniela Paoletti , Fabio Finelli

We investigate the impact of a stochastic background of Primordial Magnetic Fields (PMF) generated before recombination on the ionization history of the Universe and on the Cosmic Microwave Background radiation (CMB). Pre-recombination PMFs…

宇宙学与河外天体物理 · 物理学 2019-02-28 D. Paoletti , J. Chluba , F. Finelli , J. A. Rubino-Martin

Big bang nucleosynthesis (BBN) is affected by the energy density of a primordial magnetic field (PMF). For an easy derivation of constraints on models for PMF generations, we assume a PMF with a power law (PL) distribution in wave number…

宇宙学与河外天体物理 · 物理学 2012-12-14 Dai G. Yamazaki , Motohiko Kusakabe

Primordial magnetic field (PMF) is one of the feasible candidates to explain observed large-scale magnetic fields, for example, intergalactic magnetic fields. We present a new mechanism that brings us information about PMFs on small scales…

宇宙学与河外天体物理 · 物理学 2020-05-28 Shohei Saga , Hiroyuki Tashiro , Shuichiro Yokoyama

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

We discuss whether an unaccounted contribution to the Cosmic Microwave Background polarization $B$-mode by primordial magnetic fields (PMFs) can bias future constraints on inflationary gravitational waves. As a case-study, we consider a…

宇宙学与河外天体物理 · 物理学 2018-09-05 Fabrizio Renzi , Giovanni Cabass , Eleonora Di Valentino , Alessandro Melchiorri , Luca Pagano

We discuss the manner in which the primordial magnetic field (PMF) suppresses the cosmic microwave background (CMB) $B$ mode due to the weak-lensing (WL) effect. The WL effect depends on the lensing potential (LP) caused by matter…

宇宙学与河外天体物理 · 物理学 2018-05-28 Dai G. Yamazaki

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

Spatially varying primordial magnetic fields may be efficiently dissipated prior to the epoch of recombination due to the large viscosity of the baryon-photon fluid. We show that this dissipation may result in observable chemical potential…

天体物理学 · 物理学 2009-10-31 K. Jedamzik , V. Katalinic , A. V. Olinto

Primordial magnetic fields (PMFs) can source gravitational wave background (GWB). In this paper, we investigate the possible constraints on small-scale PMF considering the ongoing and forthcoming direct detection observations of GWB. In…

宇宙学与河外天体物理 · 物理学 2018-12-18 Shohei Saga , Hiroyuki Tashiro , Shuichiro Yokoyama

The effects of magnetic fields on Big Bang Nucleosynthesis(BBN) have been calculated, and the impact on the abundances of the light elements have been investigated numerically. An upper limit on the strength of primordial magnetic fields…

天体物理学 · 物理学 2009-12-30 Baolian Cheng , David N. Schramm , James W. Truran

The oscillation feature in primordial power spectrum (PPS), a fingerprint of not only a wide class of models of inflation but new physics, is of significant theoretical interest, and can be imprinted on the cosmic microwave background…

宇宙学与河外天体物理 · 物理学 2025-08-19 Ze-Yu Peng , Yun-Song Piao

We constrain a primordial magnetic field (PMF) generated during a phase transition (PT) using the big bang nucleosynthesis bound on the relativistic energy density. The amplitude of the PMF at large scales is determined by the shape of the…

宇宙学与河外天体物理 · 物理学 2011-01-04 Tina Kahniashvili , Alexander G. Tevzadze , Bharat Ratra