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We study the evolution of primordial magnetic fields in an expanding cosmic plasma. For this purpose we present a comprehensive theoretical model to consider the evolution of MHD turbulence that can be used over a wide range of physical…

宇宙学与河外天体物理 · 物理学 2016-10-12 Tina Kahniashvili , Axel Brandenburg , Alexander G. Tevzadze

Massive stars are crucial building blocks of galaxies and the universe, as production sites of heavy elements and as stirring agents and energy providers through stellar winds and supernovae. The field of magnetic massive stars has seen…

太阳与恒星天体物理 · 物理学 2015-05-27 Rolf Walder , Doris Folini , Georges Meynet

Magnetic fields have been detected in most if not all types of stars across the Hertzsprung-Russell diagram. Where present, these fields have the potential to significantly impact the evolution of their host stars. Furthermore, they…

太阳与恒星天体物理 · 物理学 2017-12-21 A. J. Martin

This review concerns the origin and the possible effects of magnetic fields in the early Universe. We start by providing to the reader with a short overview of the current state of art of observations of cosmic magnetic fields. We then…

天体物理学 · 物理学 2009-07-09 Dario Grasso , H. R. Rubinstein

Blazar observations point toward the possible presence of magnetic fields over intergalactic scales of the order of up to $\sim1\,$Mpc, with strengths of at least $\sim10^{-16}\,$G. Understanding the origin of these large-scale magnetic…

宇宙学与河外天体物理 · 物理学 2020-03-17 Tina Kahniashvili , Axel Brandenburg , Arthur Kosowsky , Sayan Mandal , Alberto Roper Pol

The evolutionary scenario of the neutron star magnetic field is examined assuming a spindown-induced expulsion of magnetic flux originally confined to the core, in which case the expelled flux undergoes ohmic decay. The nature of field…

天体物理学 · 物理学 2009-10-31 Sushan Konar , Dipankar Bhattacharya

While the presence of magnetic fields on low-mass stars is attributed to a dynamo process essentially driven by convective motions, the existence of magnetic fields on intermediate-mass stars has very likely other reasons. Presuming that…

太阳与恒星天体物理 · 物理学 2013-09-30 Rainer Arlt

Magnetic properties of quark matter are discussed in the light of the observation of pulsars. Our works about spontaneous spin polarization and spin density wave are reviewed and their implications on compact-star phenomena are discussed.…

高能物理 - 唯象学 · 物理学 2011-07-13 Toshitaka Tatsumi

In this talk, I review a number of particle-physics models that lead to the creation of magnetic fields in the early universe and address the complex problem of evolving such primordial magnetic fields into the fields observed today.…

天体物理学 · 物理学 2016-11-03 Ola Tornkvist

Neutron stars can have, in some phases of their life, extremely strong magnetic fields, up to 10^15-10^16 G. These objects, named magnetars, could be powerful sources of gravitational waves, since their magnetic field could determine large…

太阳与恒星天体物理 · 物理学 2015-05-20 L. Gualtieri , R. Ciolfi , V. Ferrari

There are indications that the magnetic field evolution in galaxies might be massively shaped by tidal interactions and mergers between galaxies. The details of the connection between the evolution of magnetic fields and that of their host…

星系天体物理 · 物理学 2022-03-15 Simon Selg , Wolfram Schmidt

Magnetars, highly magnetized neutron stars, host superconducting and superfluid phases. We develop a minimal model that captures the interplay between neutron superfluidity, proton superconductivity, and electromagnetic fields using the…

高能天体物理现象 · 物理学 2025-03-18 Sanjay Shukla , Rahul Pandit

Observational evidence for strong magnetic fields throughout the envelopes of evolved stars is increasing. Many of the instruments coming on line in the near-future will be able to make further contributions to this field. Specifically,…

太阳与恒星天体物理 · 物理学 2010-10-07 Wouter Vlemmings

Planetary magnetic fields are important indicators of planetary processes and evolution, from a planet's outer core to its surface (if it possesses one) to its atmosphere and near-space environment. Magnetic fields are most directly…

地球与行星天体物理 · 物理学 2024-04-25 David A. Brain , Melodie M. Kao , Joseph G. O'Rourke

We study the evolution of magnetic fields in turbulent hot plasma of the early Universe accounting for the chiral magnetic effect. The magnetohydrodynamic turbulence is modeled by replacing the matter velocity in the advection term in the…

宇宙学与河外天体物理 · 物理学 2018-01-17 Maxim Dvornikov

The many peculiarities of Ap stars (not only chemical ones, but also magnetic field and slow rotation) may vary during the main-sequence evolution of these stars. We review here briefly the evidences found in the last thirty years for such…

天体物理学 · 物理学 2009-06-25 P. North , J. Babel , D. Erspamer

Neutron stars host the strongest magnetic fields that we know of in the Universe. Their magnetic fields are the main means of generating their radiation, either magnetospheric or through the crust. Moreover, the evolution of the magnetic…

高能天体物理现象 · 物理学 2022-01-24 Konstantinos N. Gourgouliatos , Davide De Grandis , Andrei Igoshev

Cosmology, high-energy physics and astrophysics are converging on the study of large-scale magnetic fields. While the experimental evidence for the existence of large-scale magnetization in galaxies, clusters and superclusters is rather…

天体物理学 · 物理学 2009-11-10 Massimo Giovannini

Magnetars are the strongest magnets in the present universe and the combination of extreme magnetic field, gravity and density makes them unique laboratories to probe current physical theories (from quantum electrodynamics to general…

高能天体物理现象 · 物理学 2015-11-04 Roberto Turolla , Silvia Zane , Anna Watts

Magnetars are young and highly magnetized neutron stars which display a wide array of X-ray activity including short bursts, large outbursts, giant flares and quasi-periodic oscillations, often coupled with interesting timing behavior…

高能天体物理现象 · 物理学 2017-08-30 Victoria M. Kaspi , Andrei Beloborodov