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Event Horizon Telescope (EHT) observations at 230 GHz have now imaged polarized emission around the supermassive black hole in M87 on event-horizon scales. This polarized synchrotron radiation probes the structure of magnetic fields and the…

高能天体物理现象 · 物理学 2021-05-06 The Event Horizon Telescope Collaboration

Hubbard chains with periodically modulated coupling constants in a magnetic field exhibit gaps at zero temperature in their magnetic and charge excitations in a variety of situations. In addition to fully gapped situations (plateau in the…

强关联电子 · 物理学 2009-10-31 D. C. Cabra , A. De Martino , A. Honecker , P. Pujol , P. Simon

Electron drag between two two-dimensional electron gases in magnetic fields has been observed with a polarity opposite that for zero field. This negative drag requires that the electrons have a hole-like dispersion. Density dependence…

介观与纳米尺度物理 · 物理学 2009-10-31 X. G. Feng , S. Zelakiewicz , H. Noh , T. J. Ragucci , T. J. Gramila , L. N. Pfeiffer , K. W. West

A self-consistent model is presented for performing steady-state fully kinetic Particle-in-Cell simulations of magnetised plasma plumes. An energy-based electron reflection prevents the numerical pump instability associated with a typical…

等离子体物理 · 物理学 2022-02-23 Shaun Andrews , Simone Di Fede , Mirko Magarotto

We report the properties of a novel type of sub-proton scale magnetic hole found in two dimensional PIC simulations of decaying turbulence with a guide field. The simulations were performed with a realistic value for ion to electron mass…

等离子体物理 · 物理学 2015-06-23 Christopher T. Haynes , David Burgess , Enrico Camporeale , Torbjorn Sundberg

In an electron-positron plasma, an imbalance in the number of right- and left-chiral particles can lead to the growth of a helical magnetic field through a phenomenon called the chiral plasma instability (CPI). In the early universe,…

高能物理 - 唯象学 · 物理学 2025-12-11 Murman Gurgenidze , Andrew J. Long , Alberto Roper Pol , Axel Brandenburg , Tina Kahniashvili

In a spherically symmetric plasma constrained by its own gravity, the ionization degree lags behind changes in temperature and density. The ambipolar electric field accelerates ions radially and cools electrons. Ions lose energy and angular…

星系天体物理 · 物理学 2024-08-13 Haibin Chen , Rong Wu

The propulsion type plasma in oblique external magnetic field is studied in 2D3V PIC MCC simulations. A periodical structure with maxima of electron and ion densities appears with an increase of an obliqueness of magnetic field. These…

等离子体物理 · 物理学 2017-12-06 Irina Schweigert , Michael Keidar

This paper presents a solely thermal flare, which we detected in the microwave range from the thermal gyro- and free-free emission it produced. An advantage of analyzing thermal gyro emission is its unique ability to precisely yield the…

太阳与恒星天体物理 · 物理学 2015-06-23 Gregory D. Fleishman , Gelu M. Nita , Dale E. Gary

We introduce a first full analytical bubble and blow-out model for a radially inhomogeneous plasma in a quasi-static approximation. For both cases we calculate the accelerating and the focusing fields. In our model we also assume a thin…

等离子体物理 · 物理学 2016-06-14 Johannes Thomas , Igor Yu. Kostyukov , Jari Pronold , Anton Golovanov , Alexander Pukhov

We reinvestigate the generation and accumulation of magnetic flux in optically thin accretion flows around active gravitating objects. The source of the magnetic field is the azimuthal electric current associated with the Poynting-Robertson…

We present the results of direct simulation of the expansionof a two-component ultracold plasmafor various numbers of particles, densities, and electron temperatures. A description of the expansionprocess common to all plasma parameters is…

等离子体物理 · 物理学 2021-07-28 E. V. Vikhrov , S. Ya. Bronin , B. B. Zelener , B. V. Zelener

The magnetic structure in the Galactic disk, the Galactic center and the Galactic halo can be delineated more clearly than ever before. In the Galactic disk, the magnetic structure has been revealed by starlight polarization within 2 or 3…

星系天体物理 · 物理学 2009-11-13 J. L. Han

A relativistic electron-positron beam propagating through a magnetized electron-ion plasma is shown to generate both circularly and linearly polarized synchrotron radiation. The degrees of circular and linear polarizations depend both on…

等离子体物理 · 物理学 2019-05-29 Ujjwal Sinha , Christoph H. Keitel , Naveen Kumar

It is shown that the transport in low temperature, collisional, bounded plasma is enhanced by instabilities at high magnetic field. While the magnetic field confines the electrons in a stable plasma, the instability completely destroys the…

等离子体物理 · 物理学 2019-09-04 R. Lucken , A. Bourdon , M. Lieberman , P. Chabert

Unsustained matter distributions unescapely collapse unless fragmentation and centrifugal or pressure support take place. Starting from the above evidence, supermassive compact objects at the centre of large-mass galaxies are conceived as…

天体物理学 · 物理学 2009-06-23 R. Caimmi

Motivated by a scenario of magnetogenesis in which a homogeneous magnetic field is generated during inflation, we study the magnetohydrodynamic evolution of the primordial plasma motions for two kinds of initial conditions -- (i) a…

宇宙学与河外天体物理 · 物理学 2020-07-28 Axel Brandenburg , Ruth Durrer , Yiwen Huang , Tina Kahniashvili , Sayan Mandal , Shinji Mukohyama

Recent work by Mitra et al. (2014) has shown that in strongly stratified forced two-layer turbulence with helicity and corresponding large-scale dynamo action in the lower layer, a magnetic field occurs in the upper layer in the form of…

太阳与恒星天体物理 · 物理学 2015-06-03 Sarah Jabbari , Axel Brandenburg , Nathan Kleeorin , Dhrubaditya Mitra , Igor Rogachevskii

Ultracold neutral plasmas provide a useful system for studying extreme parameter regimes plasma physics in an accessible laboratory setting. The parameter space of plasma physics can be characterized in part by coupling strength and degree…

等离子体物理 · 物理学 2026-02-27 Ryan C. Baker , Bridget O'Mara , Jacob L. Roberts

A recent single quantum wire is of sufficient quality to reveal new details of the photoluminescence (PL) evolution with increasing electron--hole (e--h) pair density. At a pair density of 3.6 $\times$ 10$^{3}$ cm$^{-1}$, the PL is…

介观与纳米尺度物理 · 物理学 2007-05-23 Masahiro Yoshita , Yuhei Hayamizu , Hidefumi Akiyama , Loren N. Pfeiffer , Ken W. West , Kenichi Asano , Tetsuo Ogawa