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We present the discovery of a magnetic field on the white dwarf component in the detached post common envelope binary (PCEB) CC Cet. Magnetic white dwarfs in detached PCEBs are extremely rare, in contrast to the high incidence of magnetism…

太阳与恒星天体物理 · 物理学 2021-09-08 David J. Wilson , Odette Toloza , John D. Landstreet , Boris T. Gaensicke , Jeremy J. Drake , J. J. Hermes , Detlev Koester

Like the solar corona, the external magnetic field of magnetars is twisted by surface motions of the star. The twist energy is dissipated over time. We discuss the theory of this activity and its observational status. (1) Theory predicts…

高能天体物理现象 · 物理学 2015-05-19 Andrei M. Beloborodov

We report on nonequilibrium transport measurements in a high-mobility two-dimensional electron system subject to weak magnetic field and dc excitation. Detailed study of dc-induced magneto-oscillations, first observed by Yang {\em et al}.,…

介观与纳米尺度物理 · 物理学 2007-05-23 W. Zhang , H. -S. Chiang , M. A. Zudov , L. N. Pfeiffer , K. W. West

Since their initial discovery, the origin of isolated white dwarfs (WDs) with magnetic fields in excess of $\sim$1 MG has remained a mystery. Recently, the formation of these high-field magnetic WDs has been observationally linked to strong…

太阳与恒星天体物理 · 物理学 2015-05-30 J. Nordhaus

We study the temperature evolution of the non-linear oscillatory magnetoresistance in a high-mobility two-dimensional electron system subject to a strong dc electric field. We find that the decay of the oscillation amplitude with increasing…

介观与纳米尺度物理 · 物理学 2009-04-29 A. T. Hatke , M. A. Zudov , L. N. Pfeiffer , K. W. West

A dynamo mechanism driven by differential rotation when stars merge has been proposed to explain the presence of strong fields in certain classes of magnetic stars. In the case of the high field magnetic white dwarfs (HFMWDs), the site of…

太阳与恒星天体物理 · 物理学 2018-05-16 Gordon P. Briggs , Lilia Ferrario , Christopher A. Tout , Dayal T. Wickramasinghe

Accreting X-Ray Binaries display a wide range of behaviours. Some of them are observed to spin up steadily, others to alternate between spin-up and spin-down states, sometimes superimposed on a longer trend of either spin up or spin down.…

天体物理学 · 物理学 2009-11-13 Rosalba Perna , Enrico Bozzo , Luigi Stella

We report on magnetotransport measurements in a high-mobility two-dimentional electron system subject simultaneously to AC (microwave) and DC (Hall) fields. We find that DC excitation affects microwave photoresistance in a nontrivial way.…

介观与纳米尺度物理 · 物理学 2007-05-23 W. Zhang , M. A. Zudov , L. N. Pfeiffer , K. W. West

The relevance of pair-breaking by exchange and dipolar fields, and by injected spins in a low carrier density cuprate Y$_{1-x}$Pr$_x$Ba$_2$Cu$_3$O$_7$ sandwiched between two ferromagnetic La$_{2 / 3}$Sr$_{1 / 3}$MnO$_{3}$ layers is…

超导电性 · 物理学 2011-08-01 Soumen Mandal , R. C. Budhani , Jiaqing He , Y. Zhu

Some short-period, detached binary systems have recently been reported to experience very rapid orbital decay, much faster than is expected from the angular-momentum loss caused by gravitational radiation alone. As these systems contain…

太阳与恒星天体物理 · 物理学 2017-03-15 Wen-Cong Chen , Philipp Podsiadlowski

The magnetic white dwarfs (MWDs) are found either isolated or in interacting binaries. They divide into two groups: a high field group (0.1-1,000MegaGauss) comprising some 13% of all white dwarfs (WDs), and a low field group (B<0.1MG) whose…

太阳与恒星天体物理 · 物理学 2020-01-29 Lilia Ferrario , D. T. Wickramasinghe , Adela Kawka

Observations of magnetic A, B and O stars show that the poloidal magnetic flux per unit mass has an upper bound of 10^-6.5 G cm^2/g. A similar upper bound is found for magnetic white dwarfs even though the highest magnetic field strengths…

太阳与恒星天体物理 · 物理学 2015-06-17 Dayal T. Wickramasinghe , Christopher A. Tout , Lilia Ferrario

We propose a model for stellar binary systems consisting of a magnetic and a non-magnetic white-dwarf pair which is powered principally by electrical energy. In our model the luminosity is caused by resistive heating of the stellar…

天体物理学 · 物理学 2009-11-07 Kinwah Wu , Mark Cropper , Gavin Ramsay , Kazuhiro Sekiguchi

Wickramasinghe et al. (2014) and Briggs et al. (2015) have proposed that the strong magnetic fields observed in some single white dwarfs (MWDs) are formed by a dynamo driven by differential rotation when two stars, the more massive one with…

太阳与恒星天体物理 · 物理学 2018-01-31 G. Briggs , Lilia Ferrario , C. A. Tout , D. T. Wickramasinghe

In a series of recent papers, it has been proposed that high field magnetic white dwarfs are the result of close binary interaction and merging. Population synthesis calculations have shown that the origin of isolated highly magnetic white…

太阳与恒星天体物理 · 物理学 2018-10-16 Gordon P. Briggs , Lilia Ferrario , Christopher A. Tout , Dayal T. Wickramasinghe

The dc magnetoconductivity of the multisubband two-dimensional electron system formed on the liquid helium surface in the presence of resonant microwave irradiation is described, and a new mechanism of the negative linear response…

介观与纳米尺度物理 · 物理学 2015-03-19 Yuriy P. Monarkha

We discuss the possibility to obtain an electromagnetic emission accompanying the gravitational waves emitted in the coalescence of a compact binary system. Motivated by the existence of black hole configurations with open magnetic field…

高能天体物理现象 · 物理学 2015-05-27 S. Capozziello , M. De Laurentis , I. De Martino , M. Formisano , D. Vernieri

In a recent paper Martin & Lubow showed that a circumbinary disc around an eccentric binary can undergo damped nodal oscillations that lead to the polar (perpendicular) alignment of the disc relative to the binary orbit. The disc angular…

地球与行星天体物理 · 物理学 2018-07-04 Rebecca G. Martin , Stephen H. Lubow

Nanomagnetism concerns the engineering of magnetic interactions in heterostructures that consist of layers of magnetic and non-magnetic materials. Mostly, these interactions are dominated by the minimization of energy. Here, we propose an…

介观与纳米尺度物理 · 物理学 2025-05-21 William Huddie , Laura Filion , Marjolein Dijkstra , Rembert Duine

Intrinsic magnetic fields have long been thought to shield planets from atmospheric erosion via stellar winds; however, the influence of the plasma environment on atmospheric escape is complex. Here we study the influence of a weak…

地球与行星天体物理 · 物理学 2019-07-09 Hilary Egan , Riku Jarvinen , Yingjuan Ma , David Brain