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Magnetophoretic force acting on a rigid spherical cluster of single-domain nanoparticles in a constant-gradient weak magnetic field is investigated numerically using the Langevin dynamics simulation method. Nanoparticles are randomly and…

Mesoscale and Nanoscale Physics · Physics 2018-12-05 Andrey A. Kuznetsov

This paper deals with the design of the stellarator field with the simple coil set. In order to realize the stellarator field by the simple coil set, the tilted toroidal field coil uses for creating the rotational transform. Sixteen tilted…

Plasma Physics · Physics 2020-12-01 Yasuhiro Suzuki , Jie Huang , Nengchao Wang , Yonghua Ding

From a detailed analysis of cone-jet cross sections in effective field theory, we obtain novel factorization theorems which separate the physics associated with different energy scales present in such processes. The relevant low-energy…

High Energy Physics - Phenomenology · Physics 2017-05-08 Thomas Becher , Matthias Neubert , Lorena Rothen , Ding Yu Shao

(shortened) Planet forming discs are believed to be very weakly turbulent in the regions outside of 1 AU. For this reason, it is now believed that magnetized winds could be the dominant mechanism driving accretion in these systems. However,…

Solar and Stellar Astrophysics · Physics 2021-06-02 Geoffroy Lesur

We study the coupling of the force-free magnetosphere to the long-term internal evolution of a magnetar. We allow the relation between the poloidal and toroidal stream functions - that characterizes the magnetosphere - to evolve freely…

High Energy Astrophysical Phenomena · Physics 2018-10-17 Taner Akgün , Pablo Cerdá-Durán , Juan Antonio Miralles , José A. Pons

The effective potential energy of the particles in the field of rotating uniformly magnetized celestial body is investigated. The axis of rotation coincides with the axis of the magnetic field. Electromagnetic field of the body is composed…

High Energy Astrophysical Phenomena · Physics 2018-01-11 V. Epp , O. N. Pervukhina

In the paradigm of magnetic launching of astrophysical jets, instabilities in the MHD flow are a good candidate to convert the Poynting flux into the kinetic energy of the plasma. If the magnetised plasma fills the almost entire space, the…

High Energy Astrophysical Phenomena · Physics 2017-10-04 E. Sobacchi , Y. E. Lyubarsky

Mechanical resonators made with monolithic piezoelectric quartz crystals are promising for studying new physical phenomena. High mechanical quality factors ($Q$) exhibited by the mm-sized quartz resonators make them ideal for studying weak…

Applied Physics · Physics 2018-06-21 Alpo Valimaa , Jorge Santos , Caspar Ockeloen-Korppi , Mika Sillanpaa

This study presents several novel approaches to improve the efficiency of a single-stage coil gun. Conventional designs typically feature a uniformly wound solenoid and a ferrite projectile. For our research, we constructed a…

Systems and Control · Electrical Eng. & Systems 2024-10-11 Sophia Chen , Annie Peng , Ava Chen , Takyiu Liu

Broken symmetries in solids involving higher order multipolar degrees of freedom are historically referred to as "hidden orders" due to the formidable task of detecting them with conventional probes. Examples of such hidden orders include…

Strongly Correlated Electrons · Physics 2019-09-10 Adarsh S. Patri , Akito Sakai , SungBin Lee , Arun Paramekanti , Satoru Nakatsuji , Yong Baek Kim

Analytically the forces and torques on a coil in a field of magnetic flux density can be calculated one of two ways. The line integral can be conducted along the coil's wire, summing up the differential force contribution. For each…

Instrumentation and Detectors · Physics 2022-09-20 Stephan Schlamminger , Lorenz Keck , Frank Seifert , Leon S. Chao , Darine Haddad , Shisong Li

The structure of protostellar cores can often be approximated by isothermal Bonnor-Ebert spheres (BES) which are stabilized by an external pressure. For the typical pressure of $10^4k_B\,\mathrm{K\,cm^{-3}}$ to…

Astrophysics of Galaxies · Physics 2021-07-07 Oliver Zier , Andreas Burkert , Christian Alig

Factorization is possible due to the universal behavior of Yang-Mills theories in soft and collinear limits. Here, we take a small step towards a more transparent understanding of these limits by proving a form of perturbative factorization…

High Energy Physics - Theory · Physics 2013-09-25 Ilya Feige , Matthew D. Schwartz

We investigate the properties of magnetized stars in the propeller regime using axisymmetric numerical simulations. We modelled the propeller regime for stars with realistically large magnetospheres (5-7 stellar radii), so that our results…

Solar and Stellar Astrophysics · Physics 2018-02-21 Marina M. Romanova , Alisa A. Blinova , Galina V. Ustyugova , Alexander V. Koldoba , Richard V. E. Lovelace

We extend the ModeCode software of Mortonson, Peiris and Easther to enable numerical computation of perturbations in K-inflation models, where the scalar field no longer has a canonical kinetic term. Focussing on models where the kinetic…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-04 Sheng Li , Andrew R. Liddle

The component of the neoclassical electrostatic potential that is non-constant on the magnetic surface, that we denote by $\tilde\varphi$, can affect radial transport of highly charged impurities, and this has motivated its inclusion in…

Plasma Physics · Physics 2018-09-12 Ivan Calvo , J. L. Velasco , Felix I. Parra , J. Arturo Alonso , J. M. García-Regaña

Magnetars are a kind of pulsars powered mainly by superhigh magnetic fields. They are popular sources with many unsolved issues in themselves, but also linked to various high energy phenomena, such as QPOs, giant flares, fast radio bursts…

High Energy Astrophysical Phenomena · Physics 2021-03-31 Zhi-Fu Gao , Hao Shan , Hui Wang

Tight tolerances have been a leading driver of cost in recent stellarator experiments, so improved definition and control of tolerances can have significant impact on progress in the field. Here we relate tolerances to the shape gradient…

Plasma Physics · Physics 2018-03-09 Matt Landreman , Elizabeth J Paul

We carried out axisymmetric simulations of disk accretion to a rapidly rotating magnetized star in the "propeller" regime. Simulations show that propellers may be "weak" (with no outflows), and "strong" (with outflows). Investigation of the…

Solar and Stellar Astrophysics · Physics 2009-01-28 M. M. Romanova , R. V. E. Lovelace , G. V. Ustyugova , A. V. Koldoba

We critically examine the theory of disk locking, which assumes that the angular momentum deposited on an accreting protostar is exactly removed by torques carried along magnetic field lines connecting the star to the disk. In this letter,…

Astrophysics · Physics 2009-11-10 Sean Matt , Ralph E. Pudritz
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