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Related papers: Dynamical Friction in Superfluids

200 papers

Dynamical friction arises from the interaction of a perturber and the gravitational wake it excites in the ambient medium. This interaction is usually derived assuming that the perturber has a constant velocity. In realistic situations,…

Astrophysics of Galaxies · Physics 2009-11-25 Fathi Namouni

Any gravitating mass traversing a relatively sparse gas experiences a retarding force created by its disturbance of the surrounding medium. In a previous contribution (Lee & Stahler 2011), we determined this dynamical friction force when…

Astrophysics of Galaxies · Physics 2015-06-17 Aaron T. Lee , Steven W. Stahler

The supersonic motion of gravitating objects through a gaseous medium constitutes a classical problem in theoretical astrophysics. Its application covers a broad range of objects and scales from planets up to galaxies. Especially the…

Astrophysics of Galaxies · Physics 2016-04-06 Daniel Thun , Rolf Kuiper , Franziska Schmidt , Wilhelm Kley

The dynamical friction force experienced by a massive gravitating body moving through a gaseous medium is modified by sufficiently strong large-scale magnetic fields. Using linear perturbation theory, we calculate the structure of the wake…

Cosmology and Nongalactic Astrophysics · Physics 2015-06-03 F. J. Sanchez-Salcedo

Recent work has suggested that the net gravitational force acting on a massive and luminous perturber travelling through a gaseous and opaque medium can have same direction as the perturber's motion (an effect sometimes called negative…

Earth and Planetary Astrophysics · Physics 2020-04-30 David A. Velasco-Romero , Frédéric S. Masset

Using time-dependent linear perturbation theory, we evaluate the dynamical friction force on a massive perturber M_p traveling at velocity V through a uniform gaseous medium of density rho_0 and sound speed c_s. This drag force acts in the…

Astrophysics · Physics 2009-10-31 Eve C. Ostriker

Using high-resolution, two-dimensional hydrodynamic simulations, we investigate nonlinear gravitational responses of gas to, and the resulting drag force on, a very massive perturber M_p moving at velocity V_p through a uniform gaseous…

Astrophysics of Galaxies · Physics 2015-05-13 Hyosun Kim , Woong-Tae Kim

When a gravitating point mass moves subsonically through a magnetized and isothermal medium, the dynamical structure of the flow is studied far from the mass using a perturbation analysis. Analytical solutions for the first-order density…

Astrophysics of Galaxies · Physics 2015-06-05 Mohsen Shadmehri , Fazeleh Khajenabi

When a gravitating object moves across a given mass distribution, it creates an overdense wake behind it. Here, we performed an analytical study of the structure of the flow far from object when the flow is isentropic and the object moves…

Astrophysics of Galaxies · Physics 2015-06-04 Fazeleh Khajenabi , Sami Dib

We study the force of dynamical friction acting on a gravitating point mass that travels through an extended, isothermal gas. This force is well established in the hypersonic limit, but remains less understood in the subsonic regime. Using…

Astrophysics of Galaxies · Physics 2015-05-28 Aaron T. Lee , Steven W. Stahler

We consider the gravitational force exerted on a point-like perturber of mass $M$ travelling within a uniform gaseous, opaque medium at constant velocity $V$. The perturber irradiates the surrounding gas with luminosity $L$. The diffusion…

Earth and Planetary Astrophysics · Physics 2017-06-23 Frédéric S. Masset , David A. Velasco Romero

We investigate diffusion in supersonic, turbulent, compressible flows. Supersonic turbulence can be characterized as network of interacting shocks. We consider flows with different rms Mach numbers and where energy necessary to maintain…

Astrophysics · Physics 2009-11-07 Ralf S. Klessen , Doug N. C. Lin

We present an analytic approach to the dynamical friction (DF) acting on a circularly moving point mass perturber in a gaseous medium. We demonstrate that, when the perturber is turned on at $t=0$, steady-state (infinite time perturbation)…

Astrophysics of Galaxies · Physics 2022-04-06 Vincent Desjacques , Adi Nusser , Robin Buehler

Wearless friction is investigated in a simple mechanical model called Frenkel-Kontorova-Tomlinson model. We have introduced this model in [Phys. Rev. B, Vol. 53, 7539 (1996)] where the static friction has already been considered. Here the…

Statistical Mechanics · Physics 2009-10-30 Michael Weiss , Franz-Josef Elmer

In this article, we calculate the friction between two counter-flowing bosonic and fermionic super-fluids. In the limit where the boson-boson and boson-fermion interactions can be treated within the mean-field approximation, we show that…

Quantum Gases · Physics 2015-05-21 F. Chevy

It is shown that the standard effective field theory of non-relativistic superfluids, which includes only the leading order action in derivative expansion, is in general inadequate for studying supersonic processes. Namely, for a proper…

High Energy Physics - Theory · Physics 2020-04-29 Lasha Berezhiani

We study dynamical friction in interacting relativistic systems with arbitrary mean free paths and medium constituent masses. Our novel framework recovers the known limits of ideal gas and ideal fluid when the mean free path goes to…

High Energy Physics - Phenomenology · Physics 2019-08-21 Andrey Katz , Aleksi Kurkela , Alexander Soloviev

We analyze the effect of a gravitational field on the sound modes of superfluids. We derive an instability condition that generalizes the well known Jeans instability of the sound mode in normal fluids. We discuss potential experimental…

High Energy Physics - Theory · Physics 2017-11-08 Itamar Hason , Yaron Oz

We consider the hydrodynamics of supersymmetric fluids. Supersymmetry is broken spontaneously and the low energy spectrum includes a fermionic massless mode, the $\mathit{phonino}$. We use two complementary approaches to describe the…

High Energy Physics - Phenomenology · Physics 2015-06-05 Carlos Hoyos , Boaz Keren-Zur , Yaron Oz

We perform particle-resolved simulations of subsonic and transonic flows past random arrays of spherical particles. The Reynolds number is held at $Re{\approx}300$ to ensure the flow remains in the continuum regime. At low volume fractions,…

Fluid Dynamics · Physics 2022-08-23 Mehdi Khalloufi , Jesse Capecelatro
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