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Finite-energy particles in free fall can collide with diverging center-of-mass energy near rapidly rotating black holes. What are the most salient observational signatures of this remarkable geometric effect? Here we revisit the problem…

广义相对论与量子宇宙学 · 物理学 2025-06-09 Delilah E. A. Gates , Shahar Hadar

In the modern Universe the existence of various forms of scalar fields is supposed. On the one hand these fields can explain recently discovered positive $\Lambda$-term(see e.g. Ref. \cite{ref:Sahni}), on the other hand its form cluster…

天体物理学 · 物理学 2007-05-23 V. Folomeev , V. Gurovich , R. Usupov

Over the past decade, there has been a significant increase in the reporting of extensive and luminous star-forming regions associated with explosive outflows. Nevertheless, there is still a lack of understanding of the possible physical…

In the three-body problem with positive energy, solutions which avoid triple collision have the property that the size of the triangle formed by the bodies tends to infinity as $t\rightarrow \pm\infty$. Furthermore, the triangles have…

动力系统 · 数学 2026-02-20 Richard Moeckel

We investigate the melt production of planetary impacts as a function of planet size ($R/R_\mathrm{Earth}$=0.1-1.5), impactor size ($L$=1-1000 km), and core size ratio ($R_\mathrm{core}/R$=0.2-0.8) using a combination of parameterized…

地球与行星天体物理 · 物理学 2025-06-24 Lukas Manske , Thomas Ruedas , Ana-Catalina Plesa , Philipp Baumeister , Nicola Tosi , Natalia Artemieva , Kai Wünnemann

Drop impact experiments allow the modelling of a wide variety of natural processes, from raindrop impacts to planetary impact craters. In particular, interpreting the consequences of planetary impacts requires an accurate description of the…

流体动力学 · 物理学 2023-05-08 Victor Lherm , Renaud Deguen

Spin off events and impacts can eject boulders from an asteroid surface and rubble pile asteroids can accumulate from debris following a collision between large asteroids. These processes produce a population of gravitational bound objects…

We develop an original apparatus of the granular impact experiment by which the incident angle of the solid projectile and inclination angle of the target granular layer can be systematically varied. Whereas most of the natural cratering…

地球与行星天体物理 · 物理学 2020-02-19 Shinta Takizawa , Ryusei Yamaguchi , Hiroaki Katsuragi

Several stars show deep transits consistent with discs of roughly 1 Solar radius seen at moderate inclinations, likely surrounding planets on eccentric orbits. We show that this configuration arises naturally as a result of planet-planet…

地球与行星天体物理 · 物理学 2024-05-16 Alexander J. Mustill , Melvyn B. Davies , Matthew A. Kenworthy

In this paper, we extend our Smooth Particle Hydrodynamics (SPH) impact code to include the effect of porosity at a sub-resolution scale by adapting the so-called $P-alpha$ model. Many small bodies in the different populations of asteroids…

天体物理学 · 物理学 2009-11-13 M. Jutzi , W. Benz , P. Michel

Planet--Planet scattering is an efficient and robust dynamical mechanism for producing eccentric exoplanets. Coupled to tidal interactions with the central star, it can also explain close--in giant planets on circularized and potentially…

地球与行星天体物理 · 物理学 2019-05-29 F. Marzari , M. Nagasawa

We present a rigorous study of the classical scattering for anytwo-body inter-particle potential of the form $v(r)=g/r^\gamma$, with$\gamma\textgreater{}0$, for repulsive ($g\textgreater{}0$) and attractive ($g\textless{}0$)interactions. We…

统计力学 · 物理学 2016-01-05 D Chiron , B Marcos

We apply a theoretical approach, originally introduced to describe aeolian ripples formation in sandy deserts, to the study of surface instability in ion sputtered surfaces. The two phenomena are distinct by several orders of magnitudes and…

无序系统与神经网络 · 物理学 2015-06-24 T. Aste , U. Valbusa

We investigate the patterns observed in ejecta curtain induced by hypervelocity impact (2-6 km/s) with a variety of the size and shape of target particles. We characterize the patterns by an angle, defined as the ratio of the characteristic…

地球与行星天体物理 · 物理学 2019-12-20 Toshihiko Kadono , Ayako I. Suzuki , Rintaro Matsumura , Junta Naka , Ryo Suetsugu , Kosuke Kurosawa , Sunao Hasegawa

We develop a microscopic theory of the scattering, transmission, and sticking of 4He atoms impinging on a superfluid 4He slab at near normal incidence, and inelastic neutron scattering from the slab. The theory includes coupling between…

凝聚态物理 · 物理学 2009-10-31 C. E. Campbell , E. Krotscheck , M. Saarela

When a jet of gas impinges vertically on a granular bed and forms a crater, the grains may be moved by several different mechanisms: viscous erosion, diffused gas eruption, bearing capacity failure, and/or diffusion-driven shearing. The…

软凝聚态物质 · 物理学 2021-04-13 Philip T. Metzger , Robert C. Latta , Jason M. Schuler , Christopher D. Immer

Crystal lattice structure is present in stellar compact objects, such as white dwarf stars and in the crust of neutron stars. These structures can be described by a body-centered cubic crystal, which is formed by ions due to Coulombian…

太阳与恒星天体物理 · 物理学 2022-12-20 S. V. C. Ramalho , S. B. Duarte , G. S. Vicente

Fractals are defined as geometric shapes that exhibit symmetry of scale. This simply implies that fractal is a shape that it would still look the same even if somebody could zoom in on one of its parts an infinite number of times. This…

空间物理 · 物理学 2015-05-29 Ioannis Haranas , Ioannis Gkigkitzis , Athanasios Alexiou

The studies of crystal collimation in the experiments at Relativistic Heavy Ion Collider and Tevatron and in computer simulations reveal strong coherent effects observed in a very broad angular range. Our theory explains the effects by…

加速器物理 · 物理学 2007-05-23 V. M. Biryukov

As accretion in protoplanetary disks is enabled by turbulent viscosity, the border between active and inactive (dead) zones constitutes a location where there is an abrupt change in the accretion flow. The gas accumulation that ensues…

地球与行星天体物理 · 物理学 2009-11-13 W. Lyra , A. Johansen , A. Zsom , H. Klahr , N. Piskunov