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The evolution and structure of sub-Neptunes may be strongly influenced by interactions between the outer gaseous envelope of the planet and a surface magma ocean. However, given the wide variety of permissible interior structures of these…

地球与行星天体物理 · 物理学 2025-11-10 Bodie Breza , Matthew C. Nixon , Eliza M. -R. Kempton

We study the stability of gaps opened by a giant planet in a self-gravitating protoplanetary disc. We find a linear instability associated with both the self-gravity of the disc and local vortensity maxima which coincide with gap edges. For…

地球与行星天体物理 · 物理学 2015-05-27 Min-Kai Lin , John Papaloizou

Magma oceans are a common result of the high degree of heating that occurs during planet formation. It is thought that almost all of the large rocky bodies in the Solar System went through at least one magma ocean phase. In this paper, we…

地球与行星天体物理 · 物理学 2018-11-14 Laura Schaefer , Linda T. Elkins-Tanton

We study the Mott transition of a mixed Bose-Fermi system of ultracold atoms in an optical lattice, where the number of (spinless) fermions and bosons adds up to one atom per lattice, n_F+n_B=1. For weak interactions, a Fermi surface…

量子气体 · 物理学 2013-05-30 Ehud Altman , Eugene Demler , Achim Rosch

It is widely accepted that Titan and the mid-sized regular satellites around Saturn were formed in the circum-Saturn disk. Thus, if these mid-sized satellites were simply accreted by collisions of similar ice-rock satellitesimals in the…

地球与行星天体物理 · 物理学 2015-05-28 Yasuhito Sekine , Hidenori Genda

Magnetic flux rope (MFR) is the core structure of the greatest eruptions, i.e., the coronal mass ejections (CMEs), on the Sun, and magnetic clouds are post-eruption MFRs in interplanetary space. There is a strong debate about whether or not…

太阳与恒星天体物理 · 物理学 2018-03-06 Yuming Wang , Chenglong Shen , Rui Liu , Jiajia Liu , Jingnan Guo , Xiaolei Li , Mengjiao Xu , Qiang Hu , Tielong Zhang

The mass assembly of galaxies leaves imprints in their outskirts, such as shells and tidal tails. The frequency and properties of such fine structures depend on the main acting mechanisms - secular evolution, minor or major mergers - and on…

Most earthquake energy release arises during fault slip many kilometers below the Earth's surface. Understanding earthquakes and their hazard requires mapping the geometry and distribution of this slip. Such finite-fault maps are typically…

地球物理 · 物理学 2024-06-21 Anthony Lomax

We review the current literature on the formation of Coherent Structures (CoSs) in strongly turbulent 3D magnetized plasmas. CoSs (Current Sheets (CS), magnetic filaments, large amplitude magnetic disturbances, vortices, and shocklets)…

高能天体物理现象 · 物理学 2023-05-03 Loukas Vlahos , Heinz Isliker

We study the dynamics of galaxy mergers, with emphasis on the gas feeding of nuclear regions, using a suite of hydrodynamical simulations of galaxy encounters. The high spatial and temporal resolution of the simulations allows us to not…

星系天体物理 · 物理学 2017-01-25 Pedro R. Capelo , Massimo Dotti

We investigate prestellar core formation and accretion based on three-dimensional hydrodynamic simulations. Our simulations represent local $\sim 1$pc regions within giant molecular clouds where a supersonic turbulent flow converges,…

太阳与恒星天体物理 · 物理学 2015-06-10 Munan Gong , Eve C. Ostriker

The phenomenon of Mott insulation involves the localization of itinerant electrons due to strong local repulsion. Upon doping, a pseudogap (PG) phase emerges - marked by selective gapping of the Fermi surface without conventional symmetry…

Interfacial fluctuation effects occuring at wedge and cone filling transitions are investigated and shown to exhibit very different characteristics. For both geometries we show how the conditions for observing critical (continuous) filling…

软凝聚态物质 · 物理学 2009-10-31 A. O. Parry , A. J. Wood , C. Rascon

We study an active-region dextral filament which was composed of two branches separated in height by about 13 Mm. This "double-decker" configuration sustained for days before the upper branch erupted with a GOES-class M1.0 flare on 2010…

太阳与恒星天体物理 · 物理学 2012-08-16 Rui Liu , Bernhard Kliem , Tibor Török , Chang Liu , Viacheslav S. Titov , Roberto Lionello , Jon A. Linker , Haimin Wang

Mean-motion resonances are expected to frequently arise at the inner edges of protoplanetary disks, where planet-disk interactions facilitate large-scale orbital convergence. Under certain conditions, however, the same dissipative forces…

地球与行星天体物理 · 物理学 2026-04-29 Konstantin Batygin , Ian R. Brunton , Alessandro Morbidelli

Volcanic eruptions are driven by decompression-induced vesiculation of supersaturated volatile components in magma. The initial phase of this phenomenon has long been described as nucleation and growth. Recently, it was proposed that…

地球物理 · 物理学 2025-10-09 Mizuki Nishiwaki

Using a novel high-performance computing implementation of a nonlinear continuum damage breakage model, we explore interactions between 3D co-seismic off-fault damage, seismic radiation, and rupture dynamics. Our simulations demonstrate…

地球物理 · 物理学 2025-03-28 Zihua Niu , Alice-Agnes Gabriel , Yehuda Ben-Zion

We investigate the fragmentation process of solid materials with crystalline and amorphous phases using the discrete element method. Damage initiates inside spherical samples above the contact zone in a region where the circumferential…

Presented in this thesis are a set of projects which lie at the intersection between strong correlations and topological phases of matter. The first of these projects is a treatment of an infinite dimensional generalization of the SSH model…

强关联电子 · 物理学 2022-12-12 Patrick J. Wong

Geological applications of phase-field methods for fracture are notably scarce. This work conducts a numerical examination of the applicability of standard phase-field models in reproducing jointing within sedimentary layers. We explore how…

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