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During planet formation, numerous small impacting bodies result in cratering impacts on large target bodies. A fraction of the target surface is eroded, while a fraction of the impactor material accretes onto the surface. These fractions…

地球与行星天体物理 · 物理学 2021-06-02 Ryuki Hyodo , Hidenori Genda

Grand Canonical Monte Carlo simulations are used to reproduce the N$_2$/CO ratio ranging between 1.7 $\times$ 10$^{-3}$ and 1.6 $\times$ 10$^{-2}$ observed {\it in situ} in the Jupiter family comet 67P/Churyumov-Gerasimenko by the ROSINA…

地球与行星天体物理 · 物理学 2015-05-27 S. Lectez , J. M. Simon , O. Mousis , S. Picaud , K. Altwegg , M. Rubin , J. M. Salazar

We derive the light profiles for a sample of 25 dwarf elliptical galaxies observed by us with HST/WFPC2 in F555W and F814W. These profiles are fitted with Nuker, R^1/4, exponential, and Sersic laws, and are also used to derive the nuclear…

天体物理学 · 物理学 2009-10-31 M. Stiavelli , B. W. Miller , H. C. Ferguson , J. Mack , B. C. Whitmore , J. Lotz

We present 2-5 $\mu$m spectroscopic observations of the dust coma of 67P/Churyumov-Gerasimenko obtained with the VIRTIS-H instrument onboard Rosetta during two outbursts that occurred on 2015, 13 September 13.6 h UT and 14 September 18.8 h…

Scale invariance property in the global geometry of Earth may lead to a coupled interactive behaviour between various components of the climate system. One of the most interesting correlations exists between spatial statistics of the global…

大气与海洋物理 · 物理学 2016-09-29 Bijan Fallah , Abbas Ali Saberi , Sahar Sodoudi

Based on the non-linear logistic equation we study, in a qualitative and semi-quantitative way, the evolution with energy and saturation of the elastic differential cross-section in $pp(\bar{p}p)$ collisions at high energy. Geometrical…

高能物理 - 唯象学 · 物理学 2010-05-21 P. Brogueira , J. Dias de Deus

Optical properties are required for the correct understanding and modelling of protoplanetary and debris discs. By assuming that comets are the most pristine bodies in the solar system, our goal is to derive optical constants of real…

This work considers the behavior of the height distributions of the equipotential lines in a region confined by two interfaces: a cathode with an irregular interface and a distant flat anode. Both boundaries, which are maintained at…

计算物理 · 物理学 2014-10-08 C. P. de Castro , T. A. de Assis , C. M. C. de Castilho , R. F. S. Andrade

Comets are icy objects that orbitally evolve from the trans-Neptunian region (the Kuiper belt and beyond) into the inner Solar System, where they are heated by solar radiation and become active due to sublimation of water ice. Here we…

地球与行星天体物理 · 物理学 2017-08-23 D. Nesvorny , D. Vokrouhlicky , L. Dones , H. F. Levison , N. Kaib , A. Morbidelli

We show that if comets (or any small icy planetesimals such as Kuiper belt objects) are composed of pebble piles, their internal radiogenic as well as geochemical heating results in considerably different evolutionary outcomes compared to…

地球与行星天体物理 · 物理学 2022-06-03 Uri Malamud , Wolf A. Landeck , Dorothea Bischoff , Christopher Kreuzig , Hagai B. Perets , Bastian Gundlach , Jurgen Blum

We report Spitzer Space Telescope observations of comet 67P/Churyumov-Gerasimenko at 5.5 and 4.3 AU from the Sun, post-aphelion. Comet 67P is the primary target of the European Space Agency's Rosetta mission. The Rosetta spacecraft will…

地球与行星天体物理 · 物理学 2009-11-13 Michael S. Kelley , Diane H. Wooden , Cecilia Tubiana , Hermann Boehnhardt , Charles E. Woodward , David E. Harker

We analyse and compare the clustering of young stars in Chamaeleon I and Taurus. We compute the mean surface-density of companion stars \bar{N} as a function of angular displacement \theta from each star. We then fit \bar{N}(\theta) with…

天体物理学 · 物理学 2009-10-30 P. P. Gladwin , S. Kitsionas , H. M. J. Boffin , A. P. Whitworth

We present the results of a wide-field survey designed to measure the size, inclination, and radial distributions of Kuiper Belt Objects (KBOs). The survey found 86 KBOs in 73 square degrees observed to limiting red magnitude 23.7 using the…

天体物理学 · 物理学 2009-11-06 Chadwick A. Trujillo , David C. Jewitt , Jane X. Luu

We show that the cusp-like structure in the nuclear symmetry energy, a consequence of topology change, visible in the skyrmion lattice description of dense matter is extremely robust. It is present in the Skyrme model -- with the pion field…

核理论 · 物理学 2019-05-15 Xiang-Hai Liu , Yong-Liang Ma , Mannque Rho

We analyse with simple real-space statistics the Virgo consortium's cosmological N-body simulations. Significant clustering rapidly develops well below the initial mean interparticle separation \Lambda_i, where the gravitational force on a…

天体物理学 · 物理学 2009-11-07 Thierry Baertschiger , Michael Joyce , Francesco Sylos Labini

The size distribution in the cold classical Kuiper belt can be approximated by two idealized power laws: one with steep slope for radii R>R* and one with shallow slope for R<R*, where R*~25-50 km. Previous works suggested that the SFD…

地球与行星天体物理 · 物理学 2015-05-27 David Nesvorny , David Vokrouhlicky , William F. Bottke , Keith Noll , Harold F. Levison

In a class of models designed to solve the cosmological constant problem by coupling scalar or tensor classical fields to the space-time curvature, the universal scale factor grows as a power law in the age, $a \propto t^\alpha$, regardless…

天体物理学 · 物理学 2016-08-25 M. Kaplinghat , G. Steigman , I. Tkachev , T. P. Walker

Complexity Theory is highly interdisciplinary, therefore any regularities must hold on all levels of organization, independent on the nature of the system. An open question in science is how complex systems self-organize to produce emergent…

太阳与恒星天体物理 · 物理学 2022-02-07 Travis Herman Butler , Georgi Yordanov Georgiev

Various features of the mass yields in heavy ion collisions are studied. The mass yields are discussed in terms of iterative one dimensional discrete maps. These maps are shown to produce orbits for a monomer or for a nucleus which generate…

核理论 · 物理学 2008-11-26 A. Z. Mekjian , S. J. Lee

Below scales of about 100/h Mpc our universe displays a complex inhomogeneous structure dominated by voids, with clusters of galaxies in sheets and filaments. The coincidence that cosmic expansion appears to start accelerating at the epoch…

宇宙学与河外天体物理 · 物理学 2011-02-11 David L. Wiltshire
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