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200 papers

Gringotts Wizarding Bank is well known as the only financial institution in all of the Wizarding UK as documented in the works recounting the heroics of Harry Potter. The concentration of power and wealth in this single bank needs to be…

General Finance · Quantitative Finance 2017-03-31 Zachary Feinstein

Assuming that gas and dust separate in the interstellar medium (ISM) so that high-density regions, where stars can form, are almost devoid of dust, the amount of metals being removed from the ISM can be significantly reduced (minimized…

Astrophysics of Galaxies · Physics 2021-12-28 Lars Mattsson

An explanation for the political processes leading to the sudden collapse of empires and states would be useful for understanding both historical and contemporary political events. We seek a general description of state collapse spanning…

Physics and Society · Physics 2015-06-16 Daniel John Lawson , Neeraj Oak

Aims: We aim to investigate the consequences of a fast massive stellar remnant - a black hole (BH) or a neutron star (NS) - encountering a planetary system. Methods: We modelled a close encounter between the actual Solar System (SS) and a…

Earth and Planetary Astrophysics · Physics 2021-04-14 Václav Pavlík , Steven N. Shore

We study the impact of regulatory capital constraints on fire sales and financial stability in a large banking system using a mean field game model. In our model banks adjust their holdings of a risky asset via trading strategies with…

Mathematical Finance · Quantitative Finance 2024-06-26 Rüdiger Frey , Theresa Traxler

We consider whether stellar collisions can explain the observed depletion of red giants in the Galactic center. We model the stellar population with two different IMFs: 1) the Miller-Scalo and 2) a much flatter IMF. In the former case,…

Astrophysics of Galaxies · Physics 2010-03-03 M. B. Davies , R. P. Church , D. Malmberg , S. Nzoke , J. Dale , M. Freitag

The initial mass and metallicity of stars both have a strong impact on their fate. Stellar axial rotation also has a strong impact on the structure and evolution of massive stars. In this study, we exploit the large grid of GENEC models,…

Solar and Stellar Astrophysics · Physics 2025-09-08 R. Hirschi , K. Goodman , G. Meynet , A. Maeder , S. Ekström , P. Eggenberger , C. Georgy , Y. Sibony , N. Yusof , S. Martinet , Vishnu Varma , K. Nomoto

Extrasolar planets and belts of debris orbiting post-main-sequence single stars may become unbound as the evolving star loses mass. In multiple star systems, the presence or co-evolution of the additional stars can significantly complicate…

Earth and Planetary Astrophysics · Physics 2015-06-04 Dimitri Veras , Christopher A. Tout

We report a study of a stylized banking cascade model investigating systemic risk caused by counter party failure using liabilities and assets to define banks' balance sheet. In our stylized system, banks can be in two states: normally…

General Finance · Quantitative Finance 2015-06-18 Annika Birch , Tomaso Aste

In the current environment of financial distress, many governments are likely to soon become major holders of financial assets, but the policy debate focuses only on the likelihood and extent of short-term market stabilization. This paper…

General Finance · Quantitative Finance 2016-09-08 Philip Maymin

Stars falling too close to massive black holes in the centres of galaxies can be torn apart by the strong tidal forces. Simulating the subsequent feeding of the black hole with disrupted material has proved challenging because of the range…

High Energy Astrophysical Phenomena · Physics 2024-07-11 Daniel J. Price , David Liptai , Ilya Mandel , Joanna Shepherd , Giuseppe Lodato , Yuri Levin

How massive stars die -- what sort of explosion and remnant each produces -- depends chiefly on the masses of their helium cores and hydrogen envelopes at death. For single stars, stellar winds are the only means of mass loss, and these are…

Astrophysics · Physics 2009-11-07 A. Heger , C. L. Fryer , S. E. Woosley , N. Langer , D. H. Hartmann

Trust lies at the crux of most economic transactions, with credit markets being a notable example. Drawing on insights from the literature on coordination games and network growth, we develop a simple model to clarify how trust breaks down…

General Finance · Quantitative Finance 2009-11-17 Kartik Anand , Prasanna Gai , Matteo Marsili

We study the evolution of the first stars in the universe (Population III) from the early pre-Main Sequence until the end of helium burning in the presence of WIMP dark matter annihilation inside the stellar structure. The two different…

Astrophysics · Physics 2009-11-13 F. Iocco , A. Bressan , E. Ripamonti , R. Schneider , A. Ferrara , P. Marigo

We analyze three sets of infrared star counts in the inner ~0.5 pc of the Galactic Center. We perform statistical tests on the star counts and model in detail the extinction field and the effects of dwarf-giant collisions on the luminosity…

Astrophysics · Physics 2009-10-31 Tal Alexander

For many decades scholars converse how to correctly include the Old Babylonian Empire into the absolute timeline of history. A cuneiform text from the series Enuma Anu Enlil (EAE #20) reports on the destruction of Babylon after a lunar and…

History and Philosophy of Physics · Physics 2020-07-15 Emil Khalisi

Aims. The aim of this work is to study the dynamical effects of the Galaxy on binary star systems with physical and orbital charac- teristics similar to those of the population of known wide binary stars with exoplanets. As secondary goal…

Earth and Planetary Astrophysics · Physics 2017-12-13 J. A. Correa-Otto , R. A. Gil-Hutton

It is shown that the low metallicity tail of the stellar metallicity distribution predicted by simple Outflow models for the Milky Way halo depends sensitively on whether Instantaneous Recycling is adopted or relaxed. In both cases, current…

Astrophysics · Physics 2016-08-30 Nikos Prantzos

We study the influence of gas metallicity, turbulence, and non-equilibrium chemistry on the evolution of the two-phase interstellar medium (warm and cold atomic phases), and thereby constrain the initial conditions for star formation…

Astrophysics of Galaxies · Physics 2015-05-27 S. Walch , R. Wuensch , A. Burkert , S. Glover , A. Whitworth

Astrophysics and planetary science are in crisis. The large missions we need for the next generation of observations cost too much to let us do more than one at a time. This spreads the science out onto a generational timescale, inhibiting…

Instrumentation and Methods for Astrophysics · Physics 2016-09-30 Martin Elvis
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