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We report the statistical properties of stars and brown dwarfs obtained from four radiation hydrodynamical simulations of star cluster formation that resolve masses down to the opacity limit for fragmentation. The calculations are identical…

太阳与恒星天体物理 · 物理学 2014-05-23 Matthew R. Bate

We examine whether the accretion of dark matter onto neutron stars could ever have any visible external effects. Captured dark matter which subsequently annihilates will heat the neutron stars, although it seems the effect will be too small…

星系天体物理 · 物理学 2015-03-14 Arnaud de Lavallaz , Malcolm Fairbairn

Various past theoretical considerations and observational efforts suggest the presence of a population of stellar-mass black holes in the innermost parsec of the Galactic centre. In this Letter, we investigate the impact of these black…

星系天体物理 · 物理学 2025-03-21 Jaroslav Haas , Pavel Kroupa , Ladislav Šubr , Myank Singhal

The first stars fundamentally transformed the early Universe through their production of energetic radiation and the first heavy chemical elements. The impact on cosmic evolution sensitively depends on their initial mass function (IMF),…

天体物理学 · 物理学 2009-11-13 Anna Frebel , Jarrett L. Johnson , Volker Bromm

Milky Way-mass galaxies in the FIRE-2 simulations demonstrate two main modes of star formation. At high redshifts star formation occurs in a series of short and intense bursts, while at low redshifts star formation proceeds at a steady rate…

We examine the importance of secular stellar mass loss for fueling ongoing star formation in disk galaxies during the late stages of their evolution. For a galaxy of a given stellar mass, we calculate the total mass loss rate of its entire…

星系天体物理 · 物理学 2015-03-17 Samuel N. Leitner , Andrey V. Kravtsov

Chemical evidence indicates that an appreciable fraction of Sun-like stars have engulfed rocky planets during their main-sequence lifetimes. We investigate whether the tidal evolution and destruction of ultra-short-period planets (USPs) can…

地球与行星天体物理 · 物理学 2024-10-17 Christopher E. O'Connor , Dong Lai

We explore the elemental abundance features of metal-rich disk stars, highlighting the comparisons made with those of the recently revealed Galactic bulge stars. A similarity between two of the comparisons leads to a new theoretical picture…

天体物理学 · 物理学 2009-11-13 Takuji Tsujimoto

We assume that an agent's rate of consumption is {\it ratcheted}; that is, it forms a non-decreasing process. Given the rate of consumption, we act as financial advisers and find the optimal investment strategy for the agent who wishes to…

风险管理 · 定量金融 2008-12-10 Erhan Bayraktar , Virginia R. Young

This paper casts within a unified economic framework some key challenges for the global economic order: de-globalization; the rising impracticability of global cooperation; and the increasingly confrontational nature of Great Power…

综合经济学 · 经济学 2023-10-30 Shiro Armstrong , Danny Quah

Two different model-independent mapping techniques have been applied to OSSE, SMM, TGRS and balloon data and reveal a feature in the 0.511 MeV electron-positron annihilation radiation pattern of our galaxy centered roughly at l=-2 deg. and…

天体物理学 · 物理学 2009-10-30 C. D. Dermer , J. G. Skibo

We calculate the extent to which collisionless dark matter impacts the stability of supermassive stars $(M\gtrsim10^4\,M_\odot)$. We find that, depending on the star's mass, a dark matter content in excess of ${\sim}1\%$ by mass throughout…

宇宙学与河外天体物理 · 物理学 2024-10-24 Kyle S. Kehrer , George M. Fuller

In this note, we explicitly solve the problem of maximizing utility of consumption (until the minimum of bankruptcy and the time of death) with a constraint on the probability of lifetime ruin, which can be interpreted as a risk measure on…

投资组合管理 · 定量金融 2012-06-28 Erhan Bayraktar , Virginia R. Young

The chemical abundances measured in stars of the Galactic bulge offer an unique opportunity to test galaxy formation models as well as impose strong constraints on the history of star formation and stellar nucleosynthesis. The aims of this…

星系天体物理 · 物理学 2015-05-20 Gabriele Cescutti , Francesca Matteucci

We calculate the stellar mass-metallicity relation at five epochs ranging to z~2.3. We quantify evolution in the shape of the mass-metallicity relation as a function of redshift; the mass-metallicity relation flattens at late times. There…

宇宙学与河外天体物理 · 物理学 2015-06-15 H. Jabran Zahid , Margaret Geller , Lisa Kewley , Ho Seong Hwang , Daniel Fabricant , Michael Kurtz

We present simulations of the accretion of a massive planet or brown dwarf by an AGB star. In our scenario, close planets will be engulfed by the star, spiral-in and be dissipated in the ``accretion region'' located at the bottom of the…

天体物理学 · 物理学 2007-05-23 Lionel Siess , Mario Livio

In recent observations of extremely metal-poor low-mass starburst galaxies, almost solar Fe/O ratios are reported, despite N/O ratios consistent with the low metallicity. We investigate if the peculiar Fe/O ratios can be a distinctive…

星系天体物理 · 物理学 2022-07-06 S. Goswami , L. Silva , A. Bressan , V. Grisoni , G. Costa , P. Marigo , G. L. Granato , A. Lapi , M. Spera

We propose a game-theoretic framework to study the outcomes of packetized payments, a cross-ledger transaction protocol, with strategic and possibly malicious agents. We derive the transaction failure rate and demonstrate that without…

计算机科学与博弈论 · 计算机科学 2021-12-14 Alevtina Dubovitskaya , Damien Ackerer , Jiahua Xu

We investigate the mass-metallicity relationship of star forming galaxies by analysing the absorption line spectra of $\sim$200,000 galaxies in the Sloan Digital Sky Survey. The galaxy spectra are stacked in bins of stellar mass and a…

星系天体物理 · 物理学 2023-06-07 Eva Sextl , Rolf-Peter Kudritzki , H. Jabran Zahid , I-Ting Ho

This paper empirically analyzes a dataset published by the European Banking Authority. Our main aim was to study how the Leverage Ratio is affected by adverse financial scenarios. This was be followed by observing how Leverage Ratio…

风险管理 · 定量金融 2022-06-27 Jatin Dhingra , Kartikeya Singh , Siddhartha P. Chakrabarty
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