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During a giant eruption of a very massive star in the binary system, the companion star can accrete a large amount of mass that can change its properties and potentially its subsequent evolution. The effect depends on the companion mass,…

太阳与恒星天体物理 · 物理学 2025-09-15 Bhawna Mukhija , Amit Kashi

The purpose of this review is to discuss the advantages and problems of near-infrared surveys in observing pulsating stars in the Milky Way. One of the advantages of near-infrared surveys, when compared to optical counterparts, is that the…

太阳与恒星天体物理 · 物理学 2017-09-13 Noriyuki Matsunaga

As a star evolves off the Main Sequence, it endures major structural changes that are capable of determining the fate of the planets orbiting it. Throughout its evolution along the Red Giant Branch, the star increases its radius by two…

地球与行星天体物理 · 物理学 2015-05-27 Eva Villaver

Cascading failures, such as bankruptcies and defaults, pose a serious threat for the resilience of the global financial system. Indeed, because of the complex investment and cross-holding relations within the system, failures can occur as a…

系统与控制 · 电气工程与系统科学 2025-01-22 Leonardo Stella , Dario Bauso , Franco Blanchini , Patrizio Colaneri

Stability of economic model predictive control can be proven under the assumption that a strict dissipativity condition holds. This assumption has a clear interpretation in terms of the so-called rotated stage cost, which must have its…

最优化与控制 · 数学 2026-03-10 Mario Zanon

This is the second in a series of papers presenting the results of fully general relativistic simulations of stellar tidal disruptions in which the stars' initial states are realistic main-sequence models. In the first paper (Paper I), we…

高能天体物理现象 · 物理学 2020-12-02 Taeho Ryu , Julian Krolik , Tsvi Piran , Scott C. Noble

Motivated by the observed bottom-light initial mass function (IMF) in faint dwarfs, we study how a metallicity-dependent IMF affects the feedback budget and observables of an ultra-faint dwarf galaxy. We model the evolution of a low-mass…

Ram pressure stripping of satellite galaxies is thought to be a ubiquitous process in galaxy clusters, and a growing number of observations reveal satellites at different stages of stripping. However, in order to determine the fate of any…

We investigate the imaginary world of Kalgash, a planetary system based on the novel "Nightfall" (Asimov & Silverberg, 1991). The system consists of a planet, a moon and an astonishing six suns. The six stars cause the wider universe to be…

科普物理 · 物理学 2014-08-28 Smaran Deshmukh , Jayant Murthy

When a planet falls onto the surface of its host star, the added high-metallicity material does not remain in the surface layers, as often assumed, but is diluted into the interior through fingering (thermohaline) convection. Until now,…

太阳与恒星天体物理 · 物理学 2010-11-16 Pascale Garaud

Stars orbiting supermassive black holes can generate recurring accretion flares in repeating partial tidal disruption events (TDEs). Here we develop an efficient formalism for analyzing the time-dependent response of a star to the removal…

高能天体物理现象 · 物理学 2025-05-20 Ananya Bandopadhyay , Eric R. Coughlin , C. J. Nixon

This paper investigates the possible use of space probes to explore the Milky Way, as a means both of finding life elsewhere in the Galaxy and as finding an answer to the Fermi paradox. I simulate exploration of the Galaxy by first…

天体物理学 · 物理学 2009-11-13 Rasmus Bjoerk

Rapid mass transfer in a binary system can drive the accreting star out of thermal equilibrium, causing it to expand. This can lead to a contact system, strong mass loss from the system and possibly merging of the two stars. In low…

天体物理学 · 物理学 2008-11-26 S. E. de Mink , M. Cottaar , O. R. Pols

In this work we explore the effects of adopting an initial mass function (IMF) variable in time on the chemical evolution of the Galaxy. In order to do that we adopt a chemical evolution model which assumes two main infall episodes for the…

天体物理学 · 物理学 2016-01-27 Cristina Chiappini , Francesca Matteucci

The formation processes that led to the current Galactic stellar halo are still under debate. Previous studies have provided evidence for different stellar populations in terms of elemental abundances and kinematics, pointing to different…

The number of objects in orbit is rapidly increasing, primarily driven by the launch of megaconstellations, an approach to satellite constellation design that involves large numbers of satellites paired with their rapid launch and disposal.…

地球与行星天体物理 · 物理学 2026-01-09 Sarah Thiele , Skye R. Heiland , Aaron C. Boley , Samantha M. Lawler

Civilization cannot sustain an exponential growth for long time even when neglecting numerous laws of physics! In this paper, we examine what are fundamental obstacles to long term survival of a civilization and its possibility to colonize…

科普物理 · 物理学 2007-11-13 Y. Dutil , S. Dumas

A recent paper by Bhatia, Chin, Mani, and Mossel (2026) defined stochastic processes aimed at modeling the game of War for {\em two players} with $n$ cards. That paper showed that these models, assuming uniform random decks, are equivalent…

概率论 · 数学 2026-01-29 Axel Adjei , Neil Krishnan , Elchanan Mossel

Society's drive toward ever faster socio-technical systems, means that there is an urgent need to understand the threat from 'black swan' extreme events that might emerge. On 6 May 2010, it took just five minutes for a spontaneous mix of…

物理与社会 · 物理学 2012-02-08 Neil Johnson , Guannan Zhao , Eric Hunsader , Jing Meng , Amith Ravindar , Spencer Carran , Brian Tivnan

A long-lived civilization will inevitably have to migrate towards a nearby star as its home star runs out of nuclear fuel. One way to achieve such a migration is by transforming its star into a stellar engine, and to control its motion in…

高能天体物理现象 · 物理学 2024-11-11 Clément Vidal