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arxiv.org arXiv
arxiv.org › abs › 2505.16286v2
Quantum simulation has emerged as a powerful framework for investigating complex many - body phenomena. A key requirement for emulating these dynamics is the realization of fully controllable quantum ...
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arxiv.org arXiv
arxiv.org › abs › astro-ph › 0510198v1
Many of the known extrasolar planets are ``hot Jupiters,'' giant planets with orbital periods of just a few days. We use the observed distribution of hot Jupiters to constrain the location of the ``in...
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arxiv.org arXiv
arxiv.org › abs › 2203.16152v1
Non-Uniform Rational B-Spline (NURBS) surfaces are commonly used within Computer-Aided Design (CAD) tools to represent geometric objects. When using isogeometric analysis (IGA), it is possible to use ...
arxiv.org arXiv
arxiv.org › abs › astro-ph › 0511583v2
In late August 2005, 80 researchers from more than 15 countries convened for a 4-day conference entitled ``The Tenth Anniversary of 51 Peg b: Status and Prospects for Hot Jupiter Studies''. The meetin...
arxiv.org arXiv
arxiv.org › abs › 0907.1795v1
What is long-baseline optical/IR stellar interferometry? A few years ago, many astronomers might not have been able to answer that question properly. This is today hopefully not the case anymore, beca...
arxiv.org arXiv
arxiv.org › abs › 2209.14257v1
Am stars are often components of short-period binary systems, where tidal interactions would result in low rotational velocities and help to develop the chemical peculiarities observed. However, the o...
arxiv.org arXiv
arxiv.org › abs › astro-ph › 0402650v1
We have conducted a study of optical and HI properties of spiral galaxies (size, luminosity, H-alpha flux distribution, circular velocity, HI gas mass) to explore the role of gas stripping as a driver...
arxiv.org arXiv
arxiv.org › abs › astro-ph › 9710142v1
A definite prediction from recent N-body/hydro simulations of the structure formation of the universe is the presence of a diffuse intergalactic medium (IGM) in a temperature range of 10^5 - 10^7 K. T...
arxiv.org arXiv
arxiv.org › abs › astro-ph › 0610102v2
There is currently debate over whether the dust content of planetary systems is stochastically regenerated or originates in planetesimal belts evolving in steady state. In this paper a simple model fo...
arxiv.org arXiv
arxiv.org › abs › 1308.2447v2
We started a new project which aims to find compact hot subdwarf binaries at low Galactic latitudes. Targets are selected from several photometric surveys and a spectroscopic follow-up campaign to fin...