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ru.wikipedia.org
ru.wikipedia.org › wiki › ...80%D1%8C%D0%B5%D0%BC
ba.wikipedia.org
ba.wikipedia.org › wiki › ...B5%D1%80%D0%BB%D0%B8
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bing.com › ck › a?!&am...2luLmh0bWw&ntb=1
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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 › 0511168v1
Three brown dwarfs in different evolutionary stages have been observed with the Chandra X-ray Observatory. Combining the new observations with previous studies presented in the literature yields a bro...
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arxiv.org arXiv
arxiv.org › abs › 2502.05515v1
Byzantine agreement (BA) enables all honest nodes in a decentralized network to reach consensus. In the era of emerging quantum technologies, classical cryptography-based BA protocols face inherent se...
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Easy access to plan information anytime anywhere. Get the most out of your coverage. Download our app. Manage your health quickly and securely with the app. Scan the QR code to download. Find a â¦
arxiv.org arXiv
arxiv.org › abs › astro-ph › 0306401v1
We present the first results from a series of Chandra observations carried out with the aim to examine the origin of X-ray emission in main-sequence late B-type stars. We use high spatial resolution X...
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arxiv.org arXiv
arxiv.org › abs › nucl-ex › 9702001v1
The inclusive 12C(p,p') and exclusive 12C(p,p'X) reactions have been studied with a beam energy of 156 MeV and for X = p and alpha. The study focuses on the (p,p'X) reaction mechanism and on the struc...
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arxiv.org arXiv
arxiv.org › abs › 1709.07499v1
The interfacial tension between immiscible liquids is studied as a function of a model linear surfactant length and concentration using coarse grained, dissipative particle dynamics numerical simulati...
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bing.com › ck › a?!&am...Nlcy5jb20v&ntb=1
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arxiv.org arXiv
arxiv.org › abs › 2312.11469v3
The Longest Path Problem is a question of finding the maximum length between pairs of vertices of a graph. In the general case, the problem is NP-complete. However, there is a small collection of grap...
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arxiv.org arXiv
arxiv.org › abs › astro-ph › 9708173v1
By means of numerical methods, we solve the equations of motion for the collapse of a shell of baryonic matter, made of galaxies and substructure falling into the central regions of a cluster of galax...
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Members can get instant access to manage health plan details, request member ID cards, find care and more. Invest in your health and find motivation and support. Plus, you may earn rewards for meeting...
arxiv.org arXiv
arxiv.org › abs › astro-ph › 9804151v1
Evolutionary synthesis models for Tidal Dwarf Galaxies (TDGs) are presented that allow to have varying proportions of young stars formed in the merger-induced starburst and of stars from the merging s...
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arxiv.org arXiv
arxiv.org › abs › 1310.0904v2
The purpose of this note is to give counterexamples to the containment $I^{(3)}\subset I^2$ over the real numbers....
