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ba.wikipedia.org
ba.wikipedia.org › wiki › ...83%D0%BB%D0%BB%D0%B0
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 ...
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...
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...
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...
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...
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...
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...
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...
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...
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....