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arxiv.org arXiv
arxiv.org › abs › 2506.06050v2
The impact of Angela Bracco's work on the electric dipole response of nuclei is discussed using three examples of current nuclear structure problems: disentangling different contributions to the decay...
arxiv.org arXiv
arxiv.org › abs › 2203.05010v2
The Standard Model of Particle Physics cannot explain the observed baryon asymmetry of the Universe. This observation is a clear sign of new physics beyond the Standard Model. There have been many rec...
arxiv.org arXiv
arxiv.org › abs › 1303.4033v1
Inelastic neutron scattering measurements demonstrate that the magnetic interactions in antiferromagnetic LaFeAsO are two-dimensional. Spin wave velocities within the Fe layer and the magnitude of the...
arxiv.org arXiv
arxiv.org › abs › 1903.06242v1
Our knowledge of the population of young (age
arxiv.org arXiv
arxiv.org › abs › 2203.07059v2
The baryon asymmetry of the Universe is one of the central motivations to expect physics beyond the Standard Model. In this Snowmass white paper, we review the challenges and opportunities in testing ...
arxiv.org arXiv
arxiv.org › abs › 1111.6652v1
The article covers the physical properties and evolution of single white dwarfs ranging in temperature from 20,000K to 200,000 and higher, the hottest know electron-degenerate stars. After discussing ...
arxiv.org arXiv
arxiv.org › abs › 2203.07506v2
Advances in experimental techniques make it possible to map the high redshift Universe in three dimensions at high fidelity in the near future. This will increase the observed volume by many-fold, whi...
arxiv.org arXiv
arxiv.org › abs › 1209.3722v1
We present a detailed Monte Carlo simulation of the population of the hot branch of the white dwarf luminosity function. We used the most up-to-date stellar evolutionary models and we implemented a fu...
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 › 1209.4977v1
The relatively high abundance of carbon in the hot DO white dwarf RE0503-289 indicates that it is a descendant of a PG1159 star. This is corroborated by the recent detection of the extremely high abun...