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arxiv.org arXiv
arxiv.org › abs › 1411.4413v2
A joint measurement is presented of the branching fractions $B^0_s\toμ^+μ^-$ and $B^0\toμ^+μ^-$ in proton-proton collisions at the LHC by the CMS and LHCb experiments. The data samples were collec...
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arxiv.org arXiv
arxiv.org › abs › 0901.0512v4
A detailed study is presented of the expected performance of the ATLAS detector. The reconstruction of tracks, leptons, photons, missing energy and jets is investigated, together with the performance ...
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arxiv.org arXiv
arxiv.org › abs › 1406.6311v4
This work is on the Physics of the B Factories. Part A of this book contains a brief description of the SLAC and KEK B Factories as well as their detectors, BaBar and Belle, and data taking related is...
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arxiv.org arXiv
arxiv.org › abs › 1710.05839v2
The Advanced LIGO and Advanced Virgo observatories recently discovered gravitational waves from a binary neutron star inspiral. A short gamma-ray burst (GRB) that followed the merger of this binary wa...
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arxiv.org arXiv
arxiv.org › abs › 2202.08970v1
The Nuclotron-base Ion Collider fAcility (NICA) is under construction at the Joint Institute for Nuclear Research (JINR), with commissioning of the facility expected in late 2022. The Multi-Purpose De...
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arxiv.org arXiv
arxiv.org › abs › 2601.07595v3
The discovery of joint sources of high-energy neutrinos and gravitational waves has been a primary target for the LIGO, Virgo, KAGRA, and IceCube observatories. The joint detection of high-energy neut...
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arxiv.org arXiv
arxiv.org › abs › 2512.16347v3
Gravitational waves can be gravitationally lensed by massive objects along their path. Depending on the lens mass and the lens--source geometry, this can lead to the observation of a single distorted ...
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arxiv.org arXiv
arxiv.org › abs › 2510.27022v4
Gravitational-wave detectors can probe the existence of dark matter with exquisite sensitivity. Here, we perform a search for three kinds of dark matter -- dilatons (spin-0), dark photons (spin-1) and...
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arxiv.org arXiv
arxiv.org › abs › 2510.26848v2
We search for gravitational-wave background signals produced by various early Universe processes in the Advanced LIGO O4a dataset, combined with the data from the earlier O1, O2, and O3 (LIGO-Virgo) r...
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arxiv.org arXiv
arxiv.org › abs › 2510.17487v1
The angular distribution of gravitational-wave power from persistent sources may exhibit anisotropies arising from the large-scale structure of the Universe. This motivates directional searches for as...
