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- The University of TokyoJP344 papers
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- University of New MexicoUS288 papers
- Joint Institute for Nuclear ResearchRU287 papers
- Kyoto UniversityJP283 papers
- The Ohio State UniversityUS281 papers
- Centre National de la Recherche ScientifiqueFR280 papers
- University College LondonGB275 papers
- University of PisaIT274 papers
- University of GenevaCH271 papers
- Institute for High Energy PhysicsES265 papers
- Yale UniversityUS265 papers
46 papers · 1 filter
Leptonic and semi-leptonic neutrino interactions with muons in the proto-neutron star cooling
Ken'ichi Sugiura, Shun Furusawa, Kohsuke Sumiyoshi +1
It is known that muons are scarce just after the birth of a proto-neutron star via a supernova explosion but get more abundant as the proto-neutron star cools via neutrino emission…
Online Phase Reconstruction via DNN-based Phase Differences Estimation
Yoshiki Masuyama, Kohei Yatabe, Kento Nagatomo +1
This paper presents a two-stage online phase reconstruction framework using causal deep neural networks (DNNs). Phase reconstruction is a task of recovering phase of the short-time…
Band-folding-driven high tunnel magnetoresistance ratios in (111)-oriented junctions with SrTiO barriers
Keisuke Masuda, Hiroyoshi Itoh, Yoshiaki Sonobe +3
We theoretically study the tunnel magnetoresistance (TMR) effect in (111)-oriented magnetic tunnel junctions (MTJs) with SrTiO barriers, Co/SrTiO/Co(111) and Ni/SrTiO$_…
The signaling dimension of physical systems
Michele Dall'Arno
The signaling dimension of a physical system is the minimum dimension of a classical channel that can reproduce the set of input-output correlations attainable by the given system.…
Integrable delay-difference and delay-differential analogues of the KdV, Boussinesq, and KP equations
Kenta Nakata
Delay-difference and delay-differential analogues of the KdV and Boussinesq (BSQ) equations are presented. Each of them has the N-soliton solution and reduces to an already known s…
Evidence for extended gaseous reservoirs around AGN at cosmic noon from ALMA CO(3-2) observations
G. C. Jones, R. Maiolino, C. Circosta +3
Gaseous outflows are key phenomena in the evolution of galaxies, as they affect star formation (either positively or negatively), eject gas from the core or disk, and directly caus…