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- Istituto Nazionale di Fisica Nucleare, Laboratori Nazionali del Gran SassoIT850 papers
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- Sapienza University of RomeIT442 papers
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- Istituto Nazionale di Fisica Nucleare, Sezione di Roma IIT412 papers
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- University of Naples Federico IIIT394 papers
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175 papers · 1 filter
Sensitivity of future liquid argon dark matter search experiments to core-collapse supernova neutrinos
P. Agnes, S. Albergo, I. F. M. Albuquerque +273
Future liquid-argon DarkSide-20k and ARGO detectors, designed for direct dark matter search, will be sensitive also to core-collapse supernova neutrinos, via coherent elastic neutr…
Results on Se with CUPID-0 Phase I
L Pagnanini, O Azzolini, J W Beeman +41
The nucleus is an extraordinarily complex object where fundamental forces are at work. The solution of this many-body problem has challenged physicists for decades: several models…
Structure-Constrained Process Graphs for the Process Semantics of Regular Expressions
Clemens Grabmayer
Milner (1984) introduced a process semantics for regular expressions as process graphs. Unlike for the language semantics, where every regular (that is, DFA-accepted) language is t…
Search for double -decay modes of Zn using purified zinc
F. Bellini, M. Beretta, L. Cardani +27
The production of ultra-pure raw material is a crucial step to ensure the required background level in rare event searches. In this work, we establish an innovative technique devel…
Discovery probabilities of Majorana neutrinos based on cosmological data
M. Agostini, G. Benato, S. Dell'Oro +2
We discuss the impact of the cosmological measurements on the predictions of the Majorana mass of the neutrinos, the parameter probed by neutrinoless double-beta decay experiments.…
Diving below the spin-down limit: Constraints on gravitational waves from the energetic young pulsar PSR J0537-6910
The LIGO Scientific Collaboration, the Virgo Collaboration, the KAGRA Collaboration +1589
We present a search for continuous gravitational-wave signals from the young, energetic X-ray pulsar PSR J0537-6910 using data from the second and third observing runs of LIGO and…