1.8k citations
Counting papers with at most 25 authors, so collaboration author lists do not stand in for the people here.
- University of CataniaIT433 papers
- Centre National de la Recherche ScientifiqueFR334 papers
- Institut National de Physique Nucléaire et de Physique des ParticulesFR297 papers
- Istituto Nazionale di Fisica Nucleare, Sezione di CataniaIT243 papers
- Istituto Nazionale di Fisica NucleareIT224 papers
- Istituto Nazionale di Fisica Nucleare, Sezione di NapoliIT203 papers
- Istituto Nazionale di Fisica Nucleare, Sezione di GenovaIT186 papers
- Commissariat à l'Énergie Atomique et aux Énergies AlternativesFR177 papers
- Sapienza University of RomeIT176 papers
- Istituto Nazionale di Fisica Nucleare, Sezione di BolognaIT173 papers
- Istituto Nazionale di Fisica Nucleare, Sezione di Roma IIT169 papers
- University of GenoaIT168 papers
948 papers
KM3-230213A: The Highest-Energy Cosmic Neutrino
Carla Distefano
High-energy neutrinos provide a unique probe of the most extreme non-thermal processes in the Universe. The detection of the ultra-high-energy neutrino event KM3-230213A by the KM3…
Probing collective behaviour of Heavy Quarks through -differential radial flow
Salvatore Plumari, Maria Lucia Sambataro, Santosh K. Das +1
We discuss the -differential radial flow of charmed hadrons within a Langevin dynamics coupled to relativistic Boltzmann transport approach in an event-by-event bas…
Recent applications of the subtracted second RPA method
Danilo Gambacurta, Marcella Grasso
In this review, we discuss the most recent developments and applications of the Subtracted Second RPA (SSRPA), an extension of the Second RPA (SRPA), which overcomes its pathologic…
Resilience of the physicochemical properties of graphene-based materials for applications in harsh radiation environments
Marcilei A. Guazzelli, Saulo G. Alberton, Nemitala Added +16
The development of radiation-tolerant materials capable of maintaining structural, electrical, and thermal stability in extreme, radiation-rich environments remains a critical chal…
Probing nuclear interactions à la Rutherford: Insights on He from scattering
F. Cappuzzello, V. Soukeras, S. Bacca +27
Nuclear interactions play a key role for the stability of atomic nuclei and stellar environments. Successful parametrization and models of these interactions, developed in the last…
Introduction to Higher Order Classical Dynamics: Pais-Uhlenbeck Model and Coupled Oscillators
Cássius Anderson Miquele de Melo, Ivan Francisco de Souza
Most of the laws of Nature involve derivatives up to the second order. Ostrogradski was the first to seek a formulation of the equations of higher-order derivatives. He extended Ha…
Energy-differential measurement of the C(n,p) and C(n,d) reactions at the n_TOF facility at CERN
P. Žugec, N. Colonna, D. Rochman +129
Energy-differential cross section of the C(n,p) and C(n,d) reactions was measured at the neutron time of flight facility n_TOF at CERN. The measur…
Measurement of muon (anti-)neutrino charged-current quasielastic-like cross section using off-axis NuMI beam at ICARUS
ICARUS Collaboration, F. Abd Alrahman, P. Abratenko +176
This paper presents the first neutrino cross-section measurement from the ICARUS detector at Fermilab, using NuMI (Neutrinos at the Main Injector) beam data collected from two beam…
An updated picture of pre-solar history from short-lived radioactive isotopes and inferences on the birth of the Sun
Benjámin Soós, Thomas C. L. Trueman, Andrés Yagüe López +2
We examine the origin of the short-lived radionuclides (SLRs, defined as having half-lives between 0.1 and 100 Ma) present in the early Solar System (ESS) by investigating how pred…
Directed flow of D and B mesons in an electrically and chirally conductive QGP at LHC energies
Ankit Kumar Panda, Pooja, Maria Lucia Sambataro +2
We investigate the directed flow of D and B mesons in the presence of electromagnetic fields incorporating finite electrical and chiral conductivities at LHC energies. The momentum…
Characterization of argon recoils at the keV scale with ReD and ReD+
L. Pandola, P. Agnes, I. Ahmad +43
The ReD experiment measured the ionization yield Qy of argon for nuclear recoils in the 2-10 keV range using a dual-phase Time Projection Chamber irradiated with neutrons from a Cf…
Strontium-84 Enrichments in Presolar Grains Provide First Evidence of p-process Nucleosynthesis in Core-collapse Supernovae
Ishita Pal, Manavi Jadhav, Danielle Z. Shulaker +9
This study reports detection of rare p-process isotopes within presolar grains. Presolar grains are relic dust grains from dying stars. These microscopic dust particles are found i…
Depletion depth measurements of new large area silicon carbide detectors
A. Spatafora, D. Carbone, L. La Fauci +9
The ion beam induced charge technique with proton microprobe is used to characterise newly developed p-n junction large area silicon carbide detectors. They were recently produced…
ESO Expanding Horizon White Paper: Revealing the properties of matter at supranuclear densities with gravitational waves
Tim Dietrich, Tanja Hinderer, Micaela Oertel +40
Understanding dense matter under extreme conditions is one of the most fundamental puzzles in modern physics. Complex interactions give rise to emergent, collective phenomena. Whil…
Elliptic flow of charm quarks produced in the early stage of pA collisions
Gabriele Parisi, Fabrizio Murgana, Vincenzo Greco +1
We investigate the build-up of elliptic flow of charm quarks produced in the early pre-equilibrium stage of high-energy proton--nucleus collisions. The initial stage is modeled wit…
Radiation tolerance tests on key components of the ePIC-dRICH readout card
S. Geminiani, B. R. Achari, N. Agrawal +60
The dual-radiator RICH (dRICH) detector of the ePIC experiment will employ over 300000 SiPM pixels as photosensors, organized into more than 1000 Photon Detection Units. Each PDU i…
Constraining the Synthesis of the Lightest p Nucleus 74Se
A. Tsantiri, A. Spyrou, E. C. Good +42
We provide the first experimental cross section of the reaction to constrain one of the main destruction mechanisms of the p nucleus $^{74}\text…
Search for an eV-scale sterile neutrino with the first six detection units of KM3NeT/ORCA
KM3NeT Collaboration, O. Adriani, A. Albert +285
The existence of an eV-scale sterile neutrino has been proposed to explain several anomalous experimental results obtained over the course of the past 25 years. The first search fo…
Search for planetary-mass ultra-compact binaries using data from the first part of the LIGO--Virgo--KAGRA fourth observing run
The LIGO Scientific Collaboration, the Virgo Collaboration, the KAGRA Collaboration +1765
We present a search for gravitational waves from inspiraling, planetary-mass ultra-compact binaries using data from the first part of the fourth observing run of LIGO, Virgo and KA…
Optimizing the potential of KM3NeT in detecting core-collapse supernovae
KM3NeT Collaboration, O. Adriani, A. Albert +285
Core-collapse supernovae mark the end of life of massive stars. However, despite their importance in astrophysics, their underlying mechanisms remain unclear. Neutrinos that emerge…
Sensitivity to low-mass WIMPs with an improved liquid argon ionization response model within the DarkSide programme
F. Acerbi, P. Adhikari, P. Agnes +294
Dark matter detection experiments using liquid argon rely on a precise characterization of the ionization response to nuclear recoils, especially in the keV energy range relevant f…
Characterization of the ionization response of argon to nuclear recoils at the keV scale with the ReD experiment
P. Agnes, I. Ahmad, S. Albergo +42
In the recent years, argon-based experiments looking for Dark Matter in the Universe have explored the non-standard scenario in which Dark Matter is made by low-mass Weakly Interac…
Probing the QGP through -differential radial flow of heavy quarks
Maria Lucia Sambataro, Salvatore Plumari, Santosh K. Das +1
We introduce the -differential radial flow in the heavy-quark sector. Within an event-by-event Langevin framework, we show that this observable exhibits a strong se…
Unveiling the nature of HE 0107-5240
E. Caffau, M. Steffen, P. Molaro +27
The vast majority of the most iron-poor stars in the Galaxy exhibit a strong carbon enhancement, with C/H ratios only about two orders of magnitude below solar. This unusual chemic…