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1 Contributo su Rivista 15262
- 1.1 Articolo in rivista 14358
- 1.2 Recensione in rivista 805
- 1.3 Scheda bibliografica 50
- 1.4 Nota a sentenza 0
- 1.5 Abstract in rivista 37
- 1.6 Traduzione in rivista 12

2 Contributo in Volume 4886

3 Libro 1095
- 3.1 Monografia o trattato scientifico 880
- 3.2 Concordanza 3
- 3.3 Indice 1
- 3.4 Bibliografia 5
- 3.5 Edizione critica 129
- 3.6 Pubblicazione di fonti inedite 24
- 3.7 Commento scientifico 10
- 3.8 Traduzione di libro 43

4 Contributo in Atti di Convegno (Proceeding) 1595
- 4.1 Contributo in Atti di convegno 1359
- 4.2 Abstract in Atti di convegno 187
- 4.3 Poster 49

5 Altro 285
- 5.01 Composizione 10
- 5.02 Disegno 0
- 5.03 Design 0
- 5.04 Performance 12
- 5.05 Esposizione 2
- 5.06 Mostra 17
- 5.07 Manufatto 0
- 5.08 Prototipo d'arte e relativi progetti 0
- 5.09 Cartografia 0
- 5.10 Banca dati 54
- 5.11 Software 4
- 5.12 Altro 186

6 Brevetti 117
- 6.1 Brevetto 117

7 Curatele 559
- 7.1 Curatela 559

8 Altro non ministeriale 288

9 Tesi PhD 932
- 9.1 Tesi PhD 932

Prodotti recenti

Gravitational-wave Constraints on the Equatorial Ellipticity of Millisecond Pulsars

We present a search for continuous gravitational waves from five radio pulsars, comprising three recycled pulsars (PSR J0437-4715, PSR J0711-6830, and PSR J0737-3039A) and two young pulsars: the Crab pulsar (J0534+2200) and the Vela pulsar (J0835-4510). We use data from the third observing run of Advanced LIGO and Virgo combined with data from their first and second observing runs. For the first time, we are able to match (for PSR J0437-4715) or surpass (for PSR J0711-6830) the indirect limit...

Quantum Backaction on kg-Scale Mirrors: Observation of Radiation Pressure Noise in the Advanced Virgo Detector

The quantum radiation pressure and the quantum shot noise in laser-interferometric gravitational wave detectors constitute a macroscopic manifestation of the Heisenberg inequality. If quantum shot noise can be easily observed, the observation of quantum radiation pressure noise has been elusive, so far, due to the technical noise competing with quantum effects. Here, we discuss the evidence of quantum radiation pressure noise in the Advanced Virgo gravitational wave detector. In our experimen...

Constraints on Cosmic Strings Using Data from the Third Advanced LIGO-Virgo Observing Run

We search for gravitational-wave signals produced by cosmic strings in the Advanced LIGO and Virgo full O3 dataset. Search results are presented for gravitational waves produced by cosmic string loop features such as cusps, kinks, and, for the first time, kink-kink collisions. A template-based search for short-duration transient signals does not yield a detection. We also use the stochastic gravitational-wave background energy density upper limits derived from the O3 data to constrain the cos...

Measurements of t t ¯ H Production and the CP Structure of the Yukawa Interaction between the Higgs Boson and Top Quark in the Diphoton Decay Channel

The first observation of the tt¯H process in a single Higgs boson decay channel with the full reconstruction of the final state (H→γγ) is presented, with a significance of 6.6 standard deviations (σ). The CP structure of Higgs boson couplings to fermions is measured, resulting in an exclusion of the pure CP-odd structure of the top Yukawa coupling at 3.2σ. The measurements are based on a sample of proton-proton collisions at a center-of-mass energy s=13 TeV collected by the CMS detector at th...

Observation of Gravitational Waves from the Coalescence of a 2.5–4.5Me Compact Object and a Neutron Star

We report the observation of a coalescing compact binary with component masses 2.5–4.5 Me and 1.2–2.0 Me (all measurements quoted at the 90% credible level). The gravitational-wave signal GW230529_181500 was observed during the fourth observing run of the LIGO–Virgo–KAGRA detector network on 2023 May 29 by the LIGO Livingston observatory. The primary component of the source has a mass less than 5 Me at 99% credibility. We cannot definitively determine from gravitational-wave data alone whethe...

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