Zobrazeno 1 - 10
of 7 747
pro vyhledávání: '"P. Perna"'
Autor:
Díaz, Eva, Anadón, Alberto, Olleros-Rodríguez, Pablo, Singh, Harjinder, Damas, Héloïse, Perna, Paolo, Morassi, Martina, Lemaître, Aristide, Hehn, Michel, Gorchon, Jon
Electrical current pulses can be used to manipulate magnetization efficiently via spin-orbit torques (SOTs). Pulse durations as short as a few picoseconds have been used to switch the magnetization of ferromagnetic films, reaching the THz regime. How
Externí odkaz:
http://arxiv.org/abs/2410.00474
Autor:
Antoniali, Fabiana, Conza, Maria Luisa, Conventi, Francesco Alessandro, Cirotto, Francesco, D'Avanzo, Antonio, De Iorio, Agostino, De Iorio, Annalisa, Formicola, Nunzia, Forte, Manuela, Miele, Federica, Perna, Giovanni, Rossi, Biagio, Rossi, Elvira
In this paper, a statistical analysis of the performance of a low insulin index, alkaline and functional diet developed by ANTUR evaluated with machine learning techniques is reported. The sample of patients was checked on a regular basis with a BioI
Externí odkaz:
http://arxiv.org/abs/2409.18221
Autor:
Verdini, Francesco, Melucci, Pierfrancesco, Perna, Stefano, Cariaggi, Francesco, Gaido, Marco, Papi, Sara, Mazurek, Szymon, Kasztelnik, Marek, Bentivogli, Luisa, Bratières, Sébastien, Merialdo, Paolo, Scardapane, Simone
The remarkable performance achieved by Large Language Models (LLM) has driven research efforts to leverage them for a wide range of tasks and input modalities. In speech-to-text (S2T) tasks, the emerging solution consists of projecting the output of
Externí odkaz:
http://arxiv.org/abs/2409.17044
Autor:
Jin, Sunho, Ishiguro, Masateru, Geem, Jooyeon, Naito, Hiroyuki, Takahashi, Jun, Akitaya, Hiroshi, Kuroda, Daisuke, Urakawa, Seitaro, Takagi, Seiko, Oono, Tatsuharu, Sekiguchi, Tomohiko, Perna, Davide, Ieva, Simone, Bach, Yoonsoo P., Imazawa, Ryo, Kawabata, Koji S., Watanabe, Makoto, Jo, Hangbin
Context. (4015) Wilson-Harrington (hereafter, WH) was discovered as a comet in 1949 but has a dynamical property consistent with that of a near-Earth asteroid. Although there is a report that the 1949 activity is associated with an ion tail, the caus
Externí odkaz:
http://arxiv.org/abs/2409.06448
Autor:
Bertola, E., Circosta, C., Ginolfi, M., Mainieri, V., Vignali, C., Rivera, G. Calistro, Ward, S. R., Lopez, I. E., Pensabene, A., Alexander, D. M., Bischetti, M., Brusa, M., Cappi, M., Comastri, A., Contursi, A., Cicone, C., Cresci, G., Dadina, M., D'Amato, Q., Feltre, A., Harrison, C. M., Kakkad, D., Lamperti, I., Lanzuisi, G., Mannucci, F., Marconi, A., Perna, M., Piconcelli, E., Puglisi, A., Ricci, F., Scholtz, J., Tozzi, G., Vietri, G., Zamorani, G., Zappacosta, L.
The energy released by AGN has the potential to heat or remove the gas of the ISM, thus likely impacting the cold molecular gas reservoir of host galaxies at first, with star formation following on longer timescales. Previous works on high-z galaxies
Externí odkaz:
http://arxiv.org/abs/2408.16821
The disks of Active Galactic Nuclei (AGNs) are expected to be populated by numerous stars, either formed in the outer regions of the disk via gravitational instability, or captured from the nearby nuclear star cluster. Regardless of their formation m
Externí odkaz:
http://arxiv.org/abs/2408.16050
Autor:
Pereira-Santaella, Miguel, González-Alfonso, Eduardo, García-Bernete, Ismael, Donnan, Fergus R., Santa-Maria, Miriam G., Goicoechea, Javier R., Lamperti, Isabella, Perna, Michele, Rigopoulou, Dimitra
Publikováno v:
A&A 689, L12 (2024)
We study the 3.4-4.4$\mu$m fundamental rovibrational band of H3+, a key tracer of the ionization of the molecular interstellar medium (ISM), in a sample of 12 local (d< 400 Mpc) ultra/luminous infrared galaxies (U/LIRGs) observed with JWST/NIRSpec. T
Externí odkaz:
http://arxiv.org/abs/2408.14545
Star-forming regions, characterized by dense environments, experience frequent encounters that significantly influence binary systems, leading to their hardening, softening, or ionization. We extend the Hut \& Bahcall formalism to derive an analytica
Externí odkaz:
http://arxiv.org/abs/2407.20416
The spectrum of the quasinormal modes of the gravitational waves emitted during the ringdown phase following the merger of two black holes is of primary importance in gravitational astronomy. However, the spectrum is extremely sensitive to small dist
Externí odkaz:
http://arxiv.org/abs/2407.20144
Autor:
Parlanti, Eleonora, Carniani, Stefano, Venturi, Giacomo, Herrera-Camus, Rodrigo, Arribas, Santiago, Bunker, Andrew J., Charlot, Stephane, D'Eugenio, Francesco, Maiolino, Roberto, Perna, Michele, Übler, Hannah, Böker, Torsten, Cresci, Giovanni, Curti, Mirko, Jones, Gareth C., Lamperti, Isabella, Zamora, Sandra
Galactic outflows driven by star formation or active galactic nuclei are typically formed by multi-phase gas whose temperature spans over 4 orders of magnitude. Probing the different outflow components requires multi-wavelength observations and long
Externí odkaz:
http://arxiv.org/abs/2407.19008