Zobrazeno 1 - 10
of 1 113
pro vyhledávání: '"Mignone, P"'
Autor:
Bugli, M., Lopresti, E. F., Figueiredo, E., Mignone, A., Cerutti, B., Mattia, G., Del Zanna, L., Bodo, G., Berta, V.
Relativistic magnetic reconnection is one of the most fundamental mechanisms considered responsible for the acceleration of relativistic particles in astrophysical jets and magnetospheres of compact objects. Understanding the properties of the dissip
Externí odkaz:
http://arxiv.org/abs/2410.20924
Recent studies showed that observations of line emission from shocks in YSO jets require a substantial amount of ionization of the pre-shock matter. Photoionization from X-ray emitted close to the central source may be responsible for the initial ion
Externí odkaz:
http://arxiv.org/abs/2410.11692
Autor:
Ziampras, Alexandros, Sudarshan, Prakruti, Dullemond, Cornelis P., Flock, Mario, Berta, Vittoria, Nelson, Richard P., Mignone, Andrea
Protoplanetary disks exhibit a rich variety of substructure in millimeter continuum emission, often attributed to unseen planets. As these planets carve gaps in the gas, dust particles can accumulate in the resulting pressure bumps, forming bright fe
Externí odkaz:
http://arxiv.org/abs/2409.15420
Instabilities in relativistic magnetized jets are thought to be deeply connected to their energy dissipation properties and to the consequent acceleration of the non-thermal emitting relativistic particles. Instabilities lead to the development of sm
Externí odkaz:
http://arxiv.org/abs/2407.15477
Autor:
Mignone, Andrea, Berta, Vittoria, Rossazza, Marco, Bugli, Matteo, Mattia, Giancarlo, Del Zanna, Luca, Pareschi, Lorenzo
We present a finite-volume, genuinely 4th-order accurate numerical method for solving the equations of resistive relativistic magnetohydrodynamics (Res-RMHD) in Cartesian coordinates. In our formulation, the magnetic field is evolved in time in terms
Externí odkaz:
http://arxiv.org/abs/2407.08519
The gut microbiome, crucial for human health, presents challenges in analyzing its complex metaomic data due to high dimensionality and sparsity. Traditional methods struggle to capture its intricate relationships. We investigate graph neural network
Externí odkaz:
http://arxiv.org/abs/2407.00142
Autor:
Follo, U., Gioachin, G., Ferrero, C., Mandurrino, M., Bregant, M., Bufalino, S., Carnesecchi, F., Cavazza, D., Colocci, M., Corradino, T., Rolo, M. Da Rocha, Di Nicolantonio, G., Durando, S., Margutti, G., Mignone, M., Nania, R., Pancheri, L., Rivetti, A., Sabiu, B., de Souza, G. G. A., Strazzi, S., Wheadon, R.
In this paper we report on a set of characterisations carried out on the first monolithic LGAD prototype integrated in a customised 110 nm CMOS process having a depleted active volume thickness of 48 $\mu$m. This prototype is formed by a pixel array
Externí odkaz:
http://arxiv.org/abs/2406.19906
Autor:
Adams Jr., James H., Allard, Denis, Alldredge, Phillip, Anchordoqui, Luis, Anzalone, Anna, Battisti, Matteo, Belov, Alexander A., Bertaina, Mario, Bertone, Peter F., Blin-Bondil, Sylvie, Burton, Julia, Cafagna, Francesco S., Casolino, Marco, Černý, Karel, Christ, Mark J., Colalillo, Roberta, Crawford, Hank J., Creusot, Alexandre, Cummings, Austin, Diesing, Rebecca, Di Nola, Alessandro, Ebisuzaki, Toshikazu, Eser, Johannes, Ferrarese, Silvia, Filippatos, George, Finch, William W., Flaminio, Flavia, Fornaro, Claudio, Fuehne, Duncan, Fuglesang, Christer, Garg, Diksha, Golzio, Alessio, Guarino, Fausto, Guépin, Claire, Heibges, Tobias, Judd, Eleanor G., Klimov, Pavel A., Krizmanic, John F., Kungel, Viktoria, Kupari, Luke, Kuznetsov, Evgeny, Manfrin, Massimiliano, Marszal, Wlodzimierz, Matthews, John N., Mese, Marco, Meyer, Stephan S., Mignone, Marco, Miyamoto, Hiroko, Murashov, Alexey S., Nachtman, Jane M., Olinto, Angela V., Onel, Yasar, Osteria, Giuseppe, Panico, Beatrice, Parizot, Ètienne, Paul, Tom, Pech, Miroslav, Perfetto, Francesco, Piotrowski, Lech W., Plebaniak, Zbigniew, Posligua, Jonatan, Prévôt, Guillaume, Przybylak, Marika, Reardon, Patrick, Reno, Mary Hall, Ricci, Marco, Sarazin, Fred, Schovánek, P., Scotti, Valentina, Shinozaki, Kenji, Soriano, Jorge F., Stillwell, Ben K., Szabelski, Jacek, Takizawa, Yoshiyuki, Trofimov, Daniil, Unel, Fredrik, Valore, Laura, Venters, Tonia M., Watts Jr., John, Wiencke, Lawrence, Wistrand, Hannah, Young, Roy
Publikováno v:
Astroparticle Physics 165 (2025) 103046
The Extreme Universe Space Observatory on a Super Pressure Balloon 2 (EUSO-SPB2) flew on May 13$^{\text{th}}$ and 14$^{\text{th}}$ of 2023. Consisting of two novel optical telescopes, the payload utilized next-generation instrumentation for the obser
Externí odkaz:
http://arxiv.org/abs/2406.13673
Autor:
Mandal, Ankush, Mukherjee, Dipanjan, Federrath, Christoph, Bicknell, Geoffrey V., Nesvadba, Nicole P. H., Mignone, Andrea
The impact of winds and jet-inflated bubbles driven by active galactic nuclei (AGN) are believed to significantly affect the host galaxy's interstellar medium (ISM) and regulate star formation. To explore this scenario, we perform a suite of hydrodyn
Externí odkaz:
http://arxiv.org/abs/2405.10005
Autor:
Bhandare, Asmita, Commerçon, Benoît, Laibe, Guillaume, Flock, Mario, Kuiper, Rolf, Henning, Thomas, Mignone, Andrea, Marleau, Gabriel-Dominique
Publikováno v:
A&A 687, A158 (2024)
Signposts of early planet formation are ubiquitous in substructured young discs. Dense, hot and high-pressure regions formed during gravitational collapse process, integral to star formation, facilitate dynamical mixing of dust within the protostella
Externí odkaz:
http://arxiv.org/abs/2404.09257