Zobrazeno 1 - 10
of 7 606
pro vyhledávání: '"Venuti A"'
Autor:
Liu, Jiangteng, Schoell, Ryan, Zhang, Xiyue S., Yang, Hongbin, Venuti, M. B., Paik, Hanjong, Muller, David A., Lu, Tzu-Ming, Hattar, Khalid, Eley, Serena
A promising architecture for next-generation, low energy spintronic devices uses skyrmions -- nanoscale whirlpools of magnetic moment -- as information carriers. Notably, schemes for racetrack memory have been proposed in which skyrmions and antiskyr
Externí odkaz:
http://arxiv.org/abs/2409.02325
Autor:
Wendeborn, John, Espaillat, Catherine C., Thanathibodee, Thanawuth, Robinson, Connor E., Pittman, Caeley V., Calvet, Nuria, Muzerolle, James, Walter, Fredrick M., Eisloffel, Jochen, Fiorellino, Eleonora, Manara, Carlo F., Kospal, Agnes, Abraham, Peter, Claes, Rik, Rigliaco, Elisabetta, Venuti, Laura, Campbell-White, Justyn, McGinnis, Pauline, Gangi, Manuele, Mauco, Karina, Gameiro, Filipe, Frasca, Antonio, Guo, Zhen
Classical T Tauri Stars (CTTSs) are highly variable stars that possess gas- and dust-rich disks from which planets form. Much of their variability is driven by mass accretion from the surrounding disk, a process that is still not entirely understood.
Externí odkaz:
http://arxiv.org/abs/2408.04465
Autor:
Graziosi, Patrizio, Della Valle, Raffaele Guido, Salzillo, Tommaso, d'Agostino, Simone, Zangari, Martina, Cane', Elisabetta, Masino, Matteo, Venuti, Elisabetta
We have developed a first-principles method to calculate the electron-phonon coupling for specific modes and q-points in the Brillouin Zone for crystalline organic semiconductors. Using the obtained coupling strengths, we propose an approach to compu
Externí odkaz:
http://arxiv.org/abs/2407.18824
Autor:
Claes, R. A. B., Campbell-White, J., Manara, C. F., Frasca, A., Natta, A., Alcalá, J. M., Armeni, A., Fang, M., Lovell, J. B., Stelzer, B., Venuti, L., Wyatt, M., Queitsch, A.
Studies of the stellar and accretion properties of classical T Tauri stars (CTTS) require comparison with photospheric spectral templates. Here we aim at expanding the currently available grid of wide-wavelength coverage observed spectra of non-accre
Externí odkaz:
http://arxiv.org/abs/2407.11866
Autor:
Alvari, Gianpaolo, Vallefuoco, Ersilia, Cristofolini, Melanie, Salvadori, Elio, Dianti, Marco, Moltani, Alessia, Castello, Davide Dal, Venuti, Paola, Furlanello, Cesare
Virtual Reality (VR) has emerged as a promising tool for enhancing social skills and emotional well-being in individuals with Autism Spectrum Disorder (ASD). Through a technical exploration, this study employs a multiplayer serious gaming environment
Externí odkaz:
http://arxiv.org/abs/2404.07159
Autor:
Manick, R., Sousa, A. P., Bouvier, J., Almenara, J. M., Rebull, L., Bayo, A., Carmona, A., Martioli, E., Venuti, L., Pantolmos, G., Kóspál, Á., Zanni, C., Bonfils, X., Moutou, C., Delfosse, X., consortium, the SLS
Publikováno v:
A&A 686, A249 (2024)
Detecting planets within protoplanetary disks around young stars is essential for understanding planet formation and evolution. However, planet detection using the radial velocity method faces challenges due to strong stellar activity in these early
Externí odkaz:
http://arxiv.org/abs/2403.03706
Circumstellar disk accretion across the Lagoon Nebula: the influence of environment and stellar mass
Autor:
Venuti, L., Cody, A. M., Beccari, G., Rebull, L. M., Irwin, M. J., Thanvantri, A., Thanvantri, S., Alencar, S. H. P., Leal, C. O., Barentsen, G., Drew, J. E., Howell, S. B.
Pre-main sequence disk accretion is pivotal in determining the final stellar properties and the early conditions for close-in planets. We aim to establish the impact of internal (stellar mass) and external (radiation field) parameters on disk evoluti
Externí odkaz:
http://arxiv.org/abs/2401.06767
Autor:
Venuti, M. B., Zhang, Xiyue S., Lang, Eric J, Addamane, Sadhvikas J., Paik, Hanjong, Allen, Portia, Sharma, Peter, Muller, David, Hattar, Khalid, Lu, Tzu-Ming, Eley, Serena
Skyrmions and antiskyrmions are nanoscale swirling textures of magnetic moments formed by chiral interactions between atomic spins in magnetic non-centrosymmetric materials and multilayer films with broken inversion symmetry. These quasiparticles are
Externí odkaz:
http://arxiv.org/abs/2311.13130
Dispersion relations let us leverage the analytic structure of scattering amplitudes to derive constraints such as bounds on EFT coefficients. An important input is the large-energy behavior of the amplitude. In this paper, we systematically study ho
Externí odkaz:
http://arxiv.org/abs/2310.06888
Autor:
Herczeg, Gregory J., Chen, Yuguang, Donati, Jean-Francois, Dupree, Andrea K., Walter, Frederick M., Hillenbrand, Lynne A., Johns-Krull, Christopher M., Manara, Carlo F., Guenther, Hans Moritz, Fang, Min, Schneider, P. Christian, Valenti, Jeff A., Alencar, Silvia H. P., Venuti, Laura, Alcala, Juan Manuel, Frasca, Antonio, Arulanantham, Nicole, Linsky, Jeffrey L., Bouvier, Jerome, Brickhouse, Nancy S., Calvet, Nuria, Espaillat, Catherine C., Campbell-White, Justyn, Carpenter, John M., Chang, Seok-Jun, Cruz, Kelle L., Dahm, S. E., Eisloeffel, Jochen, Edwards, Suzan, Fischer, William J., Guo, Zhen, Henning, Thomas, Ji, Tao, Jose, Jesse, Kastner, Joel H., Launhardt, Ralf, Principe, David A., Robinson, Conner E., Serna, Javier, Siwak, Michal, Sterzik, Michael F., Takasao, Shinsuke
Accretion plays a central role in the physics that governs the evolution and dispersal of protoplanetary disks. The primary goal of this paper is to analyze the stability over time of the mass accretion rate onto TW Hya, the nearest accreting solar-m
Externí odkaz:
http://arxiv.org/abs/2308.14590