Zobrazeno 1 - 10
of 9 078
pro vyhledávání: '"BELLI, P."'
Autor:
Kim, Donguk, Moon, Taeuk, Sung, Choongki, Yoon, Eisung, Yi, Sumin, Kang, Jisung, Kwon, Jae-Min, Görler, Tobias, Belli, Emily, Candy, Jeff
This study presents a cross-verification of fast ion effects on turbulence through a systematic comparison of two leading gyrokinetic codes, GENE [T.Gorler et al., J. Comput. Phys. 230 7053-7071 (2011)] and CGYRO [J.Candy et al, J. Comput. Phys. 324
Externí odkaz:
http://arxiv.org/abs/2408.13731
Autor:
Belli, P., Bernabei, R., Cappella, F., Caracciolo, V., Cerulli, R., Danevich, F. A., Denisov, V. Yu., Incicchitti, A., Kasperovych, D. V., Kobychev, V. V., Kovtun, G. P., Laubenstein, M., Poda, D. V., Polischuk, O. G., Shcherban, A. P., Solopikhin, D. A., Tessalina, S., Tretyak, V. I.
Publikováno v:
Eur. Phys. J. A 60 (2024) 150
A long-term measurement was conducted to search for $\alpha$, double-$\alpha$ and double-$\beta$ decays with $\gamma$ quanta emission in naturally occurring osmium isotopes. This study took advantage of two ultra-low background HPGe detectors and one
Externí odkaz:
http://arxiv.org/abs/2406.19062
Autor:
Belli, Francesco, Zurek, Eva
Quantum nuclear effects and anharmonicity impact a wide range of functional materials and their properties. One of the most powerful techniques to model these effects is the Stochastic Self-Consistent Harmonic Approximation (SSCHA). Unfortunately, th
Externí odkaz:
http://arxiv.org/abs/2406.13178
Autor:
Bugiani, Letizia, Belli, Sirio, Park, Minjung, Davies, Rebecca L., Mendel, J. Trevor, Johnson, Benjamin D., Khoram, Amir H., Benton, Chloë, Cimatti, Andrea, Conroy, Charlie, Emami, Razieh, Leja, Joel, Li, Yijia, Maheson, Gabriel, Mathews, Elijah P., Naidu, Rohan P., Nelson, Erica J., Tacchella, Sandro, Terrazas, Bryan A., Weinberger, Rainer
We analyze ionized gas emission lines in deep rest-frame optical spectra of 16 quiescent galaxies at redshift $1.7
Externí odkaz:
http://arxiv.org/abs/2406.08547
Autor:
Jafariyazani, Marziye, Newman, Andrew B., Mobasher, Bahram, Belli, Sirio, Ellis, Richard S., Faisst, Andreas L.
Recent stellar chemical abundance measurements of a handful of $z\sim2$ quiescent galaxies have suggested these galaxies exhibit a remarkably strong $\alpha$-enhancement compared to their local and intermediate redshift counterparts. This apparent ch
Externí odkaz:
http://arxiv.org/abs/2406.03549
Autor:
Li, Yijia, Leja, Joel, Johnson, Benjamin D., Tacchella, Sandro, Davies, Rebecca, Belli, Sirio, Park, Minjung, Emami, Razieh
The complex physics governing nebular emission in galaxies, particularly in the early universe, often defy simple low-dimensional models. This has proven to be a significant barrier in understanding the (often diverse) ionizing sources powering this
Externí odkaz:
http://arxiv.org/abs/2405.04598
Autor:
Park, Minjung, Belli, Sirio, Conroy, Charlie, Johnson, Benjamin D., Davies, Rebecca L., Leja, Joel, Tacchella, Sandro, Mendel, J. Trevor, Benton, Chloë, Bugiani, Letizia, Emami, Razieh, Khoram, Amirhossein, Li, Yijia, Maheson, Gabriel, Mathews, Elijah P., Naidu, Rohan P., Nelson, Erica J., Terrazas, Bryan A., Weinberger, Rainer
Massive quiescent galaxies in the young universe are expected to be quenched rapidly, but it is unclear whether they all experience starbursts before quenching and what physical mechanism drives rapid quenching. We study 16 massive quiescent galaxies
Externí odkaz:
http://arxiv.org/abs/2404.17945
Autor:
Zhang, Hao, Sun, Linshan, Hirschman, Jack, Shariatdoust, Mirali Seyed, Belli, Federico, Carbajo, Sergio
Four-wave mixing (FWM) in gas-filled hollow-core capillaries, a nonlinear optical process that mixes signal and pump photon frequencies to generate idler frequency photons, offers a method for precise spectral phase transfer from signal to idler at u
Externí odkaz:
http://arxiv.org/abs/2404.16993
Autor:
Pierel, J. D. R., Newman, A. B., Dhawan, S., Gu, M., Joshi, B. A., Li, T., Schuldt, S., Strolger, L. G., Suyu, S. H., Caminha, G. B., Cohen, S. H., Diego, J. M., Dsilva, J. C. J., Ertl, S., Frye, B. L., Granata, G., Grillo, C., Koekemoer, A. M., Li, J., Robotham, A., Summers, J., Treu, T., Windhorst, R. A., Zitrin, A., Agarwal, S., Agrawal, A., Arendse, N., Belli, S., Burns, C., Cañameras, R., Chakrabarti, S., Chen, W., Collett, T. E., Coulter, D. A., Ellis, R. S., Engesser, M., Foo, N., Fox, O. D., Gall, C., Garuda, N., Gezari, S., Gomez, S., Glazebrook, K., Hjorth, J., Huang, X., Jha, S. W., Kamieneski, P. S., Kelly, P., Larison, C., Moustakas, L. A., Pascale, M., Pérez-Fournon, I., Petrushevska, T., Poidevin, F., Rest, A., Shahbandeh, M., Shajib, A. J., Siebert, M., Storfer, C., Talbot, M., Wang, Q., Wevers, T., Zenati, Y.
A bright ($m_{\rm F150W,AB}$=24 mag), $z=1.95$ supernova (SN) candidate was discovered in JWST/NIRCam imaging acquired on 2023 November 17. The SN is quintuply-imaged as a result of strong gravitational lensing by a foreground galaxy cluster, detecte
Externí odkaz:
http://arxiv.org/abs/2404.02139
We explore electronic and structural properties of Fm$\overline{3}$m Lu-H-N structures with specific N,H ordering as plausible candidates for near-ambient superconductivity possibly originating from their remarkably narrow hydrogen-based bands at the
Externí odkaz:
http://arxiv.org/abs/2403.01350