Zobrazeno 1 - 10
of 2 593
pro vyhledávání: '"Coloma, P."'
Autor:
Puga, Miguel Coloma, Balmaverde, Barbara, Capetti, Alessandro, Almeida, Cristina Ramos, Massaro, Francesco, Venturi, Giacomo
The study of ionized gas kinematics in high-z active galaxies plays a key part in our understanding of galactic evolution, in an age where nuclear activity was widespread and star formation close to its peak. We present a study of TXS 0952-217, a rad
Externí odkaz:
http://arxiv.org/abs/2405.09884
Autor:
Fraudet, Dorian, Snyman, Izak, Basko, Denis M., Léger, Sébastien, Sépulcre, Théo, Ranadive, Arpit, Gal, Gwenael Le, Torras-Coloma, Alba, Florens, Serge, Roch, Nicolas
We study spontaneous photon decay into multiple photons triggered by strong non-linearities in a superconducting quantum simulator of the boundary sine-Gordon impurity model. Previously, spectroscopic signatures of photon-conversion were reported and
Externí odkaz:
http://arxiv.org/abs/2405.00411
Immersive Rover Control and Obstacle Detection based on Extended Reality and Artificial Intelligence
Autor:
Coloma, Sofía, Frantz, Alexandre, van der Meer, Dave, Skrzypczyk, Ernest, Orsula, Andrej, Olivares-Mendez, Miguel
Publikováno v:
IEEE VR Conference 2024
Lunar exploration has become a key focus, driving scientific and technological advances. Ongoing missions are deploying rovers to the surface of the Moon, targeting the far side and south pole. However, these terrains pose challenges, emphasizing the
Externí odkaz:
http://arxiv.org/abs/2404.14095
Autor:
Coloma-Nadal, J. M., Kitaura, F. -S., García-Farieta, J. E., Sinigaglia, F., Favole, G., Sánchez, D. Forero
Accurate modeling of galaxy distributions is paramount for cosmological analysis using galaxy redshift surveys. However, this endeavor is often hindered by the computational complexity of resolving the dark matter halos that host these galaxies. To a
Externí odkaz:
http://arxiv.org/abs/2403.19337
Autor:
Forero-Sánchez, Daniel, Kitaura, Francisco-Shu, Sinigaglia, Francesco, Coloma-Nadal, Jose María, Kneib, Jean-Paul
Modern galaxy surveys demand extensive survey volumes and resolutions surpassing current dark matter-only simulations' capabilities. To address this, many methods employ effective bias models on the dark matter field to approximate object counts on a
Externí odkaz:
http://arxiv.org/abs/2402.17581
The upcoming European Spallation Source (ESS) will soon provide the most intense neutrino source in the world. We propose the Search for Hidden Neutrinos at the ESS (SHiNESS) experiment, highlighting its unique opportunities to search for the existen
Externí odkaz:
http://arxiv.org/abs/2311.18509
Autor:
López-Núñez, David, Montserrat, Queralt Portell, Rius, Gemma, Bertoldo, Elia, Torras-Coloma, Alba, Martínez, M., Forn-Díaz, P.
We present a study of the superconducting penetration depth $\lambda$ in aluminum thin films of varying thickness. The range of thicknesses chosen spans from the thin-film regime to the regime approaching bulk behavior. The penetration depths observe
Externí odkaz:
http://arxiv.org/abs/2311.14119
Autor:
Puga, Miguel Coloma, Balmaverde, Barbara, Capetti, Alessandro, Massaro, Francesco, Almeida, Cristina Ramos, Miley, George, Gilli, Roberto, Marconi, Alessandro
Spatially resolved observations of AGN host galaxies undergoing feedback processes are one of the most relevant avenues through which galactic evolution can be studied, given the long lasting effects AGN feedback has on gas reservoirs, star formation
Externí odkaz:
http://arxiv.org/abs/2311.08507
Long-lived particles (LLPs) arise in many theories beyond the Standard Model. These may be copiously produced from meson decays (or through their mixing with the LLP) at neutrino facilities and leave a visible decay signal in nearby neutrino detector
Externí odkaz:
http://arxiv.org/abs/2309.06492
Autor:
Torras-Coloma, Alba, de Olcoz, Leyre Martínez, Céspedes, Eva, Bertoldo, Elia, López-Núñez, David, Paul, Sagar, Wernsdorfer, Wolfgang, Rius, Gemma, Forn-Díaz, Pol
We report the direct observation of superconductivity in nitridized-aluminum thin films. The films are produced by sputtering deposition of aluminum in a controlled mixture of nitrogen diluted in argon. The concentration of applied nitrogen directly
Externí odkaz:
http://arxiv.org/abs/2308.06240