Zobrazeno 1 - 10
of 7 764
pro vyhledávání: '"Alban, P."'
Autor:
Puech, Alban, Mirallès, François, Weiss, Jonas, Mai, Vincent, Massé, Alexandre Blondin, de Montigny, Martin, Brunschwiler, Thomas, Hamann, Hendrik F.
Quasi-static time series (QSTS) simulations have great potential for evaluating the grid's ability to accommodate the large-scale integration of distributed energy resources. However, as grids expand and operate closer to their limits, iterative powe
Externí odkaz:
http://arxiv.org/abs/2411.08652
Autor:
Montjovet-Basset, Félix, Panigrahi, Jayash, Serrano, Diana, Ferrier, Alban, Flurin, Emmanuel, Bertet, Patrice, Tiranov, Alexey, Goldner, Philippe
Quantum state lifetimes $T_2$, or equivalently homogeneous linewidths $\Gamma_h = 1/\pi T_2$, are a key parameter for understanding decoherence processes in quantum systems and assessing their potential for applications in quantum technologies. The m
Externí odkaz:
http://arxiv.org/abs/2411.06532
Quantum technologies provide many applications for information processing tasks that are impossible to realize within classical physics. These capabilities include such fundamental resources as generating secure, i.e. private and unpredictable random
Externí odkaz:
http://arxiv.org/abs/2411.04934
Autor:
de Mellos, Maitê S. Z., Riffel, Rogemar A., Schimoia, Jaderson S., Rembold, Sandro B., Riffel, Rogério, Storchi-Bergmann, Thaisa, Wylezalek, Dominika, Ilha, Gabriele S., Albán, Marco, Dors, Oli L., Gatto, Lara, Krabbe, Angela C., Mallmann, Nicolas D., Trevisan, Marina
The influence of Active Galactic Nuclei (AGN) on star formation within their host galaxies remains a topic of intense debate. One of the primary challenges in quantifying the star formation rate (SFR) within AGN hosts arises from the prevalent assump
Externí odkaz:
http://arxiv.org/abs/2410.06297
Publikováno v:
xAI 2024 - The 2nd World Conference on eXplainable Artificial Intelligence, Jul 2024, La valette, Malta. pp.TBD
In the field of explainable AI, a vibrant effort is dedicated to the design of self-explainable models, as a more principled alternative to post-hoc methods that attempt to explain the decisions after a model opaquely makes them. However, this produc
Externí odkaz:
http://arxiv.org/abs/2409.16693
Autor:
Vincent, Bjarne, Henry, Daniel, Kumar, Abhishek, Botton, Valéry, Pothérat, Alban, Miralles, Sophie
This work identifies the physical mechanisms at play in the different flow regions along an Eckart acoustic streaming jet by means of numerical simulation based on a novel modeling of the driving acoustic force including attenuation effects. The flow
Externí odkaz:
http://arxiv.org/abs/2409.15083
Autor:
Mothkuri, Sagar, Reid, Michael F., Wells, Jon-Paul R., Lafitte-Houssat, Eloïse, Ferrier, Alban, Goldner, Philippe
Publikováno v:
Journal of Luminescence 275, 120705 (2024)
Laser site-selective spectroscopy and high-resolution absorption measurements have been used to determine 51 crystal-field energy levels for one of the Ho$^{3+}$ centres in Y$_{2}$SiO$_{5}$. This centre is denoted as Site 2 and has been tentatively a
Externí odkaz:
http://arxiv.org/abs/2409.15625
In this paper we generalize the technique of deflation to define two new methods to systematically find many local minima of a nonlinear least squares problem. The methods are based on the Gauss-Newton algorithm, and as such do not require the calcul
Externí odkaz:
http://arxiv.org/abs/2409.14438
Autor:
Poirier-Ginter, Yohan, Gauthier, Alban, Philip, Julien, Lalonde, Jean-Francois, Drettakis, George
Publikováno v:
Computer Graphics Forum, Volume 43 (2024), Number 4
Relighting radiance fields is severely underconstrained for multi-view data, which is most often captured under a single illumination condition; It is especially hard for full scenes containing multiple objects. We introduce a method to create religh
Externí odkaz:
http://arxiv.org/abs/2409.08947
Autor:
Pothérat, Alban, Horn, Susanne
The interiors of many planets consist mostly of fluid layers. When these layers are subject to superadiabatic temperature or compositional gradients, turbulent convection transports heat and momentum. In addition, planets are fast rotators. Thus, the
Externí odkaz:
http://arxiv.org/abs/2409.05220