Zobrazeno 1 - 10
of 10 853
pro vyhledávání: '"Puebla A"'
Quantum information scrambling refers to the spread of the initially stored information over many degrees of freedom of a quantum many-body system. Information scrambling is intimately linked to the thermalization of isolated quantum many-body system
Externí odkaz:
http://arxiv.org/abs/2408.02735
The generation of entanglement across different nodes in distributed quantum architectures plays a pivotal role for different applications. In particular, deterministic, robust, and fast protocols that prepare genuine multipartite entangled states ar
Externí odkaz:
http://arxiv.org/abs/2408.01177
Autor:
Yalcin, Eyüp, Kalitukha, Ina V., Akimov, Ilya A., Korenev, Vladimir L., Ken, Olga S., Puebla, Jorge, Otani, Yoshichika, Hutchings, Oscar M., Gillard, Daniel J., Tartakovskii, Alexander I., Bayer, Manfred
Publikováno v:
Phys. Rev. B 110, L161405 (2024)
We study the Hanle and spin polarization recovery effects on resident electrons in a monolayer MoSe$_2$ on EuS. We demonstrate that localized electrons provide the main contribution to the spin dynamics signal at low temperatures below 15~K for small
Externí odkaz:
http://arxiv.org/abs/2407.01454
Autor:
Pucher, Thomas, Puebla, Sergio, Zamora, Victor, Viso, Estrella Sánchez, Rouco, Victor, Leon, Carlos, Garcia-Hernandez, Mar, Santamaria, Jacobo, Munuera, Carmen, Castellanos-Gomez, Andres
We present the electrostatic control of photoluminescence of monolayer MoS$_2$ at room temperature via integration of free-standing BaTiO$_3$ (BTO), a ferroelectric perovskite oxide, layers. We show that the use of BTO leads to highly tunable exciton
Externí odkaz:
http://arxiv.org/abs/2405.05862
Autor:
Rodriguez-Puebla, Aldo
The current cosmological paradigm asserts that dark matter halos provide the gravitational scaffolding for galaxy formation through a combination of hierarchical structure formation and non-linear local (g)astrophysical processes. This close relation
Externí odkaz:
http://arxiv.org/abs/2404.10801
Autor:
Stephenson, Jimena, Rodriguez-Puebla, Aldo, Faber, S. M., Primack, Joel R., Avila-Reese, Vladimir, Calette, A. R., Cannarozzo, Carlo, Kakos, James, Cano-Díaz, Mariana, Koo, David C., Shankar, Francesco, Morell, D. F.
We investigate the relation between galaxy structure and star formation rate (SFR) in a sample of $\sim2.9\times10^{4}$ central galaxies with $z<0.0674$ and axial ratios $b/a>0.5$. The star-forming main sequence (SFMS) shows a bend around the stellar
Externí odkaz:
http://arxiv.org/abs/2404.10114
Autor:
Biscione, Valerio, Yin, Dong, Malhotra, Gaurav, Dujmovic, Marin, Montero, Milton L., Puebla, Guillermo, Adolfi, Federico, Heaton, Rachel F., Hummel, John E., Evans, Benjamin D., Habashy, Karim, Bowers, Jeffrey S.
Multiple benchmarks have been developed to assess the alignment between deep neural networks (DNNs) and human vision. In almost all cases these benchmarks are observational in the sense they are composed of behavioural and brain responses to naturali
Externí odkaz:
http://arxiv.org/abs/2404.05290
Autor:
Nava-Moreno, Norma Araceli, Montaña, Alfredo, Aretxaga, Itziar, Rodríguez-Puebla, Aldo, Avila-Reese, Vladimir, Sánchez, Edgar Peralta
We present a new cosmologically motivated mock redshift survey of the Dusty Star-Forming Galaxy population. Our mock survey is based on the Bolshoi-Planck dark-matter halo simulation and covers an area of 5.3 sq. degree. Using a semi-empirical approa
Externí odkaz:
http://arxiv.org/abs/2403.15650
In this article, we consider a realistic waveguide implementation of a quantum network that serves as a testbed to show how to maximize the storage and manipulation of quantum information in QED setups. We analyze two approaches using wavepacket engi
Externí odkaz:
http://arxiv.org/abs/2403.12222
Autor:
Kakos, James, Rodriguez-Puebla, Aldo, Primack, Joel R., Faber, Sandra M., Koo, David C., Behroozi, Peter, Avila-Reese, Vladimir
We measure the clustering of low-redshift SDSS galaxies as a function of stellar mass ($10.0<\log(M_*/M_\odot)<11.5$) and specific star formation rate (sSFR) and compare the results to models of the galaxy--halo connection. We find that the auto-corr
Externí odkaz:
http://arxiv.org/abs/2403.01393