Zobrazeno 1 - 10
of 101 548
pro vyhledávání: '"A Montes"'
We explore quantum-thermodynamic effects in a phosphorous (P)-doped graphene monolayer subjected to biaxial tensile strain. Introducing substitutional P atoms in the graphene lattice generates a tunable spin magnetic moment controlled by the strain c
Externí odkaz:
http://arxiv.org/abs/2411.12959
Autor:
Lauer-Coles, A., Deibel, C. M., Blackmon, J. C., Hood, A., Good, E. C., Macon, K. T., Santiago-Gonzalez, D., Schatz, H., Ahn, T., Browne, J., Montes, F., Schmidt, K., Ong, 4 W. J., Chipps, K. A., Pain, S. D., Wiedenhöver, I., Baby, L. T., Rijal, N., Anastasiou, M., Upadhyayula, S., Bedoor, S., Hooker, J., Koshchiy, E., Rogachev, G. V.
Background: Type I X-Ray bursts (XRBs) are energetic stellar explosions that occur on the surface of a neutron star in an accreting binary system with a low-mass H/He-rich companion. The rate of the $^{34}$Ar($\alpha,p$)$^{37}$K reaction may influenc
Externí odkaz:
http://arxiv.org/abs/2411.09918
In this paper we use the collapse metric obtained by Carneiro and Fabris to calculate the power spectrum associated to gauge invariant fluctuations of the metric during the formation of a primordial scalar black hole at the end of inflation. We assum
Externí odkaz:
http://arxiv.org/abs/2411.07580
Autor:
Cortés-Contreras, M., Caballero, J. A., Montes, D., Cardona-Guillén, C., Béjar, V. J. S., Cifuentes, C., Tabernero, H. M., Osorio, M. R. Zapatero, Amado, P. J., Jeffers, S. V., Lafarga, M., Lodieu, N., Quirrenbach, A., Reiners, A., Ribas, I., Schöfer, P., Schweitzer, A., Seifert, W.
Aims. Our goals are to characterise the kinematic properties and to identify young and old stars among the M dwarfs of the CARMENES input catalogue. Methods. We compiled the spectral types, proper motions, distances, and radial velocities for 2187 M
Externí odkaz:
http://arxiv.org/abs/2411.06825
Autor:
Montes-Rodríguez, A., Virtanen, J. A.
We give very simple proofs of the classical results of Magnus and Hill on the spectral properties of the Hilbert matrix $$ H = \left ( {1 \over i+j+ 1 } \right )_{i,j\geq 0} $$ which defines a bounded linear operator on the sequence space $\ell^2$. I
Externí odkaz:
http://arxiv.org/abs/2411.07324
Autor:
Pardo, J. R., De Breuck, C., Muders, D., González, J., Pérez-Beaupuits, J. P., Cernicharo, J., Prigent, C., Serabyn, E., Montenegro-Montes, F. M., Mroczkowski, T., Phillips, N., Villard, E.
Due to the importance of a reference atmospheric radiative transfer model for both planning and calibrating ground-based observations at millimetre and submillimetre wavelengths, we have undertaken a validation campaign consisting of acquiring atmosp
Externí odkaz:
http://arxiv.org/abs/2411.03134
Autor:
Dong, Jiayin, Chontos, Ashley, Zhou, George, Stefansson, Gudmundur, Wang, Songhu, Huang, Chelsea X., Gupta, Arvind F., Halverson, Samuel, Kanodia, Shubham, Luhn, Jacob K., Mahadevan, Suvrath, Monson, Andrew, Alvarado-Montes, Jaime A., Ninan, Joe P., Robertson, Paul, Roy, Arpita, Schwab, Christian, Wright, Jason T.
Super Jupiters are giant planets with several Jupiter masses. It remains an open question whether these planets originate with such high masses or grow through collisions. Previous work demonstrates that warm super Jupiters tend to have more eccentri
Externí odkaz:
http://arxiv.org/abs/2411.01356
Autor:
Tsintari, P., Dimitrakopoulos, N., Garg, R., Hermansen, K., Marshall, C., Montes, F., Perdikakis, G., Schatz, H., Setoodehnia, K., Arora, H., Berg, G. P. A., Bhandari, R., Blackmon, J. C., Brune, C. R., Chipps, K. A., Couder, M., Deibel, C., Hood, A., Gamage, M. Horana, Jain, R., Maher, C., Miskovitch, S., Pereira, J., Ruland, T., Smith, M. S., Smith, M., Sultana, I., Tinson, C., Tsantiri, A., Villari, A., Wagner, L., Zegers, R. G. T.
The synthesis of heavy elements in supernovae is affected by low-energy (n,p) and (p,n) reactions on unstable nuclei, yet experimental data on such reaction rates are scarce. The SECAR (SEparator for CApture Reactions) recoil separator at FRIB (Facil
Externí odkaz:
http://arxiv.org/abs/2411.03338
Autor:
Alfaro, R., Alvarez, C., Arteaga-Velázquez, J. C., Rojas, D. Avila, Solares, H. A. Ayala, Babu, R., Belmont-Moreno, E., Caballero-Mora, K. S., Capistrán, T., Carramiñana, A., Casanova, S., Cotzomi, J., De la Fuente, E., Depaoli, D., Di Lalla, N., Hernandez, R. Diaz, Dingus, B. L ., DuVernois, M. A., Engel, K., Ergin, T., Espinoza, C ., Fan, K. L., Fang, K., Fraija, N., Fraija, S., García-González, J. A., Muñoz, A. González, González, M. M., Goodman, J. A., Groetsch, S., Harding, J. P., Hernández-Cadena, S., Herzog, I., Huang, D., Hueyotl-Zahuantitla, F., Hüntemeyer, P., Iriarte, A., Kaufmann, S., Lara, A ., Lee, W. H., Lee, J., de León, C., Vargas, H. León, Longinotti, A. L., Luis-Raya, G., Malone, K., Martínez-Castro, J., Matthews, J. A., Miranda-Romagnoli, P., Montes, J. A., Moreno, E., Mostafá, M., Nellen, L., Nisa, M. U ., Noriega-Papaqui, R ., Araujo, Y. Pérez, Pérez-Pérez, E. G., Rho, C. D., Rosa-González, D., Ruiz-Velasco, E ., Salazar, H., Sandoval, A., Schneider, M., Serna-Franco, J., Smith, A. J., Son, Y., Springer, R. W ., Tibolla, O., Tollefson, K., Torres, I., Torres-Escobedo, R., Turner, R., Ureña-Mena, F., Varela, E ., Villaseñor, L., Wang, X., Wang, Z., Watson, I. J., Yu, S ., Yun-Cárcamo, S., Zhou, H.
Publikováno v:
ApJ 976 (2024) 30
Very-high-energy (0.1-100 TeV) gamma-ray emission was observed in HAWC data from the lobes of the microquasar SS 433, making them the first set of astrophysical jets that were resolved at TeV energies. In this work, we update the analysis of SS 433 u
Externí odkaz:
http://arxiv.org/abs/2410.21796
Autor:
Sedighi, Nafise, Sharbaf, Zahra, Trujillo, Ignacio, Eskandarlou, Sepideh, Golini, Giulia, Infante-Sainz, Raúl, Raji, Samane, Zaritsky, Dennis, Ardakani, Pedram Ashofteh, Chamba, Nushkia, Shahisavandi, Zahra Hosseini, Donnerstein, Richard, D'Onofrio, Mauro, Martin, Garreth, Montes, Mireia, Román, Javier
With the arrival of the next generation of ultra-deep optical imaging surveys reaching $\mu_V$$\sim$30 mag/arcsec$^2$ (3$\sigma$; 10"$\times$10"), the removal of scattered light due to the point spread function (PSF) effect remains a critical step fo
Externí odkaz:
http://arxiv.org/abs/2410.20190