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pro vyhledávání: '"As S"'
This paper presents a systematic exploration of exact solutions for electrically charged wormholes, black holes, and black bounces within the hybrid metric-Palatini gravity (HMPG) framework. HMPG combines features of the metric and Palatini formulati
Externí odkaz:
http://arxiv.org/abs/2412.10324
Autor:
Bermejo-Climent, J. R., Demina, R., Krolewski, A., Chaussidon, E., Rezaie, M., Ahlen, S., Bailey, S., Bianchi, D., Brooks, D., Burtin, E., Claybaugh, T., de la Macorra, A., Dey, Arjun, Doel, P., Farren, G., Ferraro, S., Forero-Romero, J. E., Gaztañaga, E., Gontcho, S. Gontcho A, Gutierrez, G., Hahn, C., Honscheid, K., Howlett, C., Kehoe, R., Kirkby, D., Kisner, T., Landriau, M., Guillou, L. Le, Levi, M. E., Manera, M., Meisner, A., Miquel, R., Moustakas, J., Newman, J. A., Niz, G., Palanque-Delabrouille, N., Percival, W. J., Prada, F., Pérez-Ràfols, I., Rabinowitz, D., Ross, A. J., Rossi, G., Sanchez, E., Schlegel, D., Sprayberry, D., Tarlé, G., Weaver, B. A., White, M., Yèche, C., Zarrouk, P.
We use the angular cross-correlation between a Luminous Red Galaxy (LRG) sample from the DR9 DESI Legacy Survey and the $Planck$ PR4 CMB lensing maps to constrain the local primordial non-Gaussianity parameter $f_{\rm NL}$ using the scale-dependent g
Externí odkaz:
http://arxiv.org/abs/2412.10279
Autor:
Wilzewski, A., Huber, L. I., Door, M., Richter, J., Mariotti, A., Spieß, L. J., Wehrheim, M., Chen, S., King, S. A., Micke, P., Filzinger, M., Steinel, M. R., Huntemann, N., Benkler, E., Schmidt, P. O., Flannery, J., Matt, R., Stadler, M., Oswald, R., Schmid, F., Kienzler, D., Home, J., Craik, D. P. L. Aude, Eliseev, S., Filianin, P., Herkenhoff, J., Kromer, K., Blaum, K., Yerokhin, V. A., Valuev, I. A., Oreshkina, N. S., Lyu, C., Banerjee, S., Keitel, C. H., Harman, Z., Berengut, J. C., Viatkina, A., Gilles, J., Surzhykov, A., Rosner, M. K., López-Urrutia, J. R. Crespo, Fuchs, E.
Nonlinearities in King plots (KP) of isotope shifts (IS) can reveal the existence of beyond-Standard-Model (BSM) interactions that couple electrons and neutrons. However, it is crucial to distinguish higher-order Standard Model (SM) effects from BSM
Externí odkaz:
http://arxiv.org/abs/2412.10277
Autor:
Kootte, B., Reiter, M. P., Andreoiu, C., Beck, S., Bergmann, J., Brunner, T., Dickel, T., Dietrich, K. A., Dilling, J., Dunling, E., Flowerdew, J., Graham, L., Gwinner, G., Hockenbery, Z., Izzo, C., Jacobs, A., Javaji, A., Klawitter, R., Lan, Y., Leistenschneider, E., Lykiardopoulou, E. M., Miskun, I., Mukul, I., Murböck, T., Paul, S. F., Plaß, W. R., Ringuette, J., Scheidenberger, C., Silwal, R., Simpson, R., Teigelhöfer, A., Thompson, R. I., Tracy, Jr., J. L., Vansteenkiste, M., Weil, R., Wieser, M. E., Will, C., Kwiatkowski, A. A.
Direct observation of proton emission with very small emission energy is often unfeasible due to the long partial half-lives associated with tunneling through the Coulomb barrier. Therefore proton emitters with very small Q-values may require masses
Externí odkaz:
http://arxiv.org/abs/2412.10259
This paper presents a comprehensive approach to designing a reliable communication network for the main Smart Factory applications, leveraging Time Sensitive Networks (TSN) and emerging technologies. As the manufacturing sector evolves under Industry
Externí odkaz:
http://arxiv.org/abs/2412.10243
Exploration of optimal hyperfine transitions for spin-wave storage in $^{167}$Er$^{3+}$:Y$_2$SiO$_5$
The dependence of the magnetic fluctuations and the spin coherence time $T_2^{\rm hyp}$ of the lowest Stark states $^4I_{15/2}\ (Z_1)$ in $^{167}$Er$^{3+}$:Y$_2$SiO$_5$ under zero magnetic field on Er concentration is numerically investigated in the
Externí odkaz:
http://arxiv.org/abs/2412.10126
Autor:
Clontz, C., Seth, A. C., Wang, Z., Souza, S. O., Häberle, M., Nitschai, M. S., Neumayer, N., Latour, M., Milone, A. P., Feldmeier-Krause, A., Kacharov, N., Libralato, M., Bellini, A., van de Ven, G., Alfaro-Cuello, M.
Constraining the helium enhancement in stars is critical for understanding the formation mechanisms of multiple populations in star clusters. However, measuring helium variations for many stars within a cluster remains observationally challenging. We
Externí odkaz:
http://arxiv.org/abs/2412.09783
Autor:
Rivinius, Th., Klement, R., Chojnowski, S. D., Baade, D., Abdul-Masih, M., Przybilla, N., Flo, J. Guarro, Heathcote, B., Hadrava, P., Gies, D., Shepard, K., Buil, C., Garde, O., Thizy, O., Monnier, J. D., Anugu, N., Lanthermann, C., Schaefer, G., Davies, C., Kraus, S., Ennis, J., Setterholm, B. R., Gardner, T., Ibrahim, N., Chhabra, S., Gutierrez, M., Codron, I., Mortimer, D.
Many classical Be stars acquire their very rapid rotation by mass and angular-momentum transfer in massive binaries. Short-lived intermediate-phase objects have only been discovered recently. Data archives and the literature have been searched for ad
Externí odkaz:
http://arxiv.org/abs/2412.09720
Autor:
Mróz, M. J., Poleski, R., Udalski, A., Sumi, T., Tsapras, Y., Hundertmark, M., Pietrukowicz, P., Szymański, M. K., Skowron, J., Mróz, P., Gromadzki, M., Iwanek, P., Kozłowski, S., Ratajczak, M., Rybicki, K. A., Skowron, D. M., Soszyński, I., Ulaczyk, K., Wrona, M., Abe, F., Bando, K., Bennett, D. P., Bhattacharya, A., Bond, I. A., Fukui, A., Hamada, R., Hamada, S., Hamasaki, N., Hirao, Y., Silva, S. Ishitani, Itow, Y., Koshimoto, N., Matsubara, Y., Miyazaki, S., Muraki, Y., Nagai, T., Nunota, K., Olmschenk, G., Ranc, C., Rattenbury, N. J., Satoh, Y., Suzuki, D., Terry, S. K., Tristram, P. J., Vandorou, A., Yama, H., Street, R. A., Bachelet, E., Dominik, M., Cassan, A., Jaimes, R. Figuera, Horne, K., Schmidt, R., Snodgrass, C., Wambsganss, J., Steele, I. A., Menzies, J., Jørgensen, U. G., Longa-Peña, P., Peixinho, N., Skottfelt, J., Southworth, J., Andersen, M. I., Bozza, V., Burgdorf, M. J., D'Ago, G., Hinse, T. C., Kerins, E., Korhonen, H., Küffmeier, M., Mancini, L., Rabus, M., Rahvar, S.
We present a comprehensive analysis of a planetary microlensing event OGLE-2015-BLG-1609. The planetary anomaly was detected by two survey telescopes, OGLE and MOA. Each of these surveys collected enough data over the planetary anomaly to allow for a
Externí odkaz:
http://arxiv.org/abs/2412.09676
Autor:
Hamadouche, M. L., McLure, R. J., Carnall, A., McLeod, D. J., Dunlop, J. S., Whitaker, K., Donnan, C. T., Begley, R., Stanton, T. M., Almaini, O., Aird, J., Cullen, F., Cutler, S., Koekemoer, A. M.
We present the results of a study investigating the galaxy stellar-mass function (GSMF), size-mass relations and morphological properties of star-forming and quiescent galaxies over the redshift range $0.25
Externí odkaz:
http://arxiv.org/abs/2412.09592