Zobrazeno 1 - 10
of 3 730
pro vyhledávání: '"A. Feldmeier"'
Autor:
Maximilian Häberle, N. Neumayer, A. Bellini, M. Libralato, C. Clontz, A. C. Seth, M. S. Nitschai, S. Kamann, M. Alfaro-Cuello, J. Anderson, S. Dreizler, A. Feldmeier-Krause, N. Kacharov, M. Latour, A. P. Milone, R. Pechetti, G. van de Ven, K. Voggel
Publikováno v:
The Astrophysical Journal, Vol 970, Iss 2, p 192 (2024)
Omega Centauri ( ω Cen) is the most massive globular cluster of the Milky Way. It is thought to be the nucleus of an accreted dwarf galaxy because of its high mass and its complex stellar populations. To decipher its formation history and study its
Externí odkaz:
https://doaj.org/article/c6a17bba19504e269f6ba9ad4101c6b3
Autor:
M. S. Nitschai, N. Neumayer, M. Häberle, C. Clontz, A. C. Seth, A. P. Milone, M. Alfaro-Cuello, A. Bellini, S. Dreizler, A. Feldmeier-Krause, T.-O. Husser, N. Kacharov, S. Kamann, M. Latour, M. Libralato, G. van de Ven, K. Voggel, Z. Wang
Publikováno v:
The Astrophysical Journal, Vol 970, Iss 2, p 152 (2024)
ω Centauri, the most massive globular cluster in the Milky Way, has long been suspected to be the stripped nucleus of a dwarf galaxy that fell into the Galaxy a long time ago. There is considerable evidence for this scenario including a large spread
Externí odkaz:
https://doaj.org/article/2167d54e3a23419ca207b8ddb4d708be
Neutral atom arrays driven into Rydberg states constitute a promising approach for realizing programmable quantum systems. Enabled by strong interactions associated with Rydberg blockade, they allow for simulation of complex spin models and quantum d
Externí odkaz:
http://arxiv.org/abs/2408.02741
Simulating quantum dynamics of lattice gauge theories (LGTs) is an exciting frontier in quantum science. Programmable quantum simulators based on neutral atom arrays are a promising approach to achieve this goal, since strong Rydberg blockade interac
Externí odkaz:
http://arxiv.org/abs/2408.02733
Autor:
Feldmeier, Patric, Fraser, Gordon
As games challenge traditional automated white-box test generators, the Neatest approach generates test suites consisting of neural networks that exercise the source code by playing the games. Neatest generates these neural networks using an evolutio
Externí odkaz:
http://arxiv.org/abs/2407.04985
Autor:
Manovitz, Tom, Li, Sophie H., Ebadi, Sepehr, Samajdar, Rhine, Geim, Alexandra A., Evered, Simon J., Bluvstein, Dolev, Zhou, Hengyun, Köylüoğlu, Nazli Uğur, Feldmeier, Johannes, Dolgirev, Pavel E., Maskara, Nishad, Kalinowski, Marcin, Sachdev, Subir, Huse, David A., Greiner, Markus, Vuletić, Vladan, Lukin, Mikhail D.
Understanding the collective quantum dynamics of nonequilibrium many-body systems is an outstanding challenge in quantum science. In particular, dynamics driven by quantum fluctuations are important for the formation of exotic quantum phases of matte
Externí odkaz:
http://arxiv.org/abs/2407.03249
Autor:
M. S. Nitschai, N. Neumayer, C. Clontz, M. Häberle, A. C. Seth, T.-O. Husser, S. Kamann, M. Alfaro-Cuello, N. Kacharov, A. Bellini, A. Dotter, S. Dreizler, A. Feldmeier-Krause, M. Latour, M. Libralato, A. P. Milone, R. Pechetti, G. van de Ven, K. Voggel, Daniel R. Weisz
Publikováno v:
The Astrophysical Journal, Vol 958, Iss 1, p 8 (2023)
Omega Centauri ( ω Cen) is the most massive globular cluster of the Milky Way and has been the focus of many studies that reveal the complexity of its stellar populations and kinematics. However, most previous studies have used photometric and spect
Externí odkaz:
https://doaj.org/article/5d6dbf496fb745fd946b94ea21a65b27
Publikováno v:
The Astrophysical Journal, Vol 948, Iss 1, p 65 (2023)
The Hydra I cluster offers an excellent opportunity to study and compare the relic old stellar populations in the core of its two brightest galaxies. In addition, the differing kinematics of the two galaxies allows a test of the local validity of gen
Externí odkaz:
https://doaj.org/article/2a91c8378b1b483aab590c7886bcbc46
The presence of young massive stars in the Galactic Centre (GC) raises questions about star formation near the black hole Sagittarius A* (Sgr A*). Additionally, the initial mass function (IMF) in this region appears different from the standard Salpet
Externí odkaz:
http://arxiv.org/abs/2406.04166
Autor:
Nitschai, M. S., Neumayer, N., Häberle, M., Clontz, C., Seth, A. C., Milone, A. P., Alfaro-Cuello, M., Bellini, A., Dreizler, S., Feldmeier-Krause, A., Husser, T. -O., Kacharov, N., Kamann, S., Latour, M., Libralato, M., van de Ven, G., Voggel, K., Wang, Z.
Publikováno v:
ApJ 970, 152 (2024)
$\omega$ Centauri, the most massive globular cluster in the Milky Way, has long been suspected to be the stripped nucleus of a dwarf galaxy that fell into the Galaxy a long time ago. There is considerable evidence for this scenario including a large
Externí odkaz:
http://arxiv.org/abs/2406.01688