Zobrazeno 1 - 10
of 46 678
pro vyhledávání: '"Reichert, As"'
Autor:
Agarwal, S., Aguilar, J. A., Alden, N., Ali, S., Allison, P., Betts, M., Besson, D., Bishop, A., Botner, O., Bouma, S., Buitink, S., Camphyn, R., Cataldo, M., Chiche, S., Clark, B. A., Coleman, A., Couberly, K., de Kockere, S., de Vries, K. D., Deaconu, C., Glaser, C., Glüsenkamp, T., Hallgren, A., Hallmann, S., Hanson, J. C., Hendricks, B., Henrichs, J., Heyer, N., Hornhuber, C., Hughes, K., Karg, T., Karle, A., Kelley, J. L., Kerr, C., Klein, C., Korntheuer, M., Kowalski, M., Kravchenko, I., Krebs, R., Lahmann, R., Latif, U., Laub, P., Liu, C. -H., Marsee, M. J., Meyers, Z. S., Mikhailova, M., Mulrey, K., Muzio, M., Nelles, A., Novikov, A., Nozdrina, A., Oberla, E., Oeyen, B., Polfrey, S., Punsuebsay, N., Pyras, L., Ravn, M., Reichert, M., Rix, J., Ryckbosch, D., Schlüter, F., Scholten, O., Seckel, D., Seikh, M. F. H., Smith, D., Stoffels, J., Terveer, K., Toscano, S., Tosi, D., Tutt, J., Broeck, D. J. Van Den, van Eijndhoven, N., Vieregg, A. G., Vijai, A., Welling, C., Williams, D. R., Windischhofer, P., Veale, J., Wissel, S., Young, R., Zink, A.
The Radio Neutrino Observatory in Greenland (RNO-G) is the first in-ice radio array in the northern hemisphere for the detection of ultra-high energy neutrinos via the coherent radio emission from neutrino-induced particle cascades within the ice. Th
Externí odkaz:
http://arxiv.org/abs/2411.12922
Autor:
Reichert, Tom, Aichelin, Jörg
The mechanism for generating directed and elliptic flow in heavy-ion collisions is investigated and quantified for the SIS18 and SIS100 energy regimes. The observed negative elliptic flow $v_2$, at midrapidity has been explained either via (in-plane)
Externí odkaz:
http://arxiv.org/abs/2411.12908
Autor:
Bumnedpan, Thiranat, Steinheimer, Jan, Reichert, Tom, Herold, Christoph, Limphirat, Ayut, Bleicher, Marcus
The UrQMD model with a density dependent equation of state, including a first-order phase transition, is used to study the time dependence of baryon number and proton number susceptibilities up to third order in heavy ion reactions of $E_{\mathrm{lab
Externí odkaz:
http://arxiv.org/abs/2411.08444
Autor:
Hehnle, Philipp, Reichert, Manfred
Different organisations often run similar digitised business processes to achieve their business goals. However, organisations often need to slightly adapt the business processes implemented in an information system in order to adopt them. Various ap
Externí odkaz:
http://arxiv.org/abs/2410.17689
We extend the theoretical approach which includes the dynamical and statistical stages for the description of the nucleosynthesis in central collisions of relativistic ions. Previously, this approach was successfully applied to describe experimental
Externí odkaz:
http://arxiv.org/abs/2410.17449
Autonomous systems, like vehicles or robots, require reliable, accurate, fast, resource-efficient, scalable, and low-latency trajectory predictions to get initial knowledge about future locations and movements of surrounding objects for safe human-ma
Externí odkaz:
http://arxiv.org/abs/2410.06905
The quantum molecular dynamics (QMD) part of the UrQMD model is extended to allow implementation of momentum dependent potentials from a parity doubling chiral mean field (CMF) model. Important aspects like energy conservation and effects on particle
Externí odkaz:
http://arxiv.org/abs/2410.01742
We suggest a new theoretical method to describe the baryon clusterization of nuclei in hadron-nucleus reactions. As an example we have explored the nuclei production in $\pi^-+C$ and $\pi^-+W$ collisions at p$_{lab}$=1.7 GeV by using the hybrid appro
Externí odkaz:
http://arxiv.org/abs/2409.19290
Resonance suppression during the hadronic stage from the FAIR to the intermediate RHIC energy regime
The energy and centrality dependence of the kaon resonance ratio $(K^{*0}+\Bar{K}^{*0})/(K^+ + K^-)$ is explored in the RHIC-BES and CBM-FAIR energy regime. To this aim, the Ultra-relativistic Quantum Molecular Dynamics (UrQMD) model is employed to s
Externí odkaz:
http://arxiv.org/abs/2409.08639
Autor:
Griffiths, Adam, Aloy, Miguel-Á, Hirschi, Raphael, Reichert, Moritz, Obergaulinger, Matrin, Whitehead, Emily E., Martinet, Sébastien, Esktröm, Sylvia, Meynet, Georges
Stars with initial mass above roughly 8 solar masses will evolve to form a core made of iron group elements at which point no further exothermic nuclear reactions between charged nuclei may prevent the core collapse. Electron captures, neutrino losse
Externí odkaz:
http://arxiv.org/abs/2408.03368