Zobrazeno 1 - 10
of 513
pro vyhledávání: '"Mueller, Simon A."'
Revealing the internal composition and structure of giant planets is fundamental for understanding planetary formation. However, the bulk composition can only be inferred through interior models. As a result, advancements in modelling aspects are ess
Externí odkaz:
http://arxiv.org/abs/2410.21382
Publikováno v:
A&A 690, A105 (2024)
We present improved empirical density profiles of Uranus and interpret them in terms of their temperature and composition using a new random algorithm. The algorithm to determine the temperature and composition is agnostic with respect to the tempera
Externí odkaz:
http://arxiv.org/abs/2408.10336
Publikováno v:
A&A 689, A15 (2024)
Phase separation between hydrogen and helium at high pressures and temperatures leads to the rainout of helium in the deep interiors of Jupiter and Saturn. This process, also known as "helium rain", affects their long-term evolution. Therefore, model
Externí odkaz:
http://arxiv.org/abs/2407.11120
Autor:
Müller, Simon, Nevolianis, Thomas, Garcia-Ratés, Miquel, Riplinger, Christoph, Leonhard, Kai, Smirnova, Irina
The accurate prediction of solvation free energies is critical for understanding various phenomena in the liquid phase, including reaction rates, equilibrium constants, activity coefficients, and partition coefficients. Despite extensive research, pr
Externí odkaz:
http://arxiv.org/abs/2407.03434
Autor:
Hacker, Alejandro, Díaz, Rodrigo F., Armstrong, David J., Fernández, Jorge Fernández, Müller, Simon, Delgado-Mena, Elisa, Sousa, Sérgio G., Adibekyan, Vardan, Stassun, Keivan G., Collins, Karen A., Yee, Samuel W., Bayliss, Daniel, Bieryla, Allyson, Bouchy, François, Butler, R. Paul, Crane, Jeffrey D., Dumusque, Xavier, Hartman, Joel D., Helled, Ravit, Jenkins, Jon, Keniger, Marcelo Aron F., Lewis, Hannah, Lillo-Box, Jorge, Lund, Michael B., Nielsen, Louise D., Osborn, Ares, Osip, David, Paegert, Martin, Radford, Don J., Santos, Nuno C., Seager, Sara, Shectman, Stephen A., Srdoc, Gregor, Strøm, Paul A., Tan, Thiam-Guan, Teske, Johanna K., Vezie, Michael, Watanabe, David, Watkins, Cristilyn N., Wheatley, Peter J., Winn, Joshua N., Wohler, Bill, Ziegler, Carl
We report the discovery of two transiting planets detected by the Transiting Exoplanet Survey Satellite (TESS), TOI-2374 b and TOI-3071 b, orbiting a K5V and an F8V star, respectively, with periods of 4.31 and 1.27 days, respectively. We confirm and
Externí odkaz:
http://arxiv.org/abs/2406.12996
Autor:
Grigorash, Daria, Müller, Simon, Paricaud, Patrice, Stenby, Erling H., Smirnova, Irina, Yan, Wei
The COSMO-RS (Conductor-like Screening Model for Real Solvents) is a predictive thermodynamic model that has found diverse applications in various domains like chemical engineering, environmental chemistry, nanotechnology, material science, and biote
Externí odkaz:
http://arxiv.org/abs/2406.05244
Autor:
Müller, Simon, Helled, Ravit
Updated formation and structure models of Jupiter predict a metal-poor envelope. This is at odds with the two to three times solar metallicity measured by the Galileo probe. Additionally, Juno data imply that water and ammonia are enriched. Here we e
Externí odkaz:
http://arxiv.org/abs/2403.16273
Autor:
Kanodia, Shubham, Cañas, Caleb I., Mahadevan, Suvrath, Ford, Eric B., Helled, Ravit, Anderson, Dana E., Boss, Alan, Cochran, William D., Delamer, Megan, Han, Te, Libby-Roberts, Jessica E., Lin, Andrea S. J., Müller, Simon, Robertson, Paul, Stefánsson, Guðmundur, Teske, Johanna
Recent discoveries of transiting giant exoplanets around M-dwarf stars (GEMS), aided by the all-sky coverage of TESS, are starting to stretch theories of planet formation through the core-accretion scenario. Recent upper limits on their occurrence su
Externí odkaz:
http://arxiv.org/abs/2402.04946
Uranus' bulk composition remains unknown. Although there are clear indications that Uranus' interior is not fully convective, and therefore has a non-adiabatic temperature profile, many interior models continue to assume an adiabatic interior. In thi
Externí odkaz:
http://arxiv.org/abs/2401.11769
Publikováno v:
Fluid Phase Equilibria 586 (November 1, 2024): 114182
Stimuli-responsive lyogels are considered to be smart materials due to their capability of undergoing significant macroscopic changes in response to external triggers. Due to their versatile and unique properties, smart lyogels exhibit great potentia
Externí odkaz:
http://arxiv.org/abs/2401.07592