Zobrazeno 1 - 10
of 8 509
pro vyhledávání: '"MUELLER B"'
Publikováno v:
Clinical Ophthalmology, Vol Volume 18, Pp 69-78 (2024)
Camila Albo,1 Taj Nasser,2 David Thomas Szynkarski,2 Ngoc Nguyen,3 Brett Mueller,2,4 Lauren Libfraind,2 Gregory Parkhurst2 1Department of Ophthalmology, University of Texas Health San Antonio, San Antonio, TX, USA; 2Department of Ophthalmology, Parkh
Externí odkaz:
https://doaj.org/article/7ca282b5bd644ed48cf533d3da39043d
Autor:
Burgemeister S, Kutz A, Conca A, Holler T, Haubitz S, Huber A, Buergi U, Mueller B, Schuetz P
Publikováno v:
Open Access Emergency Medicine, Vol Volume 9, Pp 97-106 (2017)
Susanne Burgemeister,1 Alexander Kutz,1 Antoinette Conca,2 Thomas Holler,3 Sebastian Haubitz,1 Andreas Huber,4 Ulrich Buergi,5 Beat Mueller,1 Philipp Schuetz1 1University Department of Internal Medicine, Medical Faculty of the University of Basel, Ka
Externí odkaz:
https://doaj.org/article/2e74da67df5844c4ae127179dfb2e94e
Autor:
Müller, B.
Fallback in core-collapse supernova explosions is potentially of significant importance for the birth spins of neutron stars and black holes. It has recently been pointed out that the angular momentum imparted onto a compact remnant by fallback mater
Externí odkaz:
http://arxiv.org/abs/2308.08312
Autor:
Linek, J., Wyszynski, M., Müller, B., Korinski, D., Milošević, M. V., Kleiner, R., Koelle, D.
We investigate the coupling factor $\phi_\mu$ that quantifies the magnetic flux $\Phi$ per magnetic moment $\mu$ of a point-like magnetic dipole that couples to a superconducting quantum interference device (SQUID). Representing the dipole by a curre
Externí odkaz:
http://arxiv.org/abs/2307.05724
Autor:
Arslandok, M., Bass, S. A., Baty, A. A., Bautista, I., Beattie, C., Becattini, F., Bellwied, R., Berdnikov, Y., Berdnikov, A., Bielcik, J., Blair, J. T., Bock, F., Boimska, B., Bossi, H., Caines, H., Chen, Y., Chien, Y. -T., Chiu, M., Connors, M. E., Csanád, M., da Silva, C. L., Dash, A. P., David, G., Dehmelt, K., Dexheimer, V., Dong, X., Drees, A., Du, L., Durham, J. M., Ehlers, R. J., Elfner, H., Evdokimov, O., Finger, M., Finger Jr., M., Frantz, J., Frawley, A. D., Gale, C., Geurts, F., Gonzalez, V., Grau, N., Greene, S. V., Grossberndt, S. K., Hachiya, T., He, X., Heinz, U., Hong, B., Humanic, T. J., Ivanishchev, D., Jacak, B. V., Jahan, J., Jeon, S., Jheng, H. R., Jia, J., Judd, E. G., Kapusta, J. I., Karpenko, I., Khachatryan, V., Kharzeev, D. E., Kim, M., Kimelman, B., Klay, J. L., Klein, S. R., Knospe, A. G., Koch, V., Kotov, D, Krintiras, G. K., Elayavalli, R. Kunnawalkam, Kuo, C. M., Lajoie, J. G., Lee, Y. -J., Li, W., Liao, J., Likmeta, I., Lim, S. H., Liu, M. X., Loizides, C., Longo, R., Luo, X., Luzum, M., Ma, R., Majumder, A., Mak, S., Markert, C., Mehtar-Tani, Y., Mignerey, A. C., Minafra, N., Morrison, D. P., Mueller, B., Nagle, J. L., Narde, A., Nattrass, C. E., Niida, T., Noronha, J., Noronha-Hostler, J., Nouicer, R., Novitzky, N., O'Brien, E., Odyniec, G., Okorokov, V. A., Osborn, J. D., Paquet, J. -F., Park, S., Parotto, P., Perepelitsa, D. V., Petreczky, P., Pinkenburg, C., Praszalowicz, M., Pruneau, C., Putschke, J., Ramasubramanian, N. V., Rapp, R., Ratti, C., Read, K. F., Teles, P. Rebello, Reed, R., Rinn, T., Roland, G., Rosati, M., Royon, C., Ruan, L., Sakaguchi, T., Salur, S., Sarsour, M., Menon, A. S., Schenke, B., Schmidt, N. V., Schmier, A., Schäfer, T., Seger, J., Seto, R., Sheibani, Oveis, Shen, C., Shi, Z., Shulga, E., Sickles, A. M., Singh, M., Singh, B. K., Smirnov, N., Smith, K. L., Song, H., Soudi, I., Leiton, A. G. Stahl, Steinberg, P., Stephanov, M., Strickland, M., Sumbera, M., Cerci, D. Sunar, Tachibana, Y., Tang, A. H., Takaki, D. Tapia, Teaney, D., Thomas, D., Timmins, A. R., Tribedy, P., Tu, Z., Tuo, S., Rueda, O. V., Velkovska, J., Venugopalan, R., Videbæk, F., Voloshin, S. A., Vovchenko, V., Vujanovic, G., Wang, X., Wang, F., Wang, X. -N., Weyhmiller, S., Xie, W., Xu, N., Yang, Y., Yao, X., Ye, Z., Yee, H. -U., Zajc, W. A.
Hot QCD physics studies the nuclear strong force under extreme temperature and densities. Experimentally these conditions are achieved via high-energy collisions of heavy ions at the Relativistic Heavy Ion Collider (RHIC) and the Large Hadron Collide
Externí odkaz:
http://arxiv.org/abs/2303.17254
Autor:
Achenbach, P., Adhikari, D., Afanasev, A., Afzal, F., Aidala, C. A., Al-bataineh, A., Almaalol, D. K., Amaryan, M., Androić, D., Armstrong, W. R., Arratia, M., Arrington, J., Asaturyan, A., Aschenauer, E. C., Atac, H., Avakian, H., Averett, T., Gayoso, C. Ayerbe, Bai, X., Barish, K. N., Barnea, N., Basar, G., Battaglieri, M., Baty, A. A., Bautista, I., Bazilevsky, A., Beattie, C., Behera, S. C., Bellini, V., Bellwied, R., Benesch, J. F., Benmokhtar, F., Bernardes, C. A., Bernauer, J. C., Bhatt, H., Bhatta, S., Boer, M., Boettcher, T. J., Bogacz, S. A., Bossi, H. J., Brandenburg, J. D., Brash, E. J., Briceño, R. A., Briscoe, W. J., Brodsky, S. J., Brown, D. A., Burkert, V. D., Caines, H., Cali, I. A., Camsonne, A., Carman, D. S., Caylor, J., Cerci, S., Llatas, M. Chamizo, Chatterjee, S., Chen, J. P., Chen, Y., Chen, Y. -C., Chien, Y. -T., Chou, P. -C., Chu, X., Chudakov, E., Cline, E., Cloët, I. C., Cole, P. L., Connors, M. E., Constantinou, M., Cosyn, W., Dusa, S. Covrig, Cruz-Torres, R., D'Alesio, U., da Silva, C., Davoudi, Z., Dean, C. T., Dean, D. J., Demarteau, M., Deshpande, A., Detmold, W., Deur, A., Devkota, B. R., Dhital, S., Diefenthaler, M., Dobbs, S., Döring, M., Dong, X., Dotel, R., Dow, K. A., Downie, E. J., Drachenberg, J. L., Dumitru, A., Dunlop, J. C., Dupre, R., Durham, J. M., Dutta, D., Edwards, R. G., Ehlers, R. J., Fassi, L. El, Elaasar, M., Elouadrhiri, L., Engelhardt, M., Ent, R., Esumi, S., Evdokimov, O., Eyser, O., Fanelli, C., Fatemi, R., Fernando, I. P., Flor, F. A., Fomin, N., Frawley, A. D., Frederico, T., Fries, R. J., Gal, C., Gamage, B. R., Gamberg, L., Gao, H., Gaskell, D., Geurts, F., Ghandilyan, Y., Ghimire, N., Gilman, R., Gleason, C., Gnanvo, K., Gothe, R. W., Greene, S. V., Grießhammer, H. W., Grossberndt, S. K., Grube, B., Hackett, D. C., Hague, T. J., Hakobyan, H., Hansen, J. -O., Hatta, Y., Hattawy, M., Havener, L. B., Hen, O., Henry, W., Higinbotham, D. W., Hobbs, T. J., Hodges, A. M., Holmstrom, T., Hong, B., Horn, T., Howell, C. R., Huang, H. Z., Huang, M., Huang, S., Huber, G. M., Hyde, C. E., Isupov, E. L., Jacobs, P. M., Jalilian-Marian, J., Jentsch, A., Jheng, H., Ji, C. -R., Ji, X., Jia, J., Jones, D. C., Jones, M. K., Kalantarians, N., Kalicy, G., Kang, Z. B., Karthein, J. M., Keller, D., Keppel, C., Khachatryan, V., Kharzeev, D. E., Kim, H., Kim, M., Kim, Y., King, P. M., Kinney, E., Klein, S. R., Ko, H. S., Koch, V., Kohl, M., Kovchegov, Y. V., Krintiras, G. K., Kubarovsky, V., Kuhn, S. E., Kumar, K. S., Kutz, T., Lajoie, J. G., Lauret, J., Lavrukhin, I., Lawrence, D., Lee, J. H., Lee, K., Lee, S., Lee, Y. -J., Li, S., Li, W., Li, Xiaqing, Li, Xuan, Liao, J., Lin, H. -W., Lisa, M. A., Liu, K. -F., Liu, M. X., Liu, T., Liuti, S., Liyanage, N., Llope, W. J., Loizides, C., Longo, R., Lorenzon, W., Lunkenheimer, S., Luo, X., Ma, R., McKinnon, B., Meekins, D. G., Mehtar-Tani, Y., Melnitchouk, W., Metz, A., Meyer, C. A., Meziani, Z. -E., Michaels, R., Michel, J. K. L., Milner, R. G., Mkrtchyan, H., Mohanmurthy, P., Mohanty, B., Mokeev, V. I., Moon, D. H., Mooney, I. A., Morningstar, C., Morrison, D. P., Müller, B., Mukherjee, S., Mulligan, J., Camacho, C. Munoz, Quijada, J. A. Murillo, Murray, M. J., Nadeeshani, S. A., Nadel-Turonski, P., Nam, J. D., Nattrass, C. E., Nijs, G., Noronha, J., Noronha-Hostler, J., Novitzky, N., Nycz, M., Olness, F. I., Osborn, J. D., Pak, R., Pandey, B., Paolone, M., Papandreou, Z., Paquet, J. -F., Park, S., Paschke, K. D., Pasquini, B., Pasyuk, E., Patel, T., Patton, A., Paudel, C., Peng, C., Peng, J. C., Da Costa, H. Pereira, Perepelitsa, D. V., Peters, M. J., Petreczky, P., Pisarski, R. D., Pitonyak, D., Ploskon, M. A., Posik, M., Poudel, J., Pradhan, R., Prokudin, A., Pruneau, C. A., Puckett, A. J. R., Pujahari, P., Putschke, J., Pybus, J. R., Qiu, J. -W., Rajagopal, K., Ratti, C., Read, K. F., Reed, R., Richards, D. G., Riedl, C., Ringer, F., Rinn, T., West, J. Rittenhouse, Roche, J., Rodas, A., Roland, G., Romero-López, F., Rossi, P., Rostomyan, T., Ruan, L., Ruimi, O. M., Saha, N. R., Sahoo, N. R., Sakaguchi, T., Salazar, F., Salgado, C. W., Salmè, G., Salur, S., Santiesteban, S. N., Sargsian, M. M., Sarsour, M., Sato, N., Satogata, T., Sawada, S., Schäfer, T., Scheihing-Hitschfeld, B., Schenke, B., Schindler, S. T., Schmidt, A., Seidl, R., Shabestari, M. H., Shanahan, P. E., Shen, C., Sheng, T. -A., Shepherd, M. R., Sickles, A. M., Sievert, M. D., Smith, K. L., Song, Y., Sorensen, A., Souder, P. A., Sparveris, N., Srednyak, S., Leiton, A. G. Stahl, Stasto, A. M., Steinberg, P., Stepanyan, S., Stephanov, M., Stevens, J. R., Stewart, D. J., Stewart, I. W., Stojanovic, M., Strakovsky, I., Strauch, S., Strickland, M., Cerci, D. Sunar, Suresh, M., Surrow, B., Syritsyn, S., Szczepaniak, A. P., Tadepalli, A. S., Tang, A. H., Takaki, J. D. Tapia, Tarnowsky, T. J., Tawfik, A. N., Taylor, M. I., Tennant, C., Thiel, A., Thomas, D., Tian, Y., Timmins, A. R., Tribedy, P., Tu, Z., Tuo, S., Ullrich, T., Umaka, E., Upton, D. W., Vary, J. P., Velkovska, J., Venugopalan, R., Vijayakumar, A., Vitev, I., Vogelsang, W., Vogt, R., Vossen, A., Voutier, E., Vovchenko, V., Walker-Loud, A., Wang, F., Wang, J., Wang, X., Wang, X. -N., Weinstein, L. B., Wenaus, T. J., Weyhmiller, S., Wissink, S. W., Wojtsekhowski, B., Wong, C. P., Wood, M. H., Wunderlich, Y., Wyslouch, B., Xiao, B. W., Xie, W., Xiong, W., Xu, N., Xu, Q. H., Xu, Z., Yaari, D., Yao, X., Ye, Z., Ye, Z. H., Yero, C., Yuan, F., Zajc, W. A., Zhang, C., Zhang, J., Zhao, F., Zhao, Y., Zhao, Z. W., Zheng, X., Zhou, J., Zurek, M.
Publikováno v:
Nucl.Phys.A 1047 (2024) 122874
This White Paper presents the community inputs and scientific conclusions from the Hot and Cold QCD Town Meeting that took place September 23-25, 2022 at MIT, as part of the Nuclear Science Advisory Committee (NSAC) 2023 Long Range Planning process.
Externí odkaz:
http://arxiv.org/abs/2303.02579
Fallback supernovae and the collapsar scenario for long-gamma ray burst and hypernovae have received considerable interest as pathways to black-hole formation and extreme transient events. Consistent simulations of these scenarios require a general r
Externí odkaz:
http://arxiv.org/abs/2210.12939
Publikováno v:
A&A 668, A46 (2022)
Context. The gas and ice-grain chemistry of the pre-stellar core L1544 has been the subject of several observations and modelling studies conducted in the past years. The chemical composition of the ice mantles reflects the environmental physical cha
Externí odkaz:
http://arxiv.org/abs/2208.07672
Autor:
Gavdush, A. A., Kruczkiewicz, F., Giuliano, B. M., Müller, B., Komandin, G. A., Grassi, T., Theulé, P., Zaytsev, K. I., Ivlev, A. V., Caselli, P.
Publikováno v:
A&A 667, A49 (2022)
Context: Broadband optical constants of astrophysical ice analogues in the infrared (IR) and terahertz (THz) ranges are required for modeling the dust continuum emission and radiative transfer in dense and cold regions, where thick icy mantles are fo
Externí odkaz:
http://arxiv.org/abs/2207.11052
Publikováno v:
In Cement and Concrete Research December 2024 186