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1241por Tolley, Emma“…Dark matter could be produced at the LHC if it interacts weakly with the Standard Model. …”
Publicado 2018
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1242por Briard, François“…Soirée Dark Matter day au globe de l'innovation au CERN 2018…”
Publicado 2018
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1243“…A global effort is under way to carry out a complete search for high-mass dark-matter particles using an experiment called DarkSide-20k and its successor, which rely on novel liquid-argon technologies.…”
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1244por Mazini, Rachid“…This talk presented recent results for searches of Dark Matter signals with the ATLAS detector at the LHC. …”
Publicado 2018
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1245
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1246
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1247por Ng, Ying Wun Yvonne“…Recent results on Dark matter searches…”
Publicado 2018
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1248
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1249
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1250
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1251
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1252
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1253por Bechtol, Keith, Drlica-Wagner, Alex, Abazajian, Kevork N., Abidi, Muntazir, Adhikari, Susmita, Ali-Haïmoud, Yacine, Annis, James, Ansarinejad, Behzad, Armstrong, Robert, Asorey, Jacobo, Baccigalupi, Carlo, Banerjee, Arka, Banik, Nilanjan, Bennett, Charles, Beutler, Florian, Bird, Simeon, Birrer, Simon, Biswas, Rahul, Biviano, Andrea, Blazek, Jonathan, Boddy, Kimberly K., Bonaca, Ana, Borrill, Julian, Bose, Sownak, Bovy, Jo, Frye, Brenda, Brooks, Alyson M., Buckley, Matthew R., Buckley-Geer, Elizabeth, Bulbul, Esra, Burchat, Patricia R., Burgess, Cliff, Calore, Francesca, Caputo, Regina, Castorina, Emanuele, Chang, Chihway, Chapline, George, Charles, Eric, Chen, Xingang, Clowe, Douglas, Cohen-Tanugi, Johann, Comparat, Johan, Croft, Rupert A.C., Cuoco, Alessandro, Cyr-Racine, Francis-Yan, D'Amico, Guido, Davis, Tamara M., Dawson, William A., de la Macorra, Axel, Di Valentino, Eleonora, Rivero, Ana Díaz, Digel, Seth, Dodelson, Scott, Doré, Olivier, Dvorkin, Cora, Eckner, Christopher, Ellison, John, Erkal, Denis, Farahi, Arya, Fassnacht, Christopher D., Ferreira, Pedro G., Flaugher, Brenna, Foreman, Simon, Friedrich, Oliver, Frieman, Joshua, García-Bellido, Juan, Gawiser, Eric, Gerbino, Martina, Giannotti, Maurizio, Gill, Mandeep S.S., Gluscevic, Vera, Golovich, Nathan, Gontcho, Satya Gontcho A., Gonzalez-Morales, Alma X., Grin, Daniel, Gruen, Daniel, Hearin, Andrew P., Hendel, David, Hezaveh, Yashar D., Hirata, Christopher M., Hlozek, Renee, Horiuchi, Shunsaku, Jain, Bhuvnesh, Jee, M. James, Jeltema, Tesla E., Kamionkowski, Marc, Kaplinghat, Manoj, Keeley, Ryan E., Keeton, Charles R., Khatri, Rishi, Koposov, Sergey E., Koushiappas, Savvas M., Kovetz, Ely D., Lahav, Ofer, Lam, Casey, Lee, Chien-Hsiu, Li, Ting S., Liguori, Michele, Lin, Tongyan, Lisanti, Mariangela, LoVerde, Marilena, Lu, Jessica R., Mandelbaum, Rachel, Mao, Yao-Yuan, McDermott, Samuel D., McNanna, Mitch, Medford, Michael, Meerburg, P. Daniel, Meyer, Manuel, Mirbabayi, Mehrdad, Mishra-Sharma, Siddharth, Marc, Moniez, More, Surhud, Moustakas, John, Munoz, Julian B., Murgia, Simona, Myers, Adam D., Nadler, Ethan O., Necib, Lina, Newburgh, Laura, Newman, Jeffrey A., Nord, Brian, Nourbakhsh, Erfan, Nuss, Eric, O'Connor, Paul, Pace, Andrew B., Padmanabhan, Hamsa, Palmese, Antonella, Peiris, Hiranya V., Peter, Annika H.G., Piacentni, Francesco, Plazas, Andres, Polin, Daniel A., Prakash, Abhishek, Prescod-Weinstein, Chanda, Read, Justin I., Ritz, Steven, Robertson, Brant E., Rose, Benjamin, Rosenfeld, Rogerio, Rossi, Graziano, Samushia, Lado, Sanchez, Javier, Sanchez-Conde, Miguel A., Schaan, Emmanuel, Sehgal, Neelima, Senatore, Leonardo, Seo, Hee-Jong, Shafieloo, Arman, Shan, Huanyuan, Shipp, Nora, Simon, Joshua D., Simon, Sara, Slatyer, Tracy R., Slosar, Anze, Sridhar, Srivatsan, Stebbins, Albert, Straniero, Oscar, Strigari, Louis E., Tait, Tim M.P., Tollerud, Erik, Troxel, M.A., Tyson, J. Anthony, Uhlemann, Cora, Urenna-Lopez, L. Arturo, Verma, Aprajita, Vilalta, Ricardo, Walter, Christopher W., Wang, Mei-Yu, Watson, Scott, Wechsler, Risa H., Wittman, David, Xu, Weishuang, Yanny, Brian, Young, Sam, Yu, Hai-Bo, Zaharijas, Gabrijela, Zentner, Andrew R., Zuntz, Joe“…Astrophysical observations currently provide the only robust, empirical measurements of dark matter. In the coming decade, astrophysical observations will guide other experimental efforts, while simultaneously probing unique regions of dark matter parameter space. …”
Publicado 2019
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1254
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1255por Balunas, William Keaton“…The presence of a non-baryonic dark matter component in the Universe is inferred from the observation of its gravitational interaction. …”
Publicado 2019
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1256por Balunas, William Keaton“…The presence of a non-baryonic dark matter component in the Universe is inferred from the observation of its gravitational interaction. …”
Publicado 2019
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1257por Rifki, Othmane“…The presence of a non-baryonic dark matter (DM) component in the Universe is inferred from the observation of its gravitational interaction. …”
Publicado 2019
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1258por Carlson, Benjamin Taylor“…Dark matter could be produced at the LHC if it interacts weakly with the Standard Model. …”
Publicado 2019
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1259por Farina, Edoardo Maria“…The presence of a non-baryonic dark matter (DM) component in the Universe is inferred from the observation of its gravitational interaction. …”
Publicado 2019
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1260por Vanden Broeck, Renilde“…The Dark Matter hypothesis : according to the standard cosmological model that describes the composition and evolution of the Universe, the Lambda Cold Dark Matter model, only 5% is formed of ordinary matter. 95% is due to the existence of dark matter and dark energy.…”
Publicado 2019
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