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  1. 5601
    “…We identify the mechanisms that operate in different regions of the pMSSM11 parameter space to bring the relic density of the lightest neutralino, $\tilde{\chi }^0_{1}$ , into the range indicated by cosmological data. In the fit including $(g-2)_\mu $ , coannihilations with $\tilde{\chi }^0_{2}$ and the Wino-like $\tilde{\chi }^\pm _{1}$ or with nearly-degenerate first- and second-generation sleptons are active, whereas coannihilations with the $\tilde{\chi }^0_{2}$ and the Higgsino-like $\tilde{\chi }^\pm _{1}$ or with first- and second-generation squarks may be important when the $(g-2)_\mu $ constraint is dropped. …”
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    Likelihood Analysis of the pMSSM11 in Light of LHC 13-TeV Data
  2. 5602
    por Ruggles, Clive
    Publicado 2015
    “…Thematic articles cover general themes such as cosmologies, calendars, navigation, orientations and alignments, and ancient perceptions of space and time. …”
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    Handbook of archaeoastronomy and ethnoastronomy
  3. 5603
    por Suchek, Stanislav
    Publicado 2019
    “…Dark Matter composes a significant part of the observable Universe. Despite a solid cosmological evidence, its nature, properties and interaction with the Standard Model sector is still to be unraveled. …”
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    Search for Dark Matter produced in association with hadronically decaying Standard Model bosons using $36~\textrm{fb}^{-1}$ of $pp$ collisions at the ATLAS detector
  4. 5604
    “…We explain the origin of this discrepancy, discuss its implications for the HI power spectrum Fisher matrix forecasts and argue that it motivates the HI field-level cosmological inference. On small scales in redshift space we use the difference between the model and the truth as a proxy for the Fingers-of-God effect. …”
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    Modeling HI at the field level
  5. 5605
    por Nicolás, Bernal Hernández
    Publicado 2017
    “…We discuss the constraints from collider searches and high-precision measurements, the cosmological constraints on the relic abundance of the neutralino candidate for the Dark Matter in the Universe and the gluino lifetime. …”
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    Théorie et Phénoménologie du MSSM avec des Scalaires Lourds
  6. 5606
    por Ade, P.A.R., Aghanim, N., Armitage-Caplan, C., Arnaud, M., Ashdown, M., Atrio-Barandela, F., Aumont, J., Baccigalupi, C., Banday, A.J., Barreiro, R.B., Battaner, E., Benabed, K., Benoît, A., Benoit-Lévy, A., Bernard, J. -P., Bersanelli, M., Bertincourt, B., Bielewicz, P., Bobin, J., Bock, J.J., Bond, J.R., Borrill, J., Bouchet, F.R., Boulanger, F., Bridges, M., Bucher, M., Burigana, C., Cardoso, J. -F., Catalano, A., Challinor, A., Chamballu, A., Chary, R. -R., Chen, X., Chiang, L. -Y, Chiang, H.C., Christensen, P.R., Church, S., Clements, D.L., Colombi, S., Colombo, L.P.L., Combet, C., Couchot, F., Coulais, A., Crill, B.P., Curto, A., Cuttaia, F., Danese, L., Davies, R.D., de Bernardis, P., de Rosa, A., de Zotti, G., Delabrouille, J., Delouis, J. -M., Désert, F. -X., Dickinson, C., Diego, J.M., Dole, H., Donzelli, S., Doré, O., Douspis, M., Dupac, X., Efstathiou, G., Enßlin, T.A., Eriksen, H.K., Filliard, C., Finelli, F., Forni, O., Frailis, M., Franceschi, E., Galeotta, S., Ganga, K., Giard, M., Giardino, G., Giraud-Héraud, Y., González-Nuevo, J., Górski, K.M., Gratton, S., Gregorio, A., Gruppuso, A., Hansen, F.K., Hanson, D., Harrison, D., Helou, G., Henrot-Versillé, S., Hernández-Monteagudo, C., Herranz, D., Hildebrandt, S.R., Hivon, E., Hobson, M., Holmes, W.A., Hornstrup, A., Hovest, W., Huffenberger, K.M., Jaffe, T.R., Jaffe, A.H., Jones, W.C., Juvela, M., Keihänen, E., Keskitalo, R., Kisner, T.S., Kneissl, R., Knoche, J., Knox, L., Kunz, M., Kurki-Suonio, H., Lagache, G., Lamarre, J. -M., Lasenby, A., Laureijs, R.J., Lawrence, C.R., Le Jeune, M., Lellouch, E., Leonardi, R., Leroy, C., Lesgourgues, J., Liguori, M., Lilje, P.B., Linden-Vørnle, M., López-Caniego, M., Lubin, P.M., Macías-Pérez, J.F., Maffei, B., Mandolesi, N., Maris, M., Marshall, D.J., Martin, P.G., Martínez-González, E., Masi, S., Matarrese, S., Matthai, F., Maurin, L., Mazzotta, P., McGehee, P., Meinhold, P.R., Melchiorri, A., Mendes, L., Mennella, A., Migliaccio, M., Mitra, S., Miville-Deschênes, M. -A., Moneti, A., Montier, L., Moreno, R., Morgante, G., Mortlock, D., Munshi, D., Murphy, J.A., Naselsky, P., Nati, F., Natoli, P., Netterfield, C.B., Nørgaard-Nielsen, H.U., Noviello, F., Novikov, D., Novikov, I., Osborne, S., Oxborrow, C.A., Paci, F., Pagano, L., Pajot, F., Paladini, R., Paoletti, D., Partridge, B., Pasian, F., Patanchon, G., Perdereau, O., Perotto, L., Perrotta, F., Piacentini, F., Piat, M., Pierpaoli, E., Pietrobon, D., Plaszczynski, S., Pointecouteau, E., Polenta, G., Ponthieu, N., Popa, L., Poutanen, T., Pratt, G.W., Prézeau, G., Prunet, S., Puget, J. -L., Rachen, J.P., Reinecke, M., Remazeilles, M., Renault, C., Ricciardi, S., Riller, T., Ristorcelli, I., Rocha, G., Rosset, C., Roudier, G., Rusholme, B., Santos, D., Savini, G., Shellard, E.P.S., Spencer, L.D., Starck, J. -L., Stolyarov, V., Stompor, R., Sudiwala, R., Sunyaev, R., Sureau, F., Sutton, D., Suur-Uski, A. -S., Sygnet, J. -F., Tauber, J.A., Tavagnacco, D., Techene, S., Terenzi, L., Tomasi, M., Tristram, M., Tucci, M., Umana, G., Valenziano, L., Valiviita, J., Van Tent, B., Vielva, P., Villa, F., Vittorio, N., Wade, L.A., Wandelt, B.D., Yvon, D., Zacchei, A., Zonca, A.
    Publicado 2013
    “…The lower frequencies (below 353 GHz) are calibrated using the cosmological microwave background dipole.One of the components of this anisotropy results from the orbital motion of the satellite in the Solar System, and is therefore time-variable. …”
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    Planck 2013 results. VIII. HFI photometric calibration and mapmaking
  7. 5607
    “…We analyze the impact of data from the full Run 1 of the LHC at 7 and 8 TeV on the CMSSM with [Formula: see text] and [Formula: see text] and the NUHM1 with [Formula: see text] , incorporating the constraints imposed by other experiments such as precision electroweak measurements, flavour measurements, the cosmological density of cold dark matter and the direct search for the scattering of dark matter particles in the LUX experiment. …”
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    Online Artículo Texto
    The CMSSM and NUHM1 after LHC Run 1
  8. 5608
    “…The detailed knowledge of the Milky Way radio emission is important to characterize galactic foregrounds masking extragalactic and cosmological signals. The update of the global sky models describing radio emissions over a very large spectral band requires high sensitivity experiments capable of observing large sky areas with long integration times. …”
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    Online Artículo Texto
    A high performance cost-effective digital complex correlator for an X-band polarimetry survey
  9. 5609
    “…The physics of star formation and the deposition of mass, momentum, and energy into the interstellar medium by massive stars (‘feedback’) are the main uncertainties in modern cosmological simulations of galaxy formation and evolution1, 2. …”
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    Online Artículo Texto
    Fast and inefficient star formation due to short-lived molecular clouds and rapid feedback
  10. 5610
    por Binney, James, Tremaine, Scott
    Publicado 2008
    Enlace del recurso
    Galactic dynamics
  11. 5611
    por Kozakai, Chihiro
    Publicado 2018
    “…SUSY models which predict that the Lightest SUSY Particle (LSP) is the partner of the neutral W boson (wino) are especially attractive because they are compatible with the cosmological observations. Such models also predict that the second lightest SUSY particle is the charged wino whose mass is nearly degenerated to the neutral wino mass. …”
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    Search for Long-lived Chargino via Gluino Pair Production in pp Collisions at √s = 13 TeV with the ATLAS Detector
  12. 5612
    por De Vries, Jacco Andreas
    Publicado 2018
    “…This has lead to the ambition to explain large-scale cosmological observations starting from the very small scale of particle interactions. …”
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    Asymmetries in mixed beauty decays
  13. 5613
    por Mahbubani, Rakhi, Zurita, José
    Publicado 2018
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    Probing compressed dark sectors at 100 TeV in the dileptonic mono-Z channel
  14. 5614
    por Gonzalo, Eduardo
    Publicado 2019
    “…The conjecture has far reaching consequences and applies to several interesting physical systems: i) Among chaotic inflation potentials only those asymptotically linear may survive. ii) If applied to the radion of the circle compactification of the Standard Model to 3D with Dirac neutrinos, the constraint implies that the 4D cosmological constant scale must be larger than the mass of the lightest neutrino, which must be in normal hierarchy. …”
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    A Strong Scalar Weak Gravity Conjecture and Some Implications
  15. 5615
    por Balbi, Amedeo
    Publicado 2007
    “…Molte delle informazioni codificate nella radiazione cosmica di fondo sono state impresse dal sovrapporsi di onde acustiche presenti nell’Universo primordiale: una "musica" del Big Bang, che i cosmologi hanno tentato per anni di ricostruire, usando tecniche analoghe a quelle che permettono di distinguere il suono di diversi strumenti musicali. …”
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    La musica del big bang: come la radiazione cosmica di fondo ci ha svelato i segreti dell’universo
  16. 5616
    por Kirsanov, Mikhail
    Publicado 2019
    “…The analysis of these data is not yet finished, although the sensitivity is already estimated as about 3 times better than in the previously published result on the 2016 data.For models considering scalar and fermionic thermal Dark Matter interacting with the visible sector through the vector portal the experiment starts to be sensitive to the regions of the dark-matter parameter predicted from the cosmological observations of Dark Matter.We also report the improved results on a direct search for a new 16.7 MeV boson (X) which could explain the anomalous excess of e+e- pairs observed in the excited 8Be* nucleus decays. …”
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    Recent results of the NA64 experiment at the CERN SPS
  17. 5617
    por Genest, Marie-Helene
    Publicado 2007
    “…Using WMAP (Wilkinson Microwave Anisotropy Probe) results on cosmic microwave background anisotropies, limits on the dark matter cosmological density can be set. These boundaries can then be converted in limits on the supersymmetric parameters, thus constraining the possible models of neutralino. …”
    Enlace del recurso
    Recherche du neutralino avec les détecteurs ATLAS et PICASSO
  18. 5618
    por Irastorza, Igor G, Armengaud, E., Avignone, F. T., Betz, M., Brax, P., Brun, P., Cantatore, G., Carmona, J. M., Carosi, G. P., Caspers, F., Caspi, S., Cetin, S. A., Chelouche, D., Christensen, F. E., Dael, A., Dafni, T., Davenport, M., Derbin, A.V., Desch, K., Diago, A., Dobrich, B. D., Dratchnev, I., Dudarev, A., Eleftheriadis, C., Fanourakis, G., Ferrer-Ribas, E., Galan, J., Garcia, J. A., Garza, J. G., Geralis, T., Gimeno, B., Giomataris, I., Gninenko, S., Gomez, H., Gonzalez-Diaz, D., Guendelman, E., Hailey, C. J., Hiramatsu, T., Hoffmann, D. H. H., Horns, D., Iguaz, F. J., Isern, J., Imai, K., Jakobsen, A. C., Jaeckel, J., Jakovcic, K., Kaminski, J., Kawasaki, M., Karuza, M., Krcmar, M., Kousouris, K., Krieger, C., Lakic, B., Limousin, O., Lindner, A., Liolios, A., Luzon, G., Matsuki, S., Muratova, V. N., Nones, C., Ortega, I., Papaevangelou, T., Pivovaroff, M. J., Raffelt, G., Redondo, J., Ringwald, A., Russenschuck, S., Ruz, J., Saikawa, K., Savvidis, I., Sekiguchi, T., Semertzidis, Y. K., Shilon, I., Sikivie, P., Silva, H., Kate, H. ten, Tomas, A., Troitsky, S., Vafeiadis, T., van Bibber, K., Vedrine, P., Villar, J. A., Vogel, J. K., Walckiers, L., Weltman, A., Wester, W., Yildiz, S. C., Zioutas, K.
    Publicado 2013
    “…At the very least it will firmly exclude a large region of this space of high cosmological and astrophysical relevance. In particular it will probe a large fraction of the high mass part (1 meV to 1 eV) of the QCD axion allowed window. …”
    Enlace del recurso
    The International Axion Observatory IAXO. Letter of Intent to the CERN SPS committee
  19. 5619
    por Colombo, Tommaso
    Publicado 2013
    “…Nevertheless, the Standard Model is necessarily an incomplete theory as it does neither account for gravity, nor provide an explanation to cosmological problems like the apparent existence of dark matter and the observed matter-antimatter asymmetry. …”
    Enlace del recurso
    Data-flow performance optimisation of the ATLAS data acquisition system
  20. 5620
    por Beauchemin , Pierre-Hugues
    Publicado 2017
    “…However, given, for example, the Supersyminetric Large Extra Dimension (SLED) scenario, which can provide a framework for a solution to the cosmological constant problem, the D-dimensional Planck scale is approximately fixed and so is the graviton production rate. …”
    Enlace del recurso
    Phenomenology of Bulk Scalar Production at the LHC
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