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  1. 161
    por Ade, P.A.R., Aghanim, N., Arnaud, M., Arroja, F., Ashdown, M., Aumont, J., Baccigalupi, C., Ballardini, M., Banday, A.J., Barreiro, R.B., Bartolo, N., Battaner, E., Benabed, K., Benoit, A., Benoit-Levy, A., Bernard, J.P., Bersanelli, M., Bielewicz, P., Bonaldi, A., Bonavera, L., Bond, J.R., Borrill, J., Bouchet, F.R., Boulanger, F., Bucher, M., Burigana, C., Butler, R.C., Calabrese, E., Cardoso, J.F., Catalano, A., Challinor, A., Chamballu, A., Chary, R.R., Chiang, H.C., Christensen, P.R., Church, S., Clements, D.L., Colombi, S., Colombo, L.P.L., Combet, C., Contreras, D., Couchot, F., Coulais, A., Crill, B.P., Curto, A., Cuttaia, F., Danese, L., Davies, R.D., Davis, R.J., de Bernardis, P., de Rosa, A., de Zotti, G., Delabrouille, J., Desert, F.X., Diego, J.M., Dole, H., Donzelli, S., Dore, O., Douspis, M., Ducout, A., Dupac, X., Efstathiou, G., Elsner, F., Ensslin, T.A., Eriksen, H.K., Fergusson, J., Finelli, F., Forni, O., Frailis, M., Fraisse, A.A., Franceschi, E., Frejsel, A., Frolov, A., Galeotta, S., Galli, S., Ganga, K., Gauthier, C., Giard, M., Giraud-Heraud, Y., Gjerlow, E., Gonzalez-Nuevo, J., Gorski, K.M., Gratton, S., Gregorio, A., Gruppuso, A., Gudmundsson, J.E., Hamann, J., Handley, W., Hansen, F.K., Hanson, D., Harrison, D.L., Henrot-Versille, S., Hernandez-Monteagudo, C., Herranz, D., Hildebrandt, S.R., Hivon, E., Hobson, M., Holmes, W.A., Hornstrup, A., Hovest, W., Huang, Z., Huffenberger, K.M., Hurier, G., Jaffe, A.H., Jaffe, T.R., Jones, W.C., Juvela, M., Keihanen, E., Keskitalo, R., Kim, J., Kisner, T.S., Kneissl, R., Knoche, J., Kunz, M., Kurki-Suonio, H., Lagache, G., Lahteenmaki, A., Lamarre, J.M., Lasenby, A., Lattanzi, M., Lawrence, C.R., Leonardi, R., Lesgourgues, J., Levrier, F., Lewis, A., Liguori, M., Lilje, P.B., Linden-Vornle, M., Lopez-Caniego, M., Lubin, P.M., Ma, Y.Z., Macias-Perez, J.F., Maggio, G., Maino, D., Mandolesi, N., Mangilli, A., Martin, P.G., Martinez-Gonzalez, E., Masi, S., Matarrese, S., Mazzotta, P., McGehee, P., Meinhold, P.R., Melchiorri, A., Mendes, L., Mennella, A., Migliaccio, M., Mitra, S., Miville-Deschenes, M.A., Molinari, D., Moneti, A., Montier, L., Morgante, G., Mortlock, D., Moss, A., Munchmeyer, M., Munshi, D., Murphy, J.A., Naselsky, P., Nati, F., Natoli, P., Netterfield, C.B., Norgaard-Nielsen, H.U., Noviello, F., Novikov, D., Novikov, I., Oxborrow, C.A., Paci, F., Pagano, L., Pajot, F., Paladini, R., Pandolfi, S., Paoletti, D., Pasian, F., Patanchon, G., Pearson, T.J., Peiris, H.V., Perdereau, O., Perotto, L., Perrotta, F., Pettorino, V., Piacentini, F., Piat, M., Pierpaoli, E., Pietrobon, D., Plaszczynski, S., Pointecouteau, E., Polenta, G., Popa, L., Pratt, G.W., Prezeau, G., Prunet, S., Puget, J.L., Rachen, J.P., Reach, W.T., Rebolo, R., Reinecke, M., Remazeilles, M., Renault, C., Renzi, A., Ristorcelli, I., Rocha, G., Rosset, C., Rossetti, M., Roudier, G., Rowan-Robinson, M., Rubino-Martin, J.A., Rusholme, B., Sandri, M., Santos, D., Savelainen, M., Savini, G., Scott, D., Seiffert, M.D., Shellard, E.P.S., Shiraishi, M., Spencer, L.D., Stolyarov, V., Stompor, R., Sudiwala, R., Sunyaev, R., Sutton, D., Suur-Uski, A.S., Sygnet, J.F., Tauber, J.A., Terenzi, L., Toffolatti, L., Tomasi, M., Tristram, M., Trombetti, T., Tucci, M., Tuovinen, J., Valenziano, L., Valiviita, J., Van Tent, B., Vielva, P., Villa, F., Wade, L.A., Wandelt, B.D., Wehus, I.K., White, M., Yvon, D., Zacchei, A., Zibin, J.P., Zonca, A.
    Publicado 2015
    “…These results imply that $V(\phi) \propto \phi^2$ and natural inflation are now disfavoured compared to models predicting a smaller tensor-to-scalar ratio, such as $R^2$ inflation. …”
    Enlace del recurso
    Enlace del recurso
    Planck 2015. XX. Constraints on inflation
  2. 162
    por Shkerin, Andrey, Sibiryakov, Sergey
    Publicado 2015
    “…We study Coleman-De Luccia tunneling of the Standard Model Higgs field during inflation in the case when the electroweak vacuum is metastable. …”
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    On stability of electroweak vacuum during inflation
  3. 163
    Enlace del recurso
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    Phenomenological Aspects of No-Scale Inflation Models
  4. 164
    “…This is particularly problematic during inflation, which sources large perturbations of the Higgs. …”
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    Higgs portal valleys, stability and inflation
  5. 165
    “…A recent paper argued that it is not possible to infer the energy scale of inflation from the amplitude of tensor fluctuations in the Cosmic Microwave Background, because the usual connection is substantially altered if there are a large number of universally coupled fields present during inflation, with mass less than the inflationary Hubble scale. …”
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    Effective Planck Mass and the Scale of Inflation
  6. 166
    por Linde, Andrei D
    Publicado 1990
    “…Inflation and Quantum Cosmology…”
    Enlace del recurso
    Inflation and quantum cosmology: acollection of reprints
  7. 167
    por Finelli, Fabio, Bucher, Martin, Achúcarro, Ana, Ballardini, Mario, Bartolo, Nicola, Baumann, Daniel, Clesse, Sébastien, Errard, Josquin, Handley, Will, Hindmarsh, Mark, Kiiveri, Kimmo, Kunz, Martin, Lasenby, Anthony, Liguori, Michele, Paoletti, Daniela, Ringeval, Christophe, Väliviita, Jussi, Van Tent, Bartjan, Vennin, Vincent, Arroja, Frederico, Ashdown, Marc, Banday, A.J., Banerji, Ranajoy, Baselmans, Jochem, Bartlett, James G., de Bernardis, Paolo, Bersanelli, Marco, Bonaldi, Anna, Borril, Julian, Bouchet, François R., Boulanger, François, Brinckmann, Thejs, Cai, Zhen-Yi, Calvo, Martino, Challinor, Anthony, Chluba, Jens, D'Amico, Guido, Delabrouille, Jacques, Diego, Jose Maria, De Zotti,Gianfranco, Desjacques, Vincent, Di Valentino, Eleonora, Feeney, Stephen, Fergusson, James R., Ferraro, Simone, Forastieri, Francesco, Galli, Silvia, García-Bellido, Juan, Génova-Santos, Ricardo T., Gerbino, Martina, González-Nuevo, Joaquin, Grandis, Sebastian, Greenslade, Josh, Hagstotz, Steffen, Hanany, Shaul, Hazra, Dhiraj K., Hernández-Monteagudo, Carlos, Hivon, Eric, Hu, Bin, Kovetz, Ely D., Kurki-Suonio, Hannu, Lattanzi, Massimiliano, Lesgourgues, Julien, Lizarraga, Joanes, López-Caniego, Marcos, Luzzi, Gemma, Maffei, Bruno, Martins, Carlos J.A.P., Martínez-González, Enrique, McCarthy, Darragh, Matarrese, Sabino, Melchiorri, Alessandro, Melin, Jean-Baptiste, Monfardini, Alessandro, Natoli, Paolo, Negrello, Mattia, Notari, Alessio, Oppizzi, Filippo, Paiella, A., Pajer, Enrico, Patanchon, Guillaume, Patil, Subodh P., Piat, Michael, Pisano, Giampaolo, Polastri, L., Polenta, Gianluca, Poulin, Vivian, Quartin, M., Ravenni, Andrea, Remazeilles, Mathieu, Renzi, Alessandro, Roest, Diederik, Salvati, Laura, Tartari, Andrea, Tasinato, Gianmassimo, Torrado, Jesús, Trappe, Neil, Tucci, Marco, Urrestilla, Jon, Vielva, Patricio, van de Weygaert, Rien
    Publicado 2016
    “…We forecast the scientific capabilities to improve our understanding of cosmic inflation of CORE, a proposed CMB space satellite submitted in response to the ESA fifth call for a medium-size mission opportunity. …”
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    Exploring Cosmic Origins with CORE: Inflation
  8. 168
    “…As an application, we reconsider the decay of the electroweak Higgs vacuum during inflation. Our vacuum decay computation reproduces and improves bounds on the maximal inflationary Hubble scale previously computed through statistical techniques.…”
    Enlace del recurso
    Enlace del recurso
    (Higgs) vacuum decay during inflation
  9. 169
    por Salvio, Alberto
    Publicado 2017
    “…It has been pointed out that a large non-minimal coupling ξ between the Higgs and the Ricci scalar can source higher derivative operators, which may change the predictions of Higgs inflation. A variant, called critical Higgs inflation, employs the near-criticality of the top mass to introduce an inflection point in the potential and lower drastically the value of ξ . …”
    Enlace del recurso
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    Initial Conditions for Critical Higgs Inflation
  10. 170
    por Masina, Isabella
    Publicado 2018
    “…We consider critical Higgs inflation, namely, Higgs inflation with a rising inflection point at smaller field values than those of the plateau induced by the nonminimal coupling to gravity. …”
    Enlace del recurso
    Enlace del recurso
    Ruling out Critical Higgs Inflation?
  11. 171
    por Lee, Hyun Min
    Publicado 2019
    “…We consider chaotic inflation models with a pseudoscalar field containing the general couplings to the four-form flux. …”
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    Enlace del recurso
    Chaotic inflation with four-form couplings
  12. 172
    “…After reviewing the motivations for cosmological inflation formulated in the formalism of supersymmetry, we argue that the appropriate framework is that of no-scale supergravity. …”
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    Building Models of Inflation in No-Scale Supergravity
  13. 173
    por Dimopoulos, Konstantinos
    Publicado 2021
    “…Cosmic inflation and dark energy hold the key to the origin and the eventual fate of the Universe. …”
    Enlace del recurso
    Introduction to cosmic inflation and dark energy
  14. 174
    “…We compute the spectrum of scalar and tensor metric perturbations generated, as amplified vacuum fluctuations, during an epoch of dilaton-driven inflation of the type occurring naturally in string cosmology. …”
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    Metric perturbations in dilaton-driven inflation
  15. 175
    “…Conventional wisdom says that a chaotic inflation model with a power-law potential is ruled out by the recent Planck-BICEP/Keck results. …”
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    Non-minimally assisted chaotic inflation
  16. 176
    “…We study the ultraviolet behaviour of Higgs inflation models above the apparent unitarity violation scale arising from the large non minimal coupling to gravity, by computing on-shell 4-point scattering amplitudes in the presence of a large inflaton background, away from the electroweak vacuum. …”
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    Ultraviolet behaviour of Higgs inflation models
  17. 177
    por Brustein, Ram
    Publicado 1995
    “…I present an outline for cosmological evolution in the framework of string theory with emphasis on a phase of dilaton-driven kinetic inflation. It is shown that a typical background of stochastic gravitational radiation is generated, with strength that may allow its detection in future gravity wave experiments.…”
    Enlace del recurso
    Dilaton-driven inflation in string cosmology
  18. 178
    “…In this paper, we study this novel mechanism known as wash-in leptogenesis, utilizing axion inflation as the source of high-scale CP violation. …”
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    Wash-in leptogenesis after axion inflation
  19. 179
    por Davis, A C, Dimopoulos, K
    Publicado 1995
    “…We show that, during hybrid inflation, a primordial magnetic field can be created, sufficiently strong to seed the galactic dynamo and generate the observed galactic magnetic fields. …”
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    Primordial magnetic fields in hybrid inflation
  20. 180
    “…The general scalar-tensor theory that includes all the dimension-four terms has parameter regions that can produce successful inflation consistent with cosmological observations. …”
    Enlace del recurso
    Enlace del recurso
    Ultraviolet Sensitivity in Higgs-Starobinsky Inflation
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