Zobrazeno 1 - 10
of 180
pro vyhledávání: '"Picon, C. A."'
Autor:
Armendariz-Picon, C.
In previous work we argued that the correct procedure to predict the gravitational wave signal from preheating after inflation rests on the in-in formalism. We extend here our previous analysis to include the backreaction of the produced matter on th
Externí odkaz:
http://arxiv.org/abs/2003.01542
Autor:
Armendariz-Picon, C.
The existing predictions of the energy density of gravitational waves produced during preheating mostly rely on computer simulations in which the matter field inhomogeneities essentially behave classically. In this article we follow instead a full qu
Externí odkaz:
http://arxiv.org/abs/1905.05724
Autor:
Armendariz-Picon, C.
In order for the inflaton to decay into radiation at the end of inflation, it needs to couple to light matter fields. In this article we determine whether such couplings cause the inflaton to decay during inflation rather than after it. We calculate
Externí odkaz:
http://arxiv.org/abs/1708.09755
Autor:
Armendariz-Picon, C.
Because the scale of inflation is conformal frame dependent, in order to fully characterize it one should quote its value in terms of all the independent equal-time dimensionless ratios in the theory. We argue that when couplings depend on the inflat
Externí odkaz:
http://arxiv.org/abs/1510.07956
We study the growth of cosmic structure under the assumption that dark matter self-annihilates with an averaged cross section times relative velocity that grows with the scale factor, an increase known as Sommerfeld-enhancement. Such an evolution is
Externí odkaz:
http://arxiv.org/abs/1210.3017
Autor:
Hewett, J. L., Weerts, H., Brock, R., Butler, J. N., Casey, B. C. K., Collar, J., de Gouvea, A., Essig, R., Grossman, Y., Haxton, W., Jaros, J. A., Jung, C. K., Lu, Z. T., Pitts, K., Ligeti, Z., Patterson, J. R., Ramsey-Musolf, M., Ritchie, J. L., Roodman, A., Scholberg, K., Wagner, C. E. M., Zeller, G. P., Aefsky, S., Afanasev, A., Agashe, K., Albright, C., Alonso, J., Ankenbrandt, C., Aoki, M., Arguelles, C. A., Arkani-Hamed, N., Armendariz, J. R., Armendariz-Picon, C., Diaz, E. Arrieta, Asaadi, J., Asner, D. M., Babu, K. S., Bailey, K., Baker, O., Balantekin, B., Baller, B., Bass, M., Batell, B., Beacham, J., Behr, J., Berger, N., Bergevin, M., Berman, E., Bernstein, R., Bevan, A. J., Bishai, M., Blanke, M., Blessing, S., Blondel, A., Blum, T., Bock, G., Bodek, A., Bonvicini, G., Bossi, F., Boyce, J., Breedon, R., Breidenbach, M., Brice, S. J., Briere, R. A., Brodsky, S., Bromberg, C., Bross, A., Browder, T. E., Bryman, D. A., Buckley, M., Burnstein, R., Caden, E., Campana, P., Carlini, R., Carosi, G., Castromonte, C., Cenci, R., Chakaberia, I., Chen, M. C., Cheng, C. H., Choudhary, B., Christ, N. H., Christensen, E., Christy, M. E., Chupp, T. E., Church, E., Cline, D. B., Coan, T. E., Coloma, P., Comfort, J., Coney, L., Cooper, J., Cooper, R. J., Cowan, R., Cowen, D. F., Cronin-Hennessy, D., Datta, A., Davies, G. S., Demarteau, M., DeMille, D. P., Denig, A., Dermisek, R., Deshpande, A., Dewey, M. S., Dharmapalan, R., Dhooghe, J., Dietrich, M. R., Diwan, M., Djurcic, Z., Dobbs, S., Duraisamy, M., Dutta, B., Duyang, H., Dwyer, D. A., Eads, M., Echenard, B., Elliott, S. R., Escobar, C., Fajans, J., Farooq, S., Faroughy, C., Fast, J. E., Feinberg, B., Felde, J., Feldman, G., Fierlinger, P., Perez, P. Fileviez, Filippone, B., Fisher, P., Flemming, B. T., Flood, K. T., Forty, R., Frank, M. J., Freyberger, A., Friedland, A., Gandhi, R., Ganezer, K. S., Garcia, A., Garcia, F. G., Gardner, S., Garrison, L., Gasparian, A., Geer, S., Gehman, V. M., Gershon, T., Gilchriese, M., Ginsberg, C., Gogoladze, I., Gonderinger, M., Goodman, M., Gould, H., Graham, M., Graham, P. W., Gran, R., Grange, J., Gratta, G., Green, J. P., Greenlee, H., Group, R. C., Guardincerri, E., Gudkov, V., Guenette, R., Haas, A., Hahn, A., Han, T., Handler, T., Hardy, J. C., Harnik, R., Harris, D. A., Harris, F. A., Harris, P. G., Hartnett, J., He, B., Heckel, B. R., Heeger, K. M., Henderson, S., Hertzog, D., Hill, R., Hinds, E. A, Hitlin, D. G., Holt, R. J., Holtkamp, N., Horton-Smith, G., Huber, P., Huelsnitz, W., Imber, J., Irastorza, I., Jaeckel, J., Jaegle, I., James, C., Jawahery, A., Jensen, D., Jessop, C. P., Jones, B., Jostlein, H., Junk, T., Kagan, A. L., Kalita, M., Kamyshkov, Y., Kaplan, D. M., Karagiorgi, G., Karle, A., Katori, T., Kayser, B., Kephart, R., Kettell, S., Kim, Y. K., Kirby, M., Kirch, K., Klein, J., Kneller, J., Kobach, A., Kohl, M., Kopp, J., Kordosky, M., Korsch, W., Kourbanis, I., Krisch, A. D., Krizan, P., Kronfeld, A. S., Kulkarni, S., Kumar, K. S., Kuno, Y., Kutter, T., Lachenmaier, T., Lamm, M., Lancaster, J., Lancaster, M., Lane, C., Lang, K., Langacker, P., Lazarevic, S., Le, T., Lee, K., Lesko, K. T., Li, Y., Lindgren, M., Lindner, A., Link, J., Lissauer, D., Littenberg, L. S., Littlejohn, B., Liu, C. Y., Loinaz, W., Lorenzon, W., Louis, W. C., Lozier, J., Ludovici, L., Lueking, L., Lunardini, C., MacFarlane, D. B., Machado, P. A. N., Mackenzie, P. B., Maloney, J., Marciano, W. J., Marsh, W., Marshak, M., Martin, J. W., Mauger, C., McFarland, K. S., McGrew, C., McLaughlin, G., McKeen, D., McKeown, R., Meadows, B. T., Mehdiyev, R., Melconian, D., Merkel, H., Messier, M., Miller, J. P., Mills, G., Minamisono, U. K., Mishra, S. R., Mocioiu, I., Sher, S. Moed, Mohapatra, R. N., Monreal, B., Moore, C. D., Morfin, J. G., Mousseau, J., Moustakas, L. A., Mueller, G., Mueller, P., Muether, M., Mumm, H. P., Munger, C., Murayama, H., Nath, P., Naviliat-Cuncin, O., Nelson, J. K., Neuffer, D., Nico, J. S., Norman, A., Nygren, D., Obayashi, Y., O'Connor, T. P., Okada, Y., Olsen, J., Orozco, L., Orrell, J. L., Osta, J., Pahlka, B., Paley, J., Papadimitriou, V., Papucci, M., Parke, S., Parker, R. H., Parsa, Z., Partyka, K., Patch, A., Pati, J. C., Patterson, R. B., Pavlovic, Z., Paz, G., Perdue, G. N., Perevalov, D., Perez, G., Petti, R., Pettus, W., Piepke, A., Pivovaroff, M., Plunkett, R., Polly, C. C., Pospelov, M., Povey, R., Prakesh, A., Purohit, M. V., Raby, S., Raaf, J. L., Rajendran, R., Rajendran, S., Rameika, G., Ramsey, R., Rashed, A., Ratcliff, B. N., Rebel, B., Redondo, J., Reimer, P., Reitzner, D., Ringer, F., Ringwald, A., Riordan, S., Roberts, B. L., Roberts, D. A., Robertson, R., Robicheaux, F., Rominsky, M., Roser, R., Rosner, J. L., Rott, C., Rubin, P., Saito, N., Sanchez, M., Sarkar, S., Schellman, H., Schmidt, B., Schmitt, M., Schmitz, D. W., Schneps, J., Schopper, A., Schuster, P., Schwartz, A. J., Schwarz, M., Seeman, J., Semertzidis, Y. K., Seth, K. K., Shafi, Q., Shanahan, P., Sharma, R., Sharpe, S. R., Shiozawa, M., Shiltsev, V., Sigurdson, K., Sikivie, P., Singh, J., Sivers, D., Skwarnicki, T., Smith, N., Sobczyk, J., Sobel, H., Soderberg, M., Song, Y. H., Soni, A., Souder, P., Sousa, A., Spitz, J., Stancari, M., Stavenga, G. C., Steffen, J. H., Stepanyan, S., Stoeckinger, D., Stone, S., Strait, J., Strassler, M., Sulai, I. A., Sundrum, R., Svoboda, R., Szczerbinska, B., Szelc, A., Takeuchi, T., Tanedo, P., Taneja, S., Tang, J., Tanner, D. B., Tayloe, R., Taylor, I., Thomas, J., Thorn, C., Tian, X., Tice, B. G., Tobar, M., Tolich, N., Toro, N., Towner, I. S., Tsai, Y., Tschirhart, R., Tunnell, C. D., Tzanov, M., Upadhye, A., Urheim, J., Vahsen, S., Vainshtein, A., Valencia, E., Van de Water, R. G., Van de Water, R. S., Velasco, M., Vogel, J., Vogel, P., Vogelsang, W., Wah, Y. W., Walker, D., Weiner, N., Weltman, A., Wendell, R., Wester, W., Wetstein, M., White, C., Whitehead, L., Whitmore, J., Widmann, E., Wiedemann, G., Wilkerson, J., Wilkinson, G., Wilson, P., Wilson, R. J., Winter, W., Wise, M. B., Wodin, J., Wojcicki, S., Wojtsekhowski, B., Wongjirad, T., Worcester, E., Wurtele, J., Xin, T., Xu, J., Yamanaka, T., Yamazaki, Y., Yavin, I., Yeck, J., Yeh, M., Yokoyama, M., Yoo, J., Young, A., Zimmerman, E., Zioutas, K., Zisman, M., Zupan, J., Zwaska, R.
The Proceedings of the 2011 workshop on Fundamental Physics at the Intensity Frontier. Science opportunities at the intensity frontier are identified and described in the areas of heavy quarks, charged leptons, neutrinos, proton decay, new light weak
Externí odkaz:
http://arxiv.org/abs/1205.2671
Autor:
Armendariz-Picon, C.
A central assumption in our analysis of cosmic structure is that cosmological perturbations have zero ensemble mean. This property is one of the consequences of statistically homogeneity, the invariance of correlation functions under spatial translat
Externí odkaz:
http://arxiv.org/abs/1012.2849
Autor:
Armendariz-Picon, C., Pekowsky, Larne
Publikováno v:
Phys.Rev.Lett.102:031301,2009
It is often assumed that primordial perturbations are statistically isotropic, which implies, among other properties, that their power spectrum is invariant under rotations. In this article, we test this assumption by placing model-independent bounds
Externí odkaz:
http://arxiv.org/abs/0807.2687
Autor:
Armendariz-Picon, C.
Publikováno v:
JCAP 0709:014,2007
In almost all structure formation models, primordial perturbations are created within a homogeneous and isotropic universe, like the one we observe. Because their ensemble averages inherit the symmetries of the spacetime in which they are seeded, cos
Externí odkaz:
http://arxiv.org/abs/0705.1167
Autor:
Armendariz-Picon, C.
Publikováno v:
JCAP 0702:031,2007
In order to calculate the power spectrum generated during a stage of inflation, we have to specify the quantum state of the inflaton perturbations, which is conventionally assumed to be the Bunch-Davies vacuum. We argue that this choice is justified
Externí odkaz:
http://arxiv.org/abs/astro-ph/0612288