Results 21 to 29 of about 20,249 (29)
Brane-World Gravity [PDF]
, 2010 The observable universe could be a 1+3-surface (the "brane") embedded in a
1+3+\textit{d}-dimensional spacetime (the "bulk"), with Standard Model
particles and fields trapped on the brane while gravity is free to access the
bulk.A Albrecht, A Bayntun, A Campos, A Campos, A Campos, A Cardoso, A Cardoso, A Cardoso, A Chamblin, A Chamblin, A Chamblin, A Feinstein, A Hebecker, A Karch, A Kehagias, A Lue, A Lue, A Lue, A Lue, A Lukas, A Lukas, A Lukas, A Mazumdar, A Mennim, A Mennim, A Mennim, A Neronov, A Neronov, A Padilla, A Pérez-Lorenzana, AA Coley, AA Coley, AD Linde, AJ Tolley, AJ Tolley, AJ Tolley, AR Liddle, AR Liddle, AR Liddle, AS Majumdar, AS Majumdar, AV Frolov, AV Toporensky, B Boisseau, B Gumjudpai, B Gumjudpai, B Leong, B Leong, B Wang, C Barceló, C Barceló, C Barceló, C Barceló, C Bruck van de, C Bruck van de, C Charmousis, C Charmousis, C Charmousis, C Charmousis, C Charmousis, C Charmousis, C Deffayet, C Deffayet, C Deffayet, C Deffayet, C Germani, C Germani, C Germani, C Gordon, C Rham de, C Rham de, C Rham de, C Rham de, C Rham de, C Rham de, C-M Chen, CJ Hogan, CP Burgess, CP Burgess, CP Burgess, CP Burgess, CP Burgess, CS Rhodes, D Baumann, D Baumann, D Baumann, D Clancy, D Gorbunov, D Ida, D Langlois, D Langlois, D Langlois, D Langlois, D Langlois, D Langlois, D Langlois, D Langlois, D Langlois, D Langlois, D Langlois, D Langlois, D Seery, D Seery, D Wands, D Wands, DJH Chung, DJH Chung, DS Gorbunov, E Anderson, E Kiritsis, E Leeper, E Papantonopoulos, E Papantonopoulos, E Papantonopoulos, E Papantonopoulos, E Silverstein, ED Stewart, EJ Copeland, EJ Copeland, EJ Copeland, EV Linder, F Arroja, F Quevedo, G Calcagni, G Dvali, G Dvali, G Dvali, G Gabadadze, G Huey, G Huey, G Kofinas, G Kofinas, G Kofinas, G Kofinas, GA Diamandis, GF Giudice, GFR Ellis, GN Felder, GR Dvali, GW Gibbons, H Collins, H Collins, H Ishihara, H Kodama, H Kodama, H Kodama, H Kudoh, H Stoica, H Yoshino, HA Bridgman, HA Bridgman, HL Verlinde, I Antoniadis, I Antoniadis, I Giannakis, I Giannakis, I Navarro, I Savonije, I Sawicki, IP Neupane, J Garriga, J Garriga, J Garriga, J Garriga, J Gray, J Hewett, J Khoury, J Lesgourgues, J Martin, J Polchinski, J Soda, J Soda, J Soda, J Sollerman, J Vinet, J Vinet, J Yokoyama, JC Long, JD Barrow, JD Barrow, JD Barrow, JD Bratt, JE Lidsey, JE Lidsey, JE Lidsey, JE Lidsey, JE Lidsey, JJ Blanco-Pillado, JL Hovdebo, JM Aguirregabiria, JM Cline, JP Gregory, JP Gregory, K Akama, K Ichiki, K Ichiki, K Koyama, K Koyama, K Koyama, K Koyama, K Koyama, K Koyama, K Koyama, K Koyama, K Koyama, K Koyama, K Koyama, K Koyama, K Koyama, K Koyama, K Koyama, K Koyama, K Maeda, K Maeda, K Maeda, KE Kunze, KT Inoue, L Anchordoqui, L Guzzo, L Mendes, L Randall, L Randall, LP Chimento, M Bastero-Gil, M Bouhmadi-López, M Bruni, M Cavaglià, M Dorca, M Gogberashvili, M Govender, M Kolanovic, M Kunz, M Minamitsuji, M Minamitsuji, M Minamitsuji, M Peloso, M Peloso, M Rinaldi, M Sasaki, M Visser, M Visser, MC Bento, MC Bento, MC Bento, MG Santos, MJ Duff, N Agarwal, N Arkani-Hamed, N Dadhich, N Dadhich, N Deruelle, N Deruelle, N Deruelle, N Deruelle, N Deruelle, N Kaloper, N Kaloper, N Kaloper, N Kaloper, N Sago, NE Mavromatos, NE Mavromatos, NJ Nunes, O Corradini, O Corradini, O Corradini, O Seto, P Binétruy, P Binétruy, P Binétruy, P Bostock, P Bowcock, P Brax, P Brax, P Brax, P Horava, P Kanti, P Kanti, P Kraus, PJ Steinhardt, PR Ashcroft, PR Ashcroft, R Allahverdi, R Brustein, R Casadio, R Casadio, R Durrer, R Easther, R Emparan, R Emparan, R Emparan, R Gregory, R Guedens, R Guedens, R Hawkins, R Lazkoz, R Maartens, R Maartens, R Maartens, R Maartens, R Maartens, R Maartens, RA Battye, RE Kallosh, RH Brandenberger, RM Wald, RP Geroch, RR Caldwell, S Fujii, S Förste, S Hannestad, S Kachru, S Kachru, S Kanno, S Kanno, S Kanno, S Kobayashi, S Mizuno, S Mizuno, S Mukohyama, S Mukohyama, S Mukohyama, S Mukohyama, S Mukohyama, S Mukohyama, S Mukohyama, S Nojiri, S Nojiri, S Nojiri, S Nojiri, S Tsujikawa, S Tsujikawa, SB Giddings, SB Giddings, SB Giddings, SC Davis, SL Dubovsky, SP Alwis de, SP Alwis de, SS Gubser, SS Seahra, SS Seahra, SW Hawking, SW Hawking, T Boehm, T Giannantonio, T Giannantonio, T Giannantonio, T Hiramatsu, T Hiramatsu, T Hiramatsu, T Kobayashi, T Kobayashi, T Multamäki, T Shiromizu, T Shiromizu, T Shiromizu, T Shiromizu, T Shiromizu, T Tanaka, T Tanaka, T Tanaka, T Thiemann, T Wiseman, T Wiseman, U Gen, U Gen, V Sahni, V Sahni, V Sahni, V Sahni, VA Rubakov, VA Rubakov, VF Mukhanov, W Fang, WD Goldberger, Y Aghababaie, Y Aghababaie, Y Aghababaie, Y Himemoto, Y Himemoto, Y Himemoto, Y Himemoto, Y Sendouda, Y Sendouda, Y Sendouda, Y Shtanov, Y Shtanov, Y Shtanov, Y-S Song, Z Keresztes, Z Keresztes, ÉÉ Flanagan, ÉÉ Flanagan +393 morecore +4 more sourcesA Zero-Parameter Extension of General Relativity with Varying
Cosmological Constant
, 2019 We provide a new extension of general relativity (GR) which has the
remarkable property of being more constrained than GR plus a cosmological
constant, having one less free parameter.Alexander, Stephon, Cortês, Marina, Liddle, Andrew R., Magueijo, João, Sims, Robert, Smolin, Lee +5 morecore +1 more sourceA candidate for a background independent formulation of M theory
, 1999 A class of background independent membrane field theories are studied, and
several properties are discovered which suggest that they may play a role in a
background independent form of M theory.A. Ashtekar, A. Ashtekar, A. Ashtekar, A. Ashtekar, A. Ashtekar, A. Ashtekar, A. Barbieri, A. Sen, A. Sen, B. Bruegmann, B. Bruegmann, B. DeWitt, Brian R. Greene, C. M. Hull, C. Rovelli, C. Rovelli, C. Rovelli, C. Rovelli, C. Rovelli, C. Rovelli, C. Rovelli, D. Armand-Ugon, D. Rayner, D. Rayner, E. Verlinde, E. Witten, E. Witten, E. Witten, E. Witten, F. Markopoulou, F. Markopoulou, F. Markopoulou, F. Markopoulou, F. Markopoulou, G. Moore, G. Moore, G. ’t Hooft, Gary T. Horowitz, H. Kodama, H. Kunitomo, H. Kunitomo, J. Ambjorn, J. Ambjorn, J. Baez, J. Barrett, J. D. Bekenstein, J. Lewandowski, Juan M. Maldacena, Juan M. Maldacena, K. Ezawa, K. Krasnov, K. Krasnov, K. Krasnov, L. Bombelli, L. Buffon, L. Crane, L. Crane, L. Crane, L. Kauffman, L. Smolin, L. Smolin, L. Smolin, L. Smolin, L. Susskind, L. Susskind, L. Susskind, L. Susskind, Lee Smolin, M. Reisenberger, N. Yu. Reshetikhin, N. Yu. Reshetikhin, P. Bak, P. Bak, P. S. Aspinwall, P. S. Aspinwall, P. Townsend, Petr Horava, R. Borissov, R. Borissov, R. Bousso, R. Bousso, R. DePietri, R. Dijkgraaf, R. Gambini, R. Loll, R. Loll, S. Major, S. S. Gubser, Simonetta Frittelli, Simonetta Frittelli, Simonetta Frittelli, Simonetta Frittelli, T. Banks, T. Jacobson, T. Jaocobson, T. Kadoyoshi, T. Thiemann, T. Thiemann, T. Thiemann, T. Thiemann, T. Thiemann, T. Thiemann, T. Thiemann, T. Thiemann, Takashi Sano, Tom Banks, V. Turaev, Y. Ling, Yi Li +108 morecore +3 more sourcesQuantum gravity in the very early universe
, 2011 General relativity describes the gravitational field geometrically and in a
self-interacting way because it couples to all forms of energy, including its
own.Ashtekar, Ashtekar, Bojowald, Bojowald, Bojowald, Bojowald, Bojowald, Bojowald, Hayward, Martin Bojowald, Meissner, Mielczarek, Novello, Roman, Rovelli, Rovelli, Singh, Thiemann, Thiemann, Thiemann +19 morecore +1 more source
