Results 1 to 10 of about 36,935 (199)
A UNIFIED MODEL OF HIGH-ENERGY ASTROPHYSICAL PHENOMENA [PDF]
International Journal of Modern Physics A, 2005 I outline a unified model of high-energy astrophysics, in which the gamma background radiation, cluster "cooling flows", gamma-ray bursts, X-ray flashes and cosmic-ray electrons and nuclei of all energies — share a common origin. The mechanism underlying these phenomena is the emission of relativistic "cannonballs" by ordinary supernovae, analogous to A. Rújulaopenaire +4 more sourcesThe Phenomena of High Energy Astrophysics [PDF]
Symposium - International Astronomical Union, 2003 A brief summary of some highlights in the study of high energy astrophysical sources over the past decade is presented. It is argued that the great progress that has been made derives largely from the application of new technology to observation throughout all of the electromagnetic and other spectra and that, on this basis, the next decade should be ...R. Blandfordopenaire +5 more sourcesGrailQuest: hunting for atoms of space and time hidden in the wrinkle of Space-Time [PDF]
Experimental Astronomy, 2021 AbstractGrailQuest(Gamma Ray Astronomy International Laboratory for QUantum Exploration of Space-Time) is a mission concept based on a constellation (hundreds/thousands) of nano/micro/small-satellites in low (or near) Earth orbits. Each satellite hosts a non-collimated array of scintillator crystals coupled with Silicon Drift Detectors with broad ...Burderi L., Sanna A., Di Salvo T., Amati L., Amelino-Camelia G., Branchesi M., Capozziello S., Coccia E., Colpi M., Costa E., D'Amico N., De Bernardis P., De Laurentis M., Valle M. D., Falcke H., Feroci M., Fiore F., Frontera F., Gambino A. F., Ghisellini G., Hurley K. C., Iaria R., Kataria D., Labanti C., Lodato G., Negri B., Papitto A., Piran T., Riggio A., Rovelli C., Santangelo A., Vidotto F., Zane S. +32 moreopenaire +7 more sourcesSimilarity Properties and Scaling Laws of Radiation Hydrodynamic Flows
in Laboratory Astrophysics [PDF]
, 2011 The spectacular recent development of modern high-energy density laboratory
facilities which concentrate more and more energy in millimetric volumes allows
the astrophysical community to reproduce and to explore, in millimeter-scale
targets and during ..., Basko, Birkhoff, Bluman, Bouquet, C. Michaut, Drake, Drake, Falize, Falize, Falize, Gregory, Hartigan, Hoogerwerf, Kuranz, Lynden-Bell, Mihalas, Pomraning, Ryutov, Ryutov, Ryutov, S. Bouquet, Sedov, Zeldovich, É. Falize +24 morecore +5 more sourcesHIGH ENERGY APPROACHES TO LOW ENERGY PHENOMENA IN ASTROPHYSICS [PDF]
Electromagnetic Interactions in Nuclear and Hadron Physics, 2002 Studies in nuclear astrophysics have long been associated with long runs at small accelerators, measuring ever-decreasing cross sections as one approached (but rarely reached) the energy of reactions in stars. But in recent years pioneering studies have shown that studies at high-energy accelerators can often yield the same information, and in some ...openaire +2 more sourcesSimilar phenomena at different scales: Black Holes, the Sun, Gamma-ray
Bursts, Supernovae, Galaxies and Galaxy Clusters [PDF]
, 2007 Many similar phenomena occur in astrophysical systems with spatial and mass
scales different by many orders of magnitudes. For examples, collimated
outflows are produced from the Sun, proto-stellar systems, gamma-ray bursts,
neutron star and black hole X-Aschenbach, Bassani, Chen, Mineshige, Mirabel, Priest, Shakura, Shuang Nan Zhang, Takeuchi, Walsh, Zhang, Zhang, Zhang +12 morecore +2 more sourcesOscillations and waves in solar spicules [PDF]
, 2009 Since their discovery, spicules have attracted increased attention as energy/mass bridges between the dense and dynamic photosphere and the tenuous hot solar corona.A. Ajabshirizadeh, A. Osin, A.C. Sterling, B. Fleck, B. Fleck, B. Pontieu De, B. Pontieu De, B. Pontieu De, B. Pontieu De, B. Pontieu De, B. Pontieu De, B. Pontieu De, B. Roberts, B. Rompolt, C. Malins, C.D. Pike, C.D. Pike, D. Banerjee, D.B. Jess, E. Khutsishvili, E. O’Shea, F. Schmitz, G. Sutmann, G. Verth, G.L. Withbroe, G.M. Nikolsky, G.M. Nikolsky, H.C. Spruit, H.C. Spruit, I. Ballai, I.C. Rae, J. Koza, J.D. Bochlin, J.G. Doyle, J.M. Beckers, J.M. Beckers, J.M. Pasachoff, J.V. Hollweg, J.V. Hollweg, K. Matsuno, L. Heggland, L.D. Xia, L.H.M. Rouppe van der Voort, M. Abramowitz, M.I. Pishkalo, M.J. Aschwanden, M.S. Madjarska, M.S. Ruderman, N. Nishizuka, P.A. Secchi, P.G. Papushev, P.M. Edwin, P.M. Morse, R. Erdélyi, R. Erdélyi, R. Erdélyi, R. Erdélyi, S. Parenti, S.R. Weart, S.S. Hasan, S.S. Hasan, T. Doorsselaere Van, T. Doorsselaere Van, T. V. Zaqarashvili, T.G. Gadzhiev, T.J. Bogdan, T.J. Bogdan, T.V. Zaqarashvili, T.V. Zaqarashvili, T.V. Zaqarashvili, V. Kukhianidze, V.H. Hansteen, V.I. Kulidzanishvili, V.I. Kulidzanishvili, W.O. Roberts, Y. Yamauchi, Z.E. Musielak +76 morecore +2 more sourcesGalaxy Formation Theory [PDF]
, 2010 We review the current theory of how galaxies form within the cosmological
framework provided by the cold dark matter paradigm for structure formation.
Beginning with the pre-galactic evolution of baryonic material we describe the
analytical and numerical Abadi, Abadi, Abel, Abel, Abel, Abraham, Agertz, Ahn, Allen, Andrew J. Benson, Angus, Arad, Arons, Athanassoula, Athanassoula, Aubert, Bahcall, Bahcall, Banerjee, Bardeen, Barnes, Barnes, Barnes, Baugh, Baugh, Baugh, Baugh, Baugh, Baugh, Baugh, Baugh, Begelman, Begelman, Bell, Belokurov, Belokurov, Benson, Benson, Benson, Benson, Benson, Benson, Benson, Benson, Benson, Benson, Benson, Benson, Benson, Benson, Benson, Benson, Benson, Berezinsky, Berti, Bertin, Bertone, Bertschinger, Bertschinger, Bett, Binney, Binney, Birnboim, Birzan, Blaizot, Blaizot, Blaizot, Blanchet, Bland-Hawthorn, Blandford, Blandford, Blumenthal, Blumenthal, Bode, Boehm, Bond, Bondi, Booth, Borgani, Bournaud, Bournaud, Bower, Bower, Bower, Bower, Boylan-Kolchin, Boyle, Bromm, Bromm, Brook, Brook, Brooks, Bruzual, Brüggen, Brüggen, Bullock, Bullock, Bullock, Bullock, Cardone, Cattaneo, Cazaux, Chabrier, Chakrabarti, Chandrasekhar, Chary, Chiu, Christodoulou, Christodoulou, Ciardi, Ciardi, Ciotti, Clarke, Clarke, Cole, Cole, Cole, Cole, Cole, Cole, Cole, Colín, Conroy, Conroy, Conroy, Cooray, Covington, Cox, Cox, Crain, Croton, Croton, Davis, Davé, de Vaucouleurs, Dekel, Devriendt, Devriendt, Diaferio, Dolag, Dotter, Dove, Draine, Dunkley, Dutton, Dutton, Edgar, Efstathiou, Efstathiou, Efstathiou, Einasto, Eisenstein, Eke, Eke, El-Zant, Elahi, Fakhouri, Fakhouri, Fall, Fan, Fardal, Favata, Federrath, Ferland, Ferrara, Ferrarese, Ferrarese, Field, Finlator, Firmani, Fitchett, Font, Font, Font, Font, Fontanot, Fontanot, François, Freeman, Frenk, Frenk, Frenk, Friedli, Fryxell, Galli, Gao, Gao, Gebhardt, Gebhardt, Glover, Gnat, Gnedin, Gnedin, Gnedin, Gnedin, Gnedin, Gnedin, Gnedin, Gnedin, Goerdt, Goldreich, Gonçalves, Gould, Governato, Governato, Governato, Granato, Greif, Guiderdoni, Gunn, Gunn, Guo, Gustafsson, Haardt, Hahn, Hamilton, Harris, Hatton, Heitmann, Helly, Helly, Henriques, Hernquist, Hollenbach, Hoyle, Hubble, Jenkins, Jenkins, Jiang, Jing, Jog, Johnston, Jonsson, Jubelgas, Kampakoglou, Kant, Katz, Katz, Kauffmann, Kauffmann, Kauffmann, Kauffmann, Kauffmann, Kauffmann, Kauffmann, Kauffmann, Kaufmann, Kay, Kazantzidis, Kennicutt, Kennicutt, Kereš, Kereš, King, King, King, Klypin, Klypin, Klypin, Kobayashi, Komatsu, Komissarov, Kormendy, Kormendy, Kormendy, Kowalski, Kravtsov, Kravtsov, Kravtsov, Kriek, Kroupa, Krumholz, Kuhlen, Kuijken, Lacey, Lacey, Lacey, Lacey, Lanzoni, Larson, Laursen, Law, Lawlor, Lee, Lemson, Li, Li, Libeskind, Lin, Lin, Lintott, Lotz, Lotz, Lucia, Lucia, Lucia, Lynden-Bell, Lynden-Bell, Machida, Madau, Madau, Madau, Magorrian, Malbon, Maller, Maller, Maller, Maller, Mandelbaum, Mao, Maraston, Marigo, Marri, Martin, Martínez-Serrano, Mastropietro, Mastropietro, Mateo, Matteo, Matteo, Matteo, Matteucci, Matteucci, Mayer, Mayer, McCarthy, McCarthy, McDowell, McKee, McKee, Meier, Meier, Meiksin, Merritt, Merritt, Milosavljevic, Milosavljevic, Minchev, Miranda, Mo, Monaco, Monaco, Monaco, Moore, Moore, Moore, Moore, Moore, Murali, Murali, Murali, Murray, Nagashima, Nagashima, Narayan, Narayanan, Narlikar, Navarro, Navarro, Navarro, Navarro, Navarro, Navarro, Neistein, Nemmen, Neyman, Nulsen, Ocvirk, Okamoto, Okamoto, Omma, Oppenheimer, Ostriker, Owen, O’Shea, O’Shea, Padilla, Parkinson, Parrish, Parry, Peacock, Peacock, Peebles, Percival, Percival, Peters, Petkova, Pipino, Pipino, Plewa, Pontzen, Pope, Portinari, Prada, Press, Purcell, Putman, Quilis, Quinlan, Quinlan, Quinn, Randall, Rasmussen, Ratnatunga, Razoumov, Read, Read, Reed, Reed, Rees, Ricker, Ricotti, Ricotti, Ricotti, Rijkhorst, Robertson, Robertson, Robertson, Robertson, Robertson, Robinson, Romano, Romeo, Romeo, Roskar, Roskar, Roychowdhury, Rozo, Ruszkowski, Ruszkowski, Sales, Salpeter, Santoro, Scannapieco, Scannapieco, Scannapieco, Scannapieco, Schade, Schawinski, Schaye, Schmidt, Seljak, Sellwood, Sellwood, Sellwood, Sesana, Sesana, Shakura, Shapiro, Sharma, Shaw, Shen, Sheth, Shlosman, Sijacki, Silk, Silk, Silk, Silva, Simard, Slosar, Smith, Smith, Smoluchowksi, Somerville, Somerville, Somerville, Somerville, Somerville, Somerville, Spitzer, Spitzer, Springel, Springel, Springel, Springel, Springel, Springel, Stacy, Steinmetz, Stewart, Stinson, Strigari, Summers, Swinbank, Tasker, Tasker, Tassis, Taylor, Tegmark, Tegmark, Tegmark, Thacker, Thacker, Thorne, Tichy, Timmes, Tinker, Tinker, Tollerud, Toomre, Tormen, Toth, Tozzi, Tremaine, Tremaine, Trenti, Tumlinson, van den Bosch, van den Bosch, van den Bosch, van Dokkum, Vecchia, Vecchia, Veilleux, Velazquez, Vernaleo, Viel, Vikhlinin, Villalobos, Villiers, Vitvitska, Voit, Volonteri, Volonteri, Volonteri, Wadsley, Wang, Wang, Wang, Warren, Watanabe, Wechsler, Wechsler, Wen, White, White, White, White, White, Williams, Willman, Wise, Wise, Wise, Wise, Wise, Wise, Wuyts, Wyithe, Yajima, Yang, Yoshida, Yoshida, Yoshida, Younger, Younger, Yu, Yüksel, Zavala, Zhang, Zhao, Zhao, Zheng +563 morecore +1 more sourceObservation of collapsing radiative shocks in laboratory experiments [PDF]
, 2006 This article reports the observation of the dense, collapsed layer produced by a radiative shock in a laboratory experiment. The experiment uses laser irradiation to accelerate a thin layer of solid-density material to above 100 km/s100km∕s, the first to Boehly, T., Boireau, L., Bouquet, S., Dannenberg, K. K., Drake, R. Paul, Glendinning, S. Gail, Greenough, J., Grosskopf, M., Harding, Eric C., Knauer, J. P., Koenig, M., Kremer, D. J., Leibrandt, D. R., Perry, T. S., Reighard, A. B., Remington, Bruce A., Vinci, T. +16 morecore +3 more sources
