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Mostrando 481 - 500 Resultados de 591 Para Buscar '"supernova"', tiempo de consulta: 0.19s Limitar resultados
  1. 481
    por Smith, Francis Graham
    Publicado 1977
    “…The discovery of the pulsars ; techniques for search and for observation ; the identification with rotating neutron stars ; the X-ray pulsars ; the internal structure of neutron stars ; the magnetosphere of neutron stars ; pulse timing ; properties of the integrated radio pulses ; individual radio pulses ; the Crab nebula ; the Crab pulsar ; the interstellar medium as an indicator of pulsar distances ; the interstellar magnetic field ; interstellar scintillation ; radiation processes ; the emission mechanism I : analysis of observed particles ; the emission mechanism II : geometrical considerations ; the emission mechanism : discussion ; supernovae : the origin of the pulsars ; the distribution and the ages of pulsars ; high energies and condensed stars.…”
    Enlace del recurso
    Pulsars
  2. 482
    por Palanque-Delabrouille, N
    Publicado 2008
    “…The next lecture will cover the ongoing experiments dedicated to the study of dark matter (direct detection or microlensing experiments) and dark energy (in particular the experiments searching for supernovae). The last lecture will be devoted to high energy astrophysics, large scale cosmic ray detectors and high energy neutrino detectors. …”
    Enlace del recurso
    Astroparticle Physics (2/3)
  3. 483
    por Palanque-Delabrouille, N
    Publicado 2008
    “…The next lecture will cover the ongoing experiments dedicated to the study of dark matter (direct detection or microlensing experiments) and dark energy (in particular the experiments searching for supernovae). The last lecture will be devoted to high energy astrophysics, large scale cosmic ray detectors and high energy neutrino detectors. …”
    Enlace del recurso
    Astroparticle Physics (1/3)
  4. 484
    por Palanque-Delabrouille, N
    Publicado 2008
    “…The next lecture will cover the ongoing experiments dedicated to the study of dark matter (direct detection or microlensing experiments) and dark energy (in particular the experiments searching for supernovae). The last lecture will be devoted to high energy astrophysics, large scale cosmic ray detectors and high energy neutrino detectors. …”
    Enlace del recurso
    Astroparticle Physics (3/3)
  5. 485
    “…The next lecture will cover the ongoing experiments dedicated to the study of dark matter (direct detection or microlensing experiments) and dark energy (in particular the experiments searching for supernovae). The last lecture will be devoted to high energy astrophysics, large scale cosmic ray detectors and high energy neutrino detectors. …”
    Enlace del recurso
    Astroparticle physics (1/3)
  6. 486
    “…The next lecture will cover the ongoing experiments dedicated to the study of dark matter (direct detection or microlensing experiments) and dark energy (in particular the experiments searching for supernovae). The last lecture will be devoted to high energy astrophysics, large scale cosmic ray detectors and high energy neutrino detectors. …”
    Enlace del recurso
    Astroparticle physics (2/3)
  7. 487
    “…The next lecture will cover the ongoing experiments dedicated to the study of dark matter (direct detection or microlensing experiments) and dark energy (in particular the experiments searching for supernovae). The last lecture will be devoted to high energy astrophysics, large scale cosmic ray detectors and high energy neutrino detectors. …”
    Enlace del recurso
    Astroparticle physics (3/3)
  8. 488
    por Rees, Martin J
    Publicado 1979
    “…If there was indeed a "big bang", surprisingly strong conclusions can be drawn about the number of species of neutrinos, and about the possibility that such particles have non-zero rest mass. The dynamics of supernovae are sensitive to the det~ils of neutrino physics; such explosions would yield IO L-1053 ergs of -v IO Mev neutrinos, in a burst lasting a few milliseconds. …”
    Enlace del recurso
    Neutrinos in astrophysics
  9. 489
    “…Local structure can have important effects on luminosity distance observations, which could for example affect the local estimation of the Hubble constant based on low red-shift type Ia supernovae. Using a spherically symmetric exact solution of the Eistein's equations and a more accurate expansion of the solution of the geodesic equations, we improve the low red-shift expansion of the monopole of the luminosity distance in terms of the curvature function. …”
    Enlace del recurso
    Enlace del recurso
    Coordinate independent approach to the calculation of the effects of local structure on the luminosity distance
  10. 490
    “…We compare the sensitivities of LIGO and LISA with those of the 100 m and 1 km stages of the AION terrestrial AI project, as well as two options for the proposed AEDGE AI space mission with cold atom clouds either inside or outside the spacecraft, considering as possible sources the mergers of black holes and neutron stars, supernovae, phase transitions in the early Universe, cosmic strings and quantum fluctuations in the early Universe that could have generated primordial black holes. …”
    Enlace del recurso
    Enlace del recurso
    Prospective Sensitivities of Atom Interferometers to Gravitational Waves and Ultralight Dark Matter
  11. 491
    por Astier, Pierre
    Publicado 2000
    “…Distance measurements to Type Ia supernovae (SNe Ia) at cosmological distances indicate that the Universe is accelerating and that a large fraction of the critical energy density exists in a component with negative pressure. …”
    Enlace del recurso
    Enlace del recurso
    Can luminosity distance measurements probe the equation of state of dark energy
  12. 492
    por Ackermann, Markus, Bustamante, Mauricio, Lu, Lu, Otte, Nepomuk, Reno, Mary Hall, Wissel, Stephanie, Agarwalla, Sanjib K., Alvarez-Muñiz, Jaime, Alves Batista, Rafael, Argüelles, Carlos A., Clark, Brian A., Cummings, Austin, Das, Sudipta, Decoene, Valentin, Denton, Peter B., Dornic, Damien, Dzhilkibaev, Zhan-Arys, Farzan, Yasaman, Garcia, Alfonso, Garzelli, Maria Vittoria, Glaser, Christian, Heijboer, Aart, Hörandel, Jörg R., Illuminati, Giulia, Jeong, Yu Seon, Kelley, John L., Kelly, Kevin J., Kheirandish, Ali, Klein, Spencer R., Krizmanic, John F., Larson, Michael J., Murase, Kohta, Narang, Ashish, Otte, Nepomuk, Prechelt, Remy L., Prohira, Steven, Resconi, Elisa, Santander, Marcos, Valera, Victor B., Vandenbroucke, Justin, Vasil'evna Suvorova, Olga, Wiencke, Lawrence, Yoshida, Shigeru, Yuan, Tianlu, Zas, Enrique, Zhelnin, Pavel, Zhou, Bei, Anchordoqui, Luis A., Ashida, Yosuke, Bagheri, Mahdi, Balagopal, Aswathi, V, Basu, Vedant, Beatty, James, Bechtol, Keith, Bell, Nicole, Bishop, Abigail, Book, Julia, Brown, Anthony, Burgman, Alexander, Campana, Michael, Chau, Nhan, Chen, Thomas Y., Coleman, Alan, Connolly, Amy, Conrad, Janet M., Correa, Pablo, Creque-Sarbinowski, Cyril, Curtis-Ginsberg, Zachary, Dasgupta, Paramita, De Kockere, Simon, de Vries, Krijn, Deaconu, Cosmin, Desai, Abhishek, DeYoung, Tyce, di Matteo, Armando, Elsaesser, Dominik, Fürst, Phillip, Kwok, Lung Fan, Fedynitch, Anatoli, Fox, Derek, Ganster, Erik, Ha Minh, Martin, Haack, Christian, Hallman, Steffen, Halzen, Francis, Haungs, Andreas, Ishihara, Aya, Judd, Eleanor, Karg, Timo, Karle, Albrecht, Katori, Teppei, Kochocki, Alina, Kopper, Claudio, Kowalski, Marek, Kravchenko, Ilya, Kurahashi, Naoko, Lamoureux, Mathieu, León Vargas, Hermes, Lincetto, Massimiliano, Liu, Qinrui, Madsen, Jim, Makino, Yuya, Mammo, Joseph, Marka, Zsuzsa, Mayotte, Eric, Meagher, Kevin, Meier, Maximilian, Miramonti, Lino, Moulai, Marjon, Mulrey, Katharine, Muzio, Marco, Naab, Richard, Nelles, Anna, Nichols, William, Nozdrina, Alisa, O'Sullivan, Erin, OD́ell, Vivian, Osborne, Jesse, Pandey, Vishvas, Paudel, Ek Narayan, Pizzuto, Alex, Plum, Mattias, Pobes Aranda, Carlos, Pyras, Lilly, Raab, Christoph, Rechav, Zoe, Rojo, Juan, Matamala, Oscar Romero, Savina, Pierpaolo, Schroeder, Frank, Schumacher, Lisa, Sciutto, Sergio, Sclafani, Stephen, Ful Hossain Seikh, Mohammad, Silva, Manuel, Singh, Rajeev, Smith, Daniel, Spencer, Samuel Timothy, Springer, Robert Wayne, Stachurska, Juliana, Suvorova, Olga Vasil'evna, Taboada, Ignacio, Toscano, Simona, Tueros, Matias, Twagirayezu, Jean Pierre, van Eijndhoven, Nick, Veres, Péter, Vieregg, Abigail, Wang, Winnie, Whitehorn, Nathan, Winter, Walter, Yildizci, Emre, Yu, Shiqi
    Publicado 2022
    “…With energies far beyond solar, supernovae, atmospheric, and accelerator neutrinos, high-energy and ultra-high-energy neutrinos probe fundamental physics from the TeV scale to the EeV scale and beyond. …”
    Enlace del recurso
    Enlace del recurso
    High-Energy and Ultra-High-Energy Neutrinos: A Snowmass White Paper
  13. 493
    por Patzak, T
    Publicado 2012
    “…These future megaton scale detectors are dedicated to nucleon decay, neutrinos from supernovæ, solar and atmospheric neutrinos, as well as neutrinos from a future Super-Beam or β-Beam to measure the mixing angle θ13 , the CP violating phase δ and the mass hierarchy.…”
    Enlace del recurso
    Enlace del recurso
    LAGUNA and LAGUNA-LBNO: Future megaton neutrino detectors in Europe
  14. 494
    por Tonazzo, Alessandra
    Publicado 2015
    “…The experiment will be able to cover important issues in particle physics (proton decay) and astrophysics (neutrinos from supernovae and from the sun). A neutrino beam from CERN, at a distance of 2300 km, will provide a unique potential for assessment of the neutrino mass hierarchy and exploration of CP violation in the leptonic sector. …”
    Enlace del recurso
    Enlace del recurso
    The LAGUNA-LBNO Project
  15. 495
    por Longair, Malcolm S
    Publicado 2008
    “…A very wide range of observational data is brought to bear upon these problems, including the most recent results from WMAP, the Hubble Space Telescope, galaxy surveys like the Sloan Digital Sky Survey and the 2dF Galaxy Redshift Survey, studies of Type 1a supernovae, and many other observations.…”
    Enlace del recurso
    Enlace del recurso
    Galaxy Formation
  16. 496
    por Rico, J
    Publicado 2002
    “…Its Physics program includes the study of atmospheric, solar, supernovae and beam neutrinos as well as proton decay searches. …”
    Enlace del recurso
    Status of ICARUS
  17. 497
    por Dar, A, De Rújula, Alvaro
    Publicado 2005
    “…There is mounting evidence that supernovae produce not only roughly spherical ejecta and winds, but also highly relativistic jets of ordinary matter. …”
    Enlace del recurso
    Enlace del recurso
    The Magnetic Field in Galaxies, Galaxy Clusters, and the InterGalactic Space
  18. 498
    por Signore, Monique, Blanchard, Alain
    Publicado 2005
    “…These pedagogical lectures cover major subjects relevant to the field ( inflation; CMB: anisotropies and polarization; quintessence/dark energy; inflation; CMB: anisotropies and polarization; clusters of galaxies; gravitational lensing; galaxy formation; dark matter; supernovae and the accelerating expansion of the Universe), providing invaluable introductory material appropriate to PhD students as well as to more senior scientists who wish to become familiar with the various domains of the modern developments in Cosmology…”
    Enlace del recurso
    Enlace del recurso
    NATO Advanced Study Institute on The Frontiers of Cosmology
  19. 499
    por Shapshak, Paul
    Publicado 2023
    “…This includes cool main-sequence, sub-giant, and red-giant stars. Additionally, supernovae, black holes, and neutron and dwarf stars, will be included to widen the investigation, since they sometimes have companions, including stars and planets. …”
    Enlace del recurso
    Enlace del recurso
    Enlace del recurso
    Online Artículo Texto
    Neutrino and EM asterometric detection of habitable exoplanets
  20. 500
    “…As a ubiquitous paradigm of instabilities and mixing that occur in instances as diverse as supernovae, plasma fusion, oil recovery, and nanofabrication, the Rayleigh–Taylor (RT) problem is rightly regarded as important. …”
    Enlace del recurso
    Enlace del recurso
    Enlace del recurso
    Online Artículo Texto
    Self-similar Rayleigh–Taylor mixing with accelerations varying in time and space
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