Results 101 to 110 of about 419,552 (318)

Electron Density Structure Measurements With Scattered Intense Laser Beam

Contributions to Plasma Physics, EarlyView.
ABSTRACT Short‐pulse intense lasers have the potential to model extreme astrophysical environments in laboratories. Although there are diagnostics for energetic electrons and ions resulting from laser‐plasma interactions, the diagnostics to measure velocity distribution functions at the interaction region of the laser and plasma are limited.
K. Sakai, K. Himeno, S. J. Tanaka, T. Asai, T. Minami, Y. Abe, F. Nikaido, K. Kuramoto, M. Kanasaki, H. Kiriyama, A. Kon, K. Kondo, N. Nakanii, W. Y. Woon, C. M. Chu, K. T. Wu, C. S. Jao, Y. L. Liu, T. A. Pikuz, H. Kohri, A. O. Tokiyasu, S. Isayama, H. S. Kumar, K. Tomita, Y. Fukuda, Y. Kuramitsu   +25 more
wiley   +1 more source

Mirage (David Ralph Viviers)

Tydskrif vir Letterkunde, 2023
Paul Stephen Walters
doaj   +1 more source

On Relativistic Astrophysics.

The Astrophysical Journal, 1964
Catastrophic implosion analysis in stars with masses greater than critical mass in which general relativity becomes ...
William A. Fowler, Fred Hoyle, Geoffrey Burbidge, E. Margaret Burbidge   +3 more
openaire   +3 more sources

Predicting the Uniform Electron Gas Stopping Power at Moderate and Strong Coupling

Contributions to Plasma Physics, EarlyView.
ABSTRACT This paper presents a detailed study of the stopping power of a homogeneous electron gas in moderate and strong coupling regimes using the self‐consistent version of the method of moments as the key theoretical approach capable of expressing the dynamic characteristics of the system in terms of the static ones, which are the moments.
Saule A. Syzganbayeva, Alexey V. Filinov, Jesús Ara, Assel B. Ashikbayeva, Abdiadil Askaruly, Lazzat T. Yerimbetova, Manuel D. Barriga‐Carrasco, Yuriy V. Arkhipov, Igor M. Tkachenko   +8 more
wiley   +1 more source

Dynamical Analysis of the Redshift Drift in FLRW Universes

Universe
Redshift drift is the phenomenon whereby the observed redshift between an emitter and observer comoving with the Hubble flow in an expanding FLRW universe will slowly evolve—on a timescale comparable to the Hubble time.
Francisco S. N. Lobo, José Pedro Mimoso, Jessica Santiago, Matt Visser   +3 more
doaj   +1 more source

eScience Symposium Reflections from Christopher Erdmann: Redefining the Librarian’s Role in eScience

Journal of eScience Librarianship, 2016
Christopher Erdmann, Head Librarian, Wolbach Library, Harvard Smithsonian Center for Astrophysics, shares his multiple experiences at the University of Massachusetts and New England Area Librarian eScience Symposium, as well as current challenges he sees
Christopher Erdmann
doaj   +1 more source

Numerical Modeling of Isochoric Heating Experiments Using the Troll Code in the Warm Dense Matter Regime

Contributions to Plasma Physics, EarlyView.
ABSTRACT Experiments of isochoric heating by protons of solid material were recently performed at LULI laser facilities. In these experiments, protons, produced from target normal sheath acceleration (TNSA) of Au foil with the PICO2000 laser, deposit their energy into an aluminum or copper foil initially at room temperature and solid density.
Sébastien Rassou, Marie Bonneau, Christophe Rousseaux, Xavier Vaisseau, Witold Cayzac, Adrien Denoeud, Frédéric Perez, Tom Beaumont, Morris Demoulins, Jean‐Christophe Pain   +9 more
wiley   +1 more source

Narrating the origin of the universe through music: A case study [PDF]

Zbornik Radova Akademije Umetnosti, 2017
Our project is about the synthesis of a musical piece, based on the timeline of the Universe. We can understand music through visual and gestural analogies.
Mannone Maria, Gkoudina Kyriaki, Tyler Evan   +2 more
doaj  

Dark Matter Astrophysics

, 2009
These lectures are intended to provide a brief pedagogical review of dark matter for the newcomer to the subject. We begin with a discussion of the astrophysical evidence for dark matter.
D'Amico, Guido, Kamionkowski, Marc, Sigurdson, Kris   +2 more
core  

Parity Violation in Astrophysics

, 2004
Core collapse supernovae are gigantic explosions of massive stars that radiate 99% of their energy in neutrinos. This provides a unique opportunity for large scale parity or charge conjugation violation.
B.A. Brown, C.J. Horowitz, C.J. Horowitz, C.J. Horowitz, C.J. Horowitz, C.J. Horowitz, C.J. Horowitz, C.S. Wood, J. Carriere, J. Pons, J.M. Lattimer   +10 more
core   +1 more source