Pressure‐Induced sp 2 ‐sp 3 Transitions in Carbon‐Bearing Phases
Geophysical Monograph Series, Page 1-9., 2020 This book is Open Access. A digital copy can be downloaded for free from Wiley Online Library.
Explores the behavior of carbon in minerals, melts, and fluids under extreme conditions
Carbon trapped in diamonds and carbonate-bearing rocks in subduction zones are examples of the continuing exchange of substantial carbon ...
Sergey S. Lobanov +1 more
wiley +12 more sources
Studies of dark energy with X-ray observatories. [PDF]
Proc Natl Acad Sci U S A, 2010 I review the contribution of Chandra X-ray Observatory to studies of dark energy. There are two broad classes of observable effects of dark energy: evolution of the expansion rate of the Universe, and slow down in the rate of growth of cosmic structures. Chandra
Vikhlinin A.
europepmc +4 more sources
The X-Ray Observatory Suzaku [PDF]
Publications of the Astronomical Society of Japan, 2007 High-sensitivity wide-band X-ray spectroscopy is the key feature of the Suzaku X-ray observatory, launched on 2005 July 10. This paper summarizes the spacecraft, in-orbit performance, operations, and data processing that are related to observations. The scientific instruments, the high-throughput X-ray telescopes, X-ray CCD cameras, non-imaging hard X ...
Mitsuda, K. +142 more
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LOFT: a large observatory for x-ray timing [PDF]
SPIE Proceedings, 2010 The high time resolution observations of the X-ray sky hold the key to a number of diagnostics of fundamental physics, some of which are unaccessible to other types of investigations, such as those based on imaging and spectroscopy. Revealing strong gravitational field effects, measuring the mass and spin of black holes and the equation of state of ...
M. Feroci +48 more
openaire +7 more sources
The Large Observatory for x-ray timing [PDF]
SPIE Proceedings, 2014 Proc.
Feroci, M. +291 more
openaire +22 more sources
Predicted x-ray backgrounds for the International X-ray Observatory [PDF]
SPIE Proceedings, 2010 The background that will be observed by IXO's X-ray detectors naturally separates into two components: (1) a Cosmic X-ray Background (CXB), primarily due to unresolved point sources at high energies (E>2 keV), along with Galactic component(s) at lower energies that are generated in the disk and halo as well as the Local Bubble and charge exchange in ...
Bautz, Marshall W. +5 more
openaire +3 more sources
A portable CCD array detector for in-situ analysis of powder samples using combined x-ray diffraction/x-ray fluorescence techniques [PDF]
, 2010 This thesis was submitted for the degree of Doctor of Philosophy and awarded by Brunel University.This work describes the design, development and testing of a portable charge-coupled device detector system to be used for the simultaneous collection of X-
Intisar, Amir
core +6 more sources
The ASTRO-H X-ray Observatory [PDF]
SPIE Proceedings, 2012 The joint JAXA/NASA ASTRO-H mission is the sixth in a series of highly successful X-ray missions initiated by the Institute of Space and Astronautical Science (ISAS). ASTRO-H will investigate the physics of the high-energy universe via a suite of four instruments, covering a very wide energy range, from 0.3 keV to 600 keV.
Takahashi T. +210 more
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LOFT: the Large Observatory For X-ray Timing [PDF]
SPIE Proceedings, 2012 Proceedings of SPIE, Vol. 8443, Paper No.
M. Feroci +203 more
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The Large Observatory for X-ray Timing (LOFT) [PDF]
Experimental Astronomy, 2011 High-time-resolution X-ray observations of compact objects provide direct access to strong-field gravity, to the equation of state of ultradense matter and to black hole masses and spins. A 10 m(2)-class instrument in combination with good spectral resolution is required to exploit the relevant diagnostics and answer two of the fundamental questions of
M. Feroci +227 more
openaire +12 more sources