Resonant soft x-ray scattering – a new probe of charge, spin, and orbital ordering in the manganites.
(2005)
Journal Article
Hatton, P., Wilkins, S., Beale, T., Johal, T., Prabhakaran, D., & Boothroyd, A. (2005). Resonant soft x-ray scattering – a new probe of charge, spin, and orbital ordering in the manganites. Journal of Magnetism and Magnetic Materials, 290-291(2), 891-897. https://doi.org/10.1016/j.jmmm.2004.11.283
Outputs (283)
A New approach to inclusive decay spectra. (2005)
Presentation / Conference Contribution
Gardi, E., & Andersen, J. R. (2005, April). A New approach to inclusive decay spectra. Presented at 40th Rencontres de Moriond on QCD and High Energy Hadronic Interactions, La Thuile, Aosta ValleyThe main obstacle in describing inclusive decay spectra in QCD - which, in particular, limits the precision in extrapolating the measured \bar{B} \to X(s) gamma rate to the full phase space as well as in extracting |Vub||Vub| from inclusive measureme... Read More about A New approach to inclusive decay spectra..
Discovery of extended VHE gamma-ray emission from the asymmetric pulsar wind nebula in MSH 15-52 with HESS (2005)
Journal Article
Aharonian, F., Akhperjanian, A., Aye, K., Bazer-Bachi, A., Beilicke, M., Benbow, W., …Wagner, S. (2005). Discovery of extended VHE gamma-ray emission from the asymmetric pulsar wind nebula in MSH 15-52 with HESS. Astronomy & Astrophysics, 435(1), L17-L20. https://doi.org/10.1051/0004-6361%3A200500105The Supernova Remnant MSH 15-52 has been observed in very high energy (VHE) γ-rays using the HESS 4-telescope array located in Namibia. A γ-ray signal is detected at the 25 sigma level during an exposure of 22.1 h live time. The image reveals an elli... Read More about Discovery of extended VHE gamma-ray emission from the asymmetric pulsar wind nebula in MSH 15-52 with HESS.
The metal enrichment of the intracluster medium in hierarchical galaxy formation models (2005)
Journal Article
Nagashima, M., Lacey, C., Baugh, C., Frenk, C., & Cole, S. (2005). The metal enrichment of the intracluster medium in hierarchical galaxy formation models. Monthly Notices of the Royal Astronomical Society, 358(4), 1247-1266. https://doi.org/10.1111/j.1365-2966.2005.08766.xWe investigate the metal enrichment of the intracluster medium (ICM) within the framework of hierarchical models of galaxy formation. We calculate the formation and evolution of galaxies and clusters using a semi-analytical model which includes the e... Read More about The metal enrichment of the intracluster medium in hierarchical galaxy formation models.
Diffractive W + 2 jet production: a background to exclusive H \to WW production at hadron colliders (2005)
Preprint / Working Paper
Khoze, V., Ryskin, M., & Stirling, W. (2005). Diffractive W + 2 jet production: a background to exclusive H \to WW production at hadron colliders
Rapid growth of black holes in massive star-forming galaxies (2005)
Journal Article
Alexander, D., Smail, I., Bauer, F., Chapman, S., Blain, A., Brandt, W., & Ivison, R. (2005). Rapid growth of black holes in massive star-forming galaxies. Nature, 434(7034), 738-740. https://doi.org/10.1038/nature03473
Search for TeV emission from the region around PSR B1706-44 with the HESS experiment (2005)
Journal Article
Aharonian, F., Akhperjanian, A., Aye, K., Bazer-Bachi, A., Beilicke, M., Benbow, W., …Wagner, S. (2005). Search for TeV emission from the region around PSR B1706-44 with the HESS experiment. Astronomy & Astrophysics, 432(1), L9-L12. https://doi.org/10.1051/0004-6361%3A200500008The region around PSR B1706–44 has been observed with the HESS imaging atmospheric Cherenkov telescopes in 2003. No evidence for γ-ray emission in the TeV range was found at the pulsar position or at the radio arc which corresponds to the supernova r... Read More about Search for TeV emission from the region around PSR B1706-44 with the HESS experiment.
White polymeric light-emitting diode based on a fluorene polymer/Ir complex blend system (2005)
Journal Article
Al Attar, H., Monkman, A., Tavasli, M., Bettington, S., & Bryce, M. (2005). White polymeric light-emitting diode based on a fluorene polymer/Ir complex blend system. Applied Physics Letters, 86(12),Efficient white-polymeric light-emitting diodes (PLED) were fabricated as a single active layer containing blue-emitting poly(9,9-bis(2-ethylhexyl)fluorene-2,7-diyl) endcapped with bis(4-methylphenyl)phenylamine; (PF2/6am4), and yellow-orange-emittin... Read More about White polymeric light-emitting diode based on a fluorene polymer/Ir complex blend system.
Quantum-mechanical cumulant dynamics near stable periodic orbits in phase space: Application to the classical-like dynamics of quantum accelerator modes (2005)
Journal Article
Bach, R., Burnett, K., d'Arcy, M., & Gardiner, S. (2005). Quantum-mechanical cumulant dynamics near stable periodic orbits in phase space: Application to the classical-like dynamics of quantum accelerator modes. Physical Review A, 71, https://doi.org/10.1103/physreva.71.033417We formulate a general method for the study of semiclassical-like dynamics in stable regions of a mixed phase space, in order to theoretically study the dynamics of quantum accelerator modes. In the simplest case, this involves determining solutions,... Read More about Quantum-mechanical cumulant dynamics near stable periodic orbits in phase space: Application to the classical-like dynamics of quantum accelerator modes.
A new population of very high energy gamma-ray sources in the Milky Way (2005)
Journal Article
Aharonian, F., Akhperjanian, A., Aye, K., Bazer-Bachi, A., Beilicke, M., Benbow, W., …Wagner, S. (2005). A new population of very high energy gamma-ray sources in the Milky Way. Science, 307(5717), 1938-1942. https://doi.org/10.1126/science.1108643Very high energy {gamma}-rays probe the long-standing mystery of the origin of cosmic rays. Produced in the interactions of accelerated particles in astrophysical objects, they can be used to image cosmic particle accelerators. A first sensitive surv... Read More about A new population of very high energy gamma-ray sources in the Milky Way.