منابع مشابه
Atoms embedded in an electron gas: Phase shifts and cross sections
Rights: © 1983 American Physical Society (APS). This is the accepted version of the following article: Puska, M. J. & Nieminen, Risto M. 1983. Atoms embedded in an electron gas: Phase shifts and cross sections. Physical Review B. Volume 27, Issue 10. 6121-6128. ISSN 1550-235X (electronic). DOI: 10.1103/physrevb.27.6121, which has been published in final form at http://journals.aps.org/prb/abstr...
متن کاملAtoms embedded in an electron gas: Beyond the local-density approximation.
Rights: © 1991 American Physical Society (APS). This is the accepted version of the following article: Puska, M. J. & Nieminen, Risto M. 1991. Atoms embedded in an electron gas: Beyond the local-density approximation. Physical Review B. Volume 43, Issue 15. 12221-12233. ISSN 1550-235X (electronic). DOI: 10.1103/physrevb.43.12221, which has been published in final form at http://journals.aps.org...
متن کاملMolecular Gas in Galactic Nuclei
Dense molecular clouds are critical to the activity occurring in galactic nuclei. They are the active component from which starbursts arise, and this dense interstellar gas may be the fuel for AGNs. In both the nearby infrared bright galaxies (eg. M82, NGC 253, and IC342) and the ultralu-minous IRAS galaxies, high resolution millimeter line mapping has shown extremely high gas surface densities...
متن کاملLocalization Bounds for an Electron Gas
Mathematical analysis of the Anderson localization has been facilitated by the use of suitable fractional moments of the Green function. Related methods permit now a readily accessible derivation of a number of physical manifestations of localization, in regimes of strong disorder, extreme energies, or weak disorder away from the unperturbed spectrum. The present work establishes on this basis ...
متن کاملGas and Dust in Ultraluminous Galactic Nuclei
Millimeter-wave interferometry has clearly shown the existence of enormous masses (10 9 ?10 10 M) of molecular gas concentrated in the nuclear regions (R <500 pc) of many luminous and ultraluminous infrared galaxies. In these systems, molecular gas is an obvious source of fuel for nuclear starbursts and active galactic nuclei (AGN). In several ultraluminous systems (e.g., Arp 220 and Mrk 231), ...
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ژورنال
عنوان ژورنال: Physical Review C
سال: 2007
ISSN: 0556-2813,1089-490X
DOI: 10.1103/physrevc.76.034310