... We achieve this by using as pick-ups small quarter-wave coupling loops, positioned underneath and above the tail region, in such a place that they are sensitive to the extreme tail, but much less to the far-away dense core. ...
[
Текст
]
Ссылки http://nuclphys.sinp.msu.ru/experiment/detectors/meer-lecture.pdf -- 393.2 Кб -- 25.10.2006 Похожие документы
... These remnants of DM clumps form the low-mass tail in the standard mass distribution of small-scale clumps extended much b elow Mmin of the standard distribution. ...
[
Текст
]
Ссылки http://nuclphys.sinp.msu.ru/conf/lpp14/210809/Berezinsky_Dokuch_Erosh.pdf -- 233.2 Кб -- 16.09.2009 Похожие документы
... M = 2 p p l MW: sensitive to the edge of M T T T T (1 - cos l ) W: sensitive to the tail of MT Andrew Askew, 14th Lomonosov conference 10 DЬ WWidth Result: DЬ uses central electrons only, and 1 fb of data. ...
... variables: bl · Resolution is different among channels, worse for channel with electrons: spread dominated by radiative losses, with larger tails in negative regions ec spread dominated by tracking resolution 08/15/2009 Marcello A. Giorgi 8 Search for ...
Measurement of the cosmic ray electron spectrum with FERMI in the energy region 20 GeV 1 TeV Alexandre Chekhtman George Mason University / Naval Research Laboratory for the Fermi LAT Collaboration 1 Alexandre Chekhtman 14 Lomonosov ...
[
Текст
]
Ссылки http://nuclphys.sinp.msu.ru/conf/lpp14/210809/Chekhtman.pdf -- 1853.9 Кб -- 16.09.2009 Похожие документы
... 37 On the tail of the distribution very heavy BH may be created, MB H 107M. A mechanism of early quasar formation with evolved chemistry - one of the mysteries of the standard model. ...
... Thus, we deal with some tail-head instability leading to a growing concentration of par ticles wherever a small per turbation star ted to occur. ...
[
Текст
]
Ссылки http://nuclphys.sinp.msu.ru/conf/XFEL/XFEL-TDR_Chapter01_Introduction.pdf -- 1724.6 Кб -- 30.03.2010 Похожие документы
... i + 2I The shortcomings of the metho d. It is (i) physically clear but not-well-grounded enough; (ii) valid in the p ole approximation, i.e. only in the GR energy region (in implementations far low- and/or high-energy tails are the subject of interest ...
... We think that this remark should be taken into account, when placing upper bounds on hep from the analysis of the high-energy tail of the SK spectrum. ...