'3 kev' presentation slideshows

Energy calibration of the threshold of Medipix for ATLAS

669 views • 52 slides

Charmonium

Ted Barnes Physics Div. ORNL Dept. of Physics, U.Tenn. Charmonium. Charmonium. 1) Basic physics 2) Theoretical spectrum versus known states 3) NEW: open-flavor strong widths 4) E1 transitions 5) X(3872) The numbers quoted in 2-4) will appear in

584 views • 43 slides

+ Institute for Nuclear Research and Nuclear Energy, Sofia, Bulgaria

ON E0 TRANSITIONS BETWEEN 0 + STATES IN THE SAME NUCLEUS. V. P. Garistov + O.K. Egorov A.A. Solnyshkin ++. + Institute for Nuclear Research and Nuclear Energy, Sofia, Bulgaria ++ Joint Institute for Nuclear Research, Dubna, Russia.

553 views • 41 slides

Study of 17 O(p, ? ) 14 N reaction

458 views • 35 slides

Cosmology beyond the standard model Multi component dark matter model

480 views • 31 slides

Galactic wind in the bulge of the Andromeda galaxy

377 views • 27 slides

Status of Ultra-low Energy HPGe Detector for low-mass WIMP search

Status of Ultra-low Energy HPGe Detector for low-mass WIMP search. Li Xin (Tsinghua University) KIMS collaboration. Oct.22nd, 2005. Index. Motivation Previous status Current system setup Calibration Background data analysis Future plan. 5g Ge. 1cpd. Motivation.

473 views • 24 slides

384 views • 22 slides

K.L. Giboni, X. Ji, H. Lin, Y. Zhang, and L. Zhao Shanghai Jiao Tong University

367 views • 22 slides

The 3 He( ? , ? ) 7 Be prompt ? analysis and results

The 3 He( ? , ? ) 7 Be prompt ? analysis and results. Formulas. HPGe Efficiency. Efficienza %. Summary. 400 keV (1). 1757. Experimental spectrum. MC spectrum. 1329. 400 keV (2). Experimental spectrum. 429. MC spectrum. Angular distribution effects. Krawinkel et al 1982.

313 views • 20 slides

X-Ray Group Scaling Relations: Insights for Galaxy Formation

331 views • 19 slides

Thermal Emission from Isolated Neutron Stars:

Thermal Emission from Isolated Neutron Stars:. Spectral Features and Featureless Spectra. Silvia Zane, MSSL, UCL, UK. Congresso Nazionale Oggetti Compatti |||. Osservatorio Astronomico di Roma, 9-11 Dicembre 2003.

326 views • 17 slides

Next stage of a search for 2K(2 ? )-capture of 78 Kr

Next stage of a search for 2K(2 ? )-capture of 78 Kr. Valery V. Kuzminov Baksan Neutrino Observatory INR RAS. NON-ACCELERATOR NEW PHYSICS Dubna, Russia, June 20--25, 2005. Ju. Gavriljuk, V. Gavrin, A. Gangapshev, V. Kazalov, V. Kuzminov, N. Osetrova

275 views • 17 slides

Albert Kong and Rosanne Di Stefano

Observational Evidence for Quasi-soft X-Ray Sources in Nearby Galaxies and the link to Intermediate-mass Black Holes. Harvard-Smithsonian Center for Astrophysics. Albert Kong and Rosanne Di Stefano. X-ray Point Sources in Nearby Galaxies.

298 views • 17 slides

A Testable Conventional Hypothesis for the DAMA-LIBRA Annual Modulation Signal

A Testable Conventional Hypothesis for the DAMA-LIBRA Annual Modulation Signal. David Nygren LBNL. S is modulation signal amplitude: S = 0.0178 ?0.0020 (2-5 keV). from: arXiv 0804.2471. known background: potassium. Signal or Background: n, ?, ?, or ??.

257 views • 15 slides

The North Polar Spur: Detection of Nitrogen Enhancement with Suzaku

The North Polar Spur: Detection of Nitrogen Enhancement with Suzaku. Eric D. Miller (MIT) Hiroshi Tsunemi (Osaka. U) Mark Bautz (MIT) Dan McCammon (U. Wisconsin) Suzaku Science Working Group. North Polar Spur (NPS). region of enhanced soft X-ray, radio emission (Loop 1) nearby SNR?

343 views • 12 slides

6.7 keV

New Sources in the Sgr B & C Regions. 6.4 keV. 2.46 keV. 6.7 keV. Collisonal Ionization Z -4.3 EW of Fe~ 0.3 KeV O,Ne, Si, S, Fe : 360, 110, 70, 40, 290 eV 1.2: 0.38: 0.24: 0.14: 1 0.11: 0.06: 0.05: 0.04: 1 Cross Section of photo ionization Z -2.3 EW of Fe~1 keV

194 views • 10 slides

Structural and scaling properties of galaxy clusters Probing the physics of structure formation

193 views • 8 slides

Long-tem solar neutrino flux and geological 205 Pb assay

142 views • 1 slides

2 The XMM observation of Abell 2028

Apparent high metallicity in 3-4 keV clusters: The inverse iron-bias in action in Abell 2028. F. Gastaldello 1,2,3 , S. Ettori 4 1 INAF-IASF Milan, 2 University of California Irvine, 3 Occhialini Fellow, 4 INAF-Bologna. Abstract

162 views • 1 slides