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KETTŐS REZONANCIA GRAFIT és SZÉN NANOCSÖVEK RAMAN SPEKTRUMÁBAN

KETTŐS REZONANCIA GRAFIT és SZÉN NANOCSÖVEK RAMAN SPEKTRUMÁBAN

KETTŐS REZONANCIA GRAFIT és SZÉN NANOCSÖVEK RAMAN SPEKTRUMÁBAN. MTA SZFKI , 2005. április 4. Kürti Jenő ELTE Biológiai Fizika Tanszék e-mail: kurti@virag.elte.hu www: virag.elte.hu/~kurti. VÁZLAT. Bevezetés

By jera
(143 views)

KETTŐS REZONANCIA GRAFIT és SZÉN NANOCSÖVEK RAMAN SPEKTRUMÁBAN

KETTŐS REZONANCIA GRAFIT és SZÉN NANOCSÖVEK RAMAN SPEKTRUMÁBAN

KETTŐS REZONANCIA GRAFIT és SZÉN NANOCSÖVEK RAMAN SPEKTRUMÁBAN. MTA SZFKI , 2005. április 4. Kürti Jenő ELTE Biológiai Fizika Tanszék e-mail: kurti@virag.elte.hu www: virag.elte.hu/~kurti. VÁZLAT. Bevezetés

By chaeli
(142 views)

Fourth Annual Meeting of the „European Network of Theoretical Astroparticle Physics (ENTApP)“

Fourth Annual Meeting of the „European Network of Theoretical Astroparticle Physics (ENTApP)“

Fourth Annual Meeting of the „European Network of Theoretical Astroparticle Physics (ENTApP)“. Physics of Massive Neutrinos MILOS, May 19. to 23. 2008. Organizers : Amand Faessler , Tuebingen Haris Kosmas, Ioannina Jose Valle, Valencia.

By kyrie
(94 views)

F.Bertram et al. Material Science and Engineering B93 (2002) 19-23

F.Bertram et al. Material Science and Engineering B93 (2002) 19-23

Spatial variation of luminescence of InGaN alloys measured by highly-spatially-resolved scanning cathodoluminescence. F.Bertram et al. Material Science and Engineering B93 (2002) 19-23. Itoh Lab. Takahiro Doki. Contents. ・ Introduction -InGaN -Cathodoluminescence ・ Motivation

By bailey
(92 views)

Ionization: A key chemical pathway in ices under radiation environment?

Ionization: A key chemical pathway in ices under radiation environment?

Ionization: A key chemical pathway in ices under radiation environment?. Murthy S. Gudipati Jet Propulsion Laboratory, California Institute of Technology, 4800 Oak Grove Drive, Pasadena, CA 91109. Contents. Radiation, Ice and Organic Impurities Ionization - A Quick Tour

By shaman
(84 views)

Particles and Waves

Particles and Waves

Particles and Waves. Early Atom Models. Democritus (2500 years ago)—tiny indivisible particles, atmos Dalton (1803) Each element composed of extremely small particles Atoms of any element are identical and different from others Atoms not created or destroyed

By dakota
(136 views)

Measurement of neutrino mass with cryogenic detectors

Measurement of neutrino mass with cryogenic detectors

Measurement of neutrino mass with cryogenic detectors. The birth of the neutrino. Neutrino oscillations => neutrino mass ≠ 0. <m n > from Cosmology. m  = 0 eV. m  = 1 eV. m  = 7 eV. m  = 4 eV. S <m n > <.4-.7 eV. Measurement (or limit ) on neutrino mass by single beta decay.

By silver
(123 views)

Development of Thin Film and Nanorod ZnO-Based LEDs and Sensors

Development of Thin Film and Nanorod ZnO-Based LEDs and Sensors

Development of Thin Film and Nanorod ZnO-Based LEDs and Sensors.

By geona
(157 views)

Cosmological mass bounds on hot-dark matter axions

Cosmological mass bounds on hot-dark matter axions

NOW 2008- Neutrino Oscillation Workshop Conca Specchiulla, September 6-13 2008. Cosmological mass bounds on hot-dark matter axions. Alessandro MIRIZZI (MPI, Munich). [based on works in collaboration with S.Hannestad, G.G. Raffelt, Y.Y.Y. Wong]. OUTLINE. Strong CP problem and the axions

By celina
(97 views)

Neutrino physics : The future

Neutrino physics : The future

Neutrino physics : The future. Gabriela Barenboim TAU 04. We know that neutrinos are massive and oscillate !. Evidence for flavor change. Solar neutrinos: Compelling evidence. n e. f n e + f n m + f n t. 1. =. f n e. Pure n e source. 3. Reactor neutrinos: very strong evidence.

By louvain
(133 views)

Quantum Tunnelling

Quantum Tunnelling

Quantum Physics 2002. Quantum Tunnelling. Recommended Reading: R.Harris, Chapter 5 Sections 1, 2 and 3. Potential Barrier: E < U 0. I. II. III. U = U 0. E = K.E. E = K.E. U. x =L. x. x =0. Region III. Region I. Region II. 1. Potential. where. and. Wavefunctions.

By ganesa
(262 views)

Claudia Lederer

Claudia Lederer

Status of the 62 Ni(n, g ) analysis. Claudia Lederer. n_TOF collaboration meeting, 15.-17. 12. 2010, Seville. Measurement. C 6 D 6 detection setup sample: highly enriched in 62 Ni, 2 cm Ø, 2 g 197 Au, 2 cm Ø, 0.6 g nat Pb, 2 cm Ø, 0.3 g nat C, 2 cm Ø, 5 g. Claudia Lederer.

By erna
(188 views)

J.-E. Wahlund, A. I. Eriksson, M. W. Morooka, G. Gustafsson, R. Boström, R. Modolo

J.-E. Wahlund, A. I. Eriksson, M. W. Morooka, G. Gustafsson, R. Boström, R. Modolo

RPWS Cold Plasma Results from the Inner Magnetosphere of Saturn – dust-plasma interaction near the E-ring?. J.-E. Wahlund, A. I. Eriksson, M. W. Morooka, G. Gustafsson, R. Boström, R. Modolo Swedish Institute of Space Physics, Uppsala T. F. Averkamp, G. B. Hospodarsky, W. S. Kurth

By harvey
(114 views)

MARE

MARE

MARE. M icrocalorimeter A rrays for a R henium E xperiment. A DETECTOR OVERVIEW. Andrea Giuliani , University of Insubria, Como, and INFN Milano on behalf of the MARE collaboration. Outline of the talk. The physics case: importance of direct m n measurement

By asabi
(225 views)

ECE 874: Physical Electronics

ECE 874: Physical Electronics

ECE 874: Physical Electronics. Prof. Virginia Ayres Electrical & Computer Engineering Michigan State University ayresv@msu.edu. Lecture 09, 27 Sep 12.

By suzy
(112 views)

Molecular simulation on radiation behavior of Li 2 O

Molecular simulation on radiation behavior of Li 2 O

Molecular simulation on radiation behavior of Li 2 O. Takuji Oda , Yasuhisa Oya, Satoru Tanaka Department of Quantum Engineering & Systems Science The University of Tokyo. Background. 6 Li + n → 4 He (2.1 MeV) + T (2.7 MeV).

By kirby
(166 views)

Evolution of Ni-Al interface alloy for Ni deposited on Al surfaces at room temperature

Evolution of Ni-Al interface alloy for Ni deposited on Al surfaces at room temperature

Evolution of Ni-Al interface alloy for Ni deposited on Al surfaces at room temperature. R. J. Smith and V. Shutthanandan* Physics Department, Montana State Univ. *Currently at EMSL, PNNL, Richland WA Work supported by NSF http://www.physics.montana.edu. Metal-metal Interface Structure.

By lane
(79 views)

Fragmentation of molecules: Franck-Condon model

Fragmentation of molecules: Franck-Condon model

Photo double ionization of H 2 resp. of D 2 or the correlated motion of electrons in a two center coulomb potential. Fragmentation of molecules: Franck-Condon model Experimental technique: Imaging of the momentum space Dynamics of the electrons in a single and a two center potential.

By neviah
(152 views)

CRACOW EPIPHANY CONFERENCE ON NEUTRINOS AND DARK MATTER 5 - 7 January 2006, Cracow, Poland

CRACOW EPIPHANY CONFERENCE ON NEUTRINOS AND DARK MATTER 5 - 7 January 2006, Cracow, Poland

Status of the KATRIN experiment. CRACOW EPIPHANY CONFERENCE ON NEUTRINOS AND DARK MATTER 5 - 7 January 2006, Cracow, Poland. Jochen Bonn Johannes Gutenberg Universität Mainz Jochen.Bonn@uni-mainz.de. Introduction Neutrino mass determination The Karlsruhe TRItium Neutrino experiment KATRIN

By zuwena
(105 views)

Direct Measurements of the Neutrino Mass

Direct Measurements of the Neutrino Mass

Direct Measurements of the Neutrino Mass. Klaus Eitel Forschungszentrum Karlsruhe Institute for Nuclear Physics klaus.eitel@ik.fzk.de. Direct Measurements of the Neutrino Mass. neutrino masses in particle physics & cosmology (mass scenarios, n ´s as HDM) micro-calorimeters

By hollis
(119 views)

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