'Radiative decay' diaporamas de présentation

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The Charmonium Spectrum

The Charmonium Spectrum

The Charmonium Spectrum. Spectroscopic Notation. n 2S+1 L J. The J/ ?(1 3 S 0 ) and the ??(2 3 S 0 ). The masses of the triplet S states have been measured very precisely in e + e - collision (using resonant depolarization) and in ?pp annihilation at Fermilab (E760)

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Search for m ?e g with the MEG experiment at PSI: results and prospects

Search for m ?e g with the MEG experiment at PSI: results and prospects

Search for m ?e g with the MEG experiment at PSI: results and prospects. A.M. Baldini March 23rd for the MEG collaboration. Hep-ex:0908.2594v1 18 Aug 2009. Most recent m + ? e + g Experiments (Hincks and Pontecorvo 1948). Two orders of magnitude improvement

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What can we learn about X resonances at K1.8

What can we learn about X resonances at K1.8

J-PARC Hadron physics WS 2014.11.30. What can we learn about X resonances at K1.8. K.Imai (JAEA). X resonances in PDG. PDG Table of X. X * quark model: Chao, Isgur, Karl PRD 23 (1981). X (1690)J P ?. X (1820)3/2-. X (1530)3/2+. L (1520)3/2-. L (1405)1/2-.

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Controlling the thickness of CuCl thin films and improving their quality by means of MBE method

Controlling the thickness of CuCl thin films and improving their quality by means of MBE method

Controlling the thickness of CuCl thin films and improving their quality by means of MBE method. Ashida lab. M1 K amizono Kenta. Contents. Introduction All-optical switching devices Excitons and light in the high-quality system Background Previous results

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Lepton flavor violation in ? + ? e + ? decay: results from the MEG experiment

Lepton flavor violation in ? + ? e + ? decay: results from the MEG experiment

Lepton flavor violation in ? + ? e + ? decay: results from the MEG experiment. Cecilia Voena INFN Roma on behalf of the MEG collaboration. FPCP 2010 Torino 25-29 May 2010. Outline. History of ? + ?>e + ? searches Physics motivation Experimental technique

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1.51k views • 33 slides
Decaying Gravitino Dark Matter

Decaying Gravitino Dark Matter

Decaying Gravitino Dark Matter. Are Raklev University of Cambridge In collaboration with Deirdre Black (Cambridge), Nils-Erik Bomark (Bergen), Magda Lola (Patras), Emanuel Malek (Cambridge), Per Osland (Bergen) and Helen Vryonidou (Cambridge). Based on Lola, Osland, ARR, arXiv:0707.2510

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MEG ?? ???????????? ????????

MEG ?? ???????????? ????????

MEG ?? ???????????? ????????. Yuki Fujii On behalf of the MEG collaboration JPS meeting @ Hirosaki University 17 th Sep. 2011. Outline. Introduction Run 2009 & 2010 Status of run 2011 Noise reduction Summary and prospects. Introduction. ?.

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Speaker: Bao-Xi Sun Institute of Theoretical Physics, Beijing University of Technology

Speaker: Bao-Xi Sun Institute of Theoretical Physics, Beijing University of Technology

Dynamically generated resonances from the vector octet-baryon decuplet interaction in the hidden gauge formalism. Speaker: Bao-Xi Sun Institute of Theoretical Physics, Beijing University of Technology Collaborators: S. Sarkar, E.Oset and M. J. VicenteVacas 2009.08.24 IWND2009(Shanghai).

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293 views • 22 slides
Speaker: Bao-Xi Sun Institute of Theoretical Physics, Beijing University of Technology

Speaker: Bao-Xi Sun Institute of Theoretical Physics, Beijing University of Technology

Dynamically generated resonances from the vector octet-baryon decuplet interaction in the hidden gauge formalism. Speaker: Bao-Xi Sun Institute of Theoretical Physics, Beijing University of Technology Collaborators: S. Sarkar, E.Oset and M. J. VicenteVacas 2009.4.20 Nstar2009(Beijing).

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321 views • 22 slides
Xiang Liu xiangliu@lzu School of Physical Science and Technology Lanzhou University

Xiang Liu xiangliu@lzu School of Physical Science and Technology Lanzhou University

The oddball Y(4140) as the cousin of Y(3930). Xiang Liu xiangliu@lzu.edu.cn School of Physical Science and Technology Lanzhou University. Xiang Liu & S. L. Zhu, Phys.Rev.D80, 017502 (2009) Xiang Liu, Z. G. Luo, Y. R. Liu and S. L. Zhu, Eur.Phys.J.C61:411-428 (2009)

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STERILE NEUTRINOS and WARM DARK MATTER

STERILE NEUTRINOS and WARM DARK MATTER

STERILE NEUTRINOS and WARM DARK MATTER. The n MSM model. T. Asaka and M. Shaposhnikov Phys.Lett.B620(2005)17 M.Shaposhnokov Nucl.Phys.B763(2007)49 Minimum extension of the SM to accomodate massive neutrinos See-saw formula for active neutrinos m n =-M D (1/M I )(M D ) T

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?????????????????? MEG ?????? muon radiative decays ??????

?????????????????? MEG ?????? muon radiative decays ??????

?????????????????? MEG ?????? muon radiative decays ??????. ? muon radiative events ??????????????? ?. ????????????????? ?????? MEG Collaboration. Contents. MEG Physics MEG and muon radiative decay events Trigger Consideration

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279 views • 12 slides
Star Formation and Band 11

Star Formation and Band 11

CO 9-8. CO 13-12. CO 11-10. CO 12-11. Star Formation and Band 11. J. Cernicharo CAB. INTA-CSIC Spain. CO 10-9. Thanks to Ed Bergin , Asuncion Fuente, B. Lefloch, Javier R. Goicoechea and M. Extaluze for some viewgraphs and suggestions. Dust and Molecules.

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