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Hyperfine Interactions

, Volume 209, Issue 1–3, pp 139–143 | Cite as

Kaonic 3He and 4He X-ray measurements in SIDDHARTA

  • Tomoichi IshiwatariEmail author
  • M. Bazzi
  • G. Beer
  • C. Berucci
  • L. Bombelli
  • A. M. Bragadireanu
  • M. Cargnelli
  • A. Clozza
  • G. Corradi
  • C. Curceanu (Petrascu)
  • A. d’Uffizi
  • C. Fiorini
  • F. Ghio
  • B. Girolami
  • C. Guaraldo
  • R. S. Hayano
  • M. Iliescu
  • M. Iwasaki
  • P. Kienle
  • P. Levi Sandri
  • V. Lucherini
  • J. Marton
  • S. Okada
  • D. Pietreanu
  • K. Piscicchia
  • M. Poli Lener
  • T. Ponta
  • R. Quaglia
  • A. Rizzo
  • A. Romero Vidal
  • E. Sbardella
  • A. Scordo
  • H. Shi
  • D. L. Sirghi
  • F. Sirghi
  • H. Tatsuno
  • A. Tudorache
  • V. Tudorache
  • O. Vazquez Doce
  • E. Widmann
  • B. Wünschek
  • J. Zmeskal
Open Access
Article

Abstract

The SIDDHARTA experiment measured the kaonic 3He and 4He 3d →2p X-ray transitions using gaseous targets for the first time. The strong-interaction shift both of the kaonic 3He and 4He 2p states was determined with a precision of a few eV. The shift of kaonic 4He is much smaller than the values obtained in the experiments performed in 70’s and 80’s, while it is consistent with the recent result of the KEK E570 experiment, as well as the theoretical calculated values. Therefore, the problem on kaonic helium (the “kaonic helium puzzle”) was definitely solved. The first observation of the kaonic 3He X-rays was also achieved in the SIDDHARTA experiment. The shift both of kaonic 3He and 4He was found to be as small as a few eV.

Keywords

Kaonic helium Silicon drift detectors X-ray spectroscopy 

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Copyright information

© The Author(s) 2012

Open AccessThis is an open access article distributed under the terms of the Creative Commons Attribution Noncommercial License (https://creativecommons.org/licenses/by-nc/2.0), which permits any noncommercial use, distribution, and reproduction in any medium, provided the original author(s) and source are credited.

Authors and Affiliations

  • Tomoichi Ishiwatari
    • 1
    Email author
  • M. Bazzi
    • 2
  • G. Beer
    • 3
  • C. Berucci
    • 2
  • L. Bombelli
    • 4
  • A. M. Bragadireanu
    • 2
    • 5
  • M. Cargnelli
    • 1
  • A. Clozza
    • 2
  • G. Corradi
    • 2
  • C. Curceanu (Petrascu)
    • 2
  • A. d’Uffizi
    • 2
  • C. Fiorini
    • 4
  • F. Ghio
    • 6
  • B. Girolami
    • 6
  • C. Guaraldo
    • 2
  • R. S. Hayano
    • 7
  • M. Iliescu
    • 2
    • 5
  • M. Iwasaki
    • 8
  • P. Kienle
    • 9
  • P. Levi Sandri
    • 2
  • V. Lucherini
    • 2
  • J. Marton
    • 1
  • S. Okada
    • 2
  • D. Pietreanu
    • 5
  • K. Piscicchia
    • 2
  • M. Poli Lener
    • 2
  • T. Ponta
    • 5
  • R. Quaglia
    • 4
  • A. Rizzo
    • 2
  • A. Romero Vidal
    • 2
  • E. Sbardella
    • 2
  • A. Scordo
    • 2
  • H. Shi
    • 7
  • D. L. Sirghi
    • 2
    • 5
  • F. Sirghi
    • 2
    • 5
  • H. Tatsuno
    • 2
  • A. Tudorache
    • 5
  • V. Tudorache
    • 5
  • O. Vazquez Doce
    • 2
  • E. Widmann
    • 1
  • B. Wünschek
    • 1
  • J. Zmeskal
    • 1
  1. 1.Stefan-Meyer-Institut für subatomare PhysikViennaAustria
  2. 2.INFNLaboratori Nazionali di FrascatiFrascati (Roma)Italy
  3. 3.Department of Phys. and Astro.University of VictoriaVictoria B.C.Canada
  4. 4.Sez. di ElettronicaPolitechno di MilanoMilanoItaly
  5. 5.IFIN-HHBucharestRomania
  6. 6.INFN Sez. di Roma I and Inst. Superiore di SanitaRomaItaly
  7. 7.Univ. of TokyoTokyoJapan
  8. 8.RIKENThe Inst. of Phys. and Chem. ResearchSaitamaJapan
  9. 9.Physik Dep.Tech. Univ. MünchenGarchingGermany

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