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Observation of the 1S-2S transition in trapped antihydrogen.
Ahmadi, M; Alves, B X R; Baker, C J; Bertsche, W; Butler, E; Capra, A; Carruth, C; Cesar, C L; Charlton, M; Cohen, S; Collister, R; Eriksson, S; Evans, A; Evetts, N; Fajans, J; Friesen, T; Fujiwara, M C; Gill, D R; Gutierrez, A; Hangst, J S; Hardy, W N; Hayden, M E; Isaac, C A; Ishida, A; Johnson, M A; Jones, S A; Jonsell, S; Kurchaninov, L; Madsen, N; Mathers, M; Maxwell, D; McKenna, J T K; Menary, S; Michan, J M; Momose, T; Munich, J J; Nolan, P; Olchanski, K; Olin, A; Pusa, P; Rasmussen, C Ø; Robicheaux, F; Sacramento, R L; Sameed, M; Sarid, E; Silveira, D M; Stracka, S; Stutter, G; So, C; Tharp, T D.
Afiliação
  • Ahmadi M; Department of Physics, University of Liverpool, Liverpool L69 7ZE, UK.
  • Alves BX; Department of Physics and Astronomy, Aarhus University, DK-8000 Aarhus C, Denmark.
  • Baker CJ; Department of Physics, College of Science, Swansea University, Swansea SA2 8PP, UK.
  • Bertsche W; School of Physics and Astronomy, University of Manchester, Manchester M12 9PL, UK.
  • Butler E; Cockcroft Institute, Sci-Tech Daresbury, Warrington WA4 4AD, UK.
  • Capra A; Physics Department, CERN, CH-1211 Geneve 23, Switzerland.
  • Carruth C; TRIUMF, 4004 Wesbrook Mall, Vancouver, British Columbia V6T 2A3, Canada.
  • Cesar CL; Department of Physics, University of California at Berkeley, Berkeley, California 94720-7300, USA.
  • Charlton M; Instituto de Fisica, Universidade Federal do Rio de Janeiro, Rio de Janeiro 21941-972, Brazil.
  • Cohen S; Department of Physics, College of Science, Swansea University, Swansea SA2 8PP, UK.
  • Collister R; Department of Physics, Ben-Gurion University of the Negev, Beer-Sheva 84105, Israel.
  • Eriksson S; TRIUMF, 4004 Wesbrook Mall, Vancouver, British Columbia V6T 2A3, Canada.
  • Evans A; Department of Physics, College of Science, Swansea University, Swansea SA2 8PP, UK.
  • Evetts N; Department of Physics and Astronomy, University of Calgary, Calgary, Alberta T2N 1N4, Canada.
  • Fajans J; Department of Physics and Astronomy, University of British Columbia, Vancouver, British Columbia V6T 1Z1, Canada.
  • Friesen T; Department of Physics, University of California at Berkeley, Berkeley, California 94720-7300, USA.
  • Fujiwara MC; Department of Physics and Astronomy, Aarhus University, DK-8000 Aarhus C, Denmark.
  • Gill DR; TRIUMF, 4004 Wesbrook Mall, Vancouver, British Columbia V6T 2A3, Canada.
  • Gutierrez A; TRIUMF, 4004 Wesbrook Mall, Vancouver, British Columbia V6T 2A3, Canada.
  • Hangst JS; Department of Medical Physics and Biomedical Engineering, University College London, London WC1E 6BT, UK.
  • Hardy WN; Department of Physics and Astronomy, Aarhus University, DK-8000 Aarhus C, Denmark.
  • Hayden ME; Department of Physics and Astronomy, University of British Columbia, Vancouver, British Columbia V6T 1Z1, Canada.
  • Isaac CA; Department of Physics, Simon Fraser University, Burnaby, British Columbia V5A 1S6, Canada.
  • Ishida A; Department of Physics, College of Science, Swansea University, Swansea SA2 8PP, UK.
  • Johnson MA; Department of Physics, The University of Tokyo, 7-3-1 Hongo, Bunkyo, Tokyo 113-0033, Japan.
  • Jones SA; School of Physics and Astronomy, University of Manchester, Manchester M12 9PL, UK.
  • Jonsell S; Cockcroft Institute, Sci-Tech Daresbury, Warrington WA4 4AD, UK.
  • Kurchaninov L; Department of Physics, College of Science, Swansea University, Swansea SA2 8PP, UK.
  • Madsen N; Department of Physics, Stockholm University, SE-10691 Stockholm, Sweden.
  • Mathers M; TRIUMF, 4004 Wesbrook Mall, Vancouver, British Columbia V6T 2A3, Canada.
  • Maxwell D; Department of Physics, College of Science, Swansea University, Swansea SA2 8PP, UK.
  • McKenna JT; Department of Physics and Astronomy, York University, Toronto, Ontario M3J 1P3, Canada.
  • Menary S; Department of Physics, College of Science, Swansea University, Swansea SA2 8PP, UK.
  • Michan JM; TRIUMF, 4004 Wesbrook Mall, Vancouver, British Columbia V6T 2A3, Canada.
  • Momose T; Department of Physics and Astronomy, York University, Toronto, Ontario M3J 1P3, Canada.
  • Munich JJ; TRIUMF, 4004 Wesbrook Mall, Vancouver, British Columbia V6T 2A3, Canada.
  • Nolan P; École Polytechnique Fédérale de Lausanne (EPFL), Swiss Plasma Center (SPC), Lausanne CH-1015, Switzerland.
  • Olchanski K; Department of Physics and Astronomy, University of British Columbia, Vancouver, British Columbia V6T 1Z1, Canada.
  • Olin A; Department of Physics, Simon Fraser University, Burnaby, British Columbia V5A 1S6, Canada.
  • Pusa P; Department of Physics, University of Liverpool, Liverpool L69 7ZE, UK.
  • Rasmussen CØ; TRIUMF, 4004 Wesbrook Mall, Vancouver, British Columbia V6T 2A3, Canada.
  • Robicheaux F; TRIUMF, 4004 Wesbrook Mall, Vancouver, British Columbia V6T 2A3, Canada.
  • Sacramento RL; Department of Physics and Astronomy, University of Victoria, Victoria, British Columbia V8P 5C2, Canada.
  • Sameed M; Department of Physics, University of Liverpool, Liverpool L69 7ZE, UK.
  • Sarid E; Department of Physics and Astronomy, Aarhus University, DK-8000 Aarhus C, Denmark.
  • Silveira DM; Department of Physics and Astronomy, Purdue University, West Lafayette, Indiana 47907, USA.
  • Stracka S; Instituto de Fisica, Universidade Federal do Rio de Janeiro, Rio de Janeiro 21941-972, Brazil.
  • Stutter G; Department of Physics, College of Science, Swansea University, Swansea SA2 8PP, UK.
  • So C; Soreq NRC, Yavne 81800, Israel.
  • Tharp TD; Instituto de Fisica, Universidade Federal do Rio de Janeiro, Rio de Janeiro 21941-972, Brazil.
Nature ; 541(7638): 506-510, 2017 01 26.
Article em En | MEDLINE | ID: mdl-28005057
ABSTRACT
The spectrum of the hydrogen atom has played a central part in fundamental physics over the past 200 years. Historical examples of its importance include the wavelength measurements of absorption lines in the solar spectrum by Fraunhofer, the identification of transition lines by Balmer, Lyman and others, the empirical description of allowed wavelengths by Rydberg, the quantum model of Bohr, the capability of quantum electrodynamics to precisely predict transition frequencies, and modern measurements of the 1S-2S transition by Hänsch to a precision of a few parts in 1015. Recent technological advances have allowed us to focus on antihydrogen-the antimatter equivalent of hydrogen. The Standard Model predicts that there should have been equal amounts of matter and antimatter in the primordial Universe after the Big Bang, but today's Universe is observed to consist almost entirely of ordinary matter. This motivates the study of antimatter, to see if there is a small asymmetry in the laws of physics that govern the two types of matter. In particular, the CPT (charge conjugation, parity reversal and time reversal) theorem, a cornerstone of the Standard Model, requires that hydrogen and antihydrogen have the same spectrum. Here we report the observation of the 1S-2S transition in magnetically trapped atoms of antihydrogen. We determine that the frequency of the transition, which is driven by two photons from a laser at 243 nanometres, is consistent with that expected for hydrogen in the same environment. This laser excitation of a quantum state of an atom of antimatter represents the most precise measurement performed on an anti-atom. Our result is consistent with CPT invariance at a relative precision of about 2 × 10-10.

Texto completo: 1 Bases de dados: MEDLINE Tipo de estudo: Prognostic_studies Idioma: En Revista: Nature Ano de publicação: 2017 Tipo de documento: Article País de afiliação: Reino Unido

Texto completo: 1 Bases de dados: MEDLINE Tipo de estudo: Prognostic_studies Idioma: En Revista: Nature Ano de publicação: 2017 Tipo de documento: Article País de afiliação: Reino Unido