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Characterization of the 1S-2S transition in antihydrogen.
Ahmadi, M; Alves, B X R; Baker, C J; Bertsche, W; 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; Hangst, J S; Hardy, W N; Hayden, M E; Isaac, C A; Johnson, M A; Jones, J M; Jones, S A; Jonsell, S; Khramov, A; Knapp, P; Kurchaninov, L; Madsen, N; Maxwell, D; McKenna, J T K; Menary, S; Momose, T; Munich, J J; Olchanski, K; Olin, A; Pusa, P; Rasmussen, C Ø; Robicheaux, F; Sacramento, R L; Sameed, M; Sarid, E; Silveira, D M; Stutter, G; So, C; Tharp, T D; Thompson, R I; van der Werf, D P; Wurtele, J S.
  • Ahmadi M; Department of Physics, University of Liverpool, Liverpool, UK.
  • Alves BXR; Department of Physics and Astronomy, Aarhus University, Aarhus, Denmark.
  • Baker CJ; Department of Physics, College of Science, Swansea University, Swansea, UK.
  • Bertsche W; School of Physics and Astronomy, University of Manchester, Manchester, UK.
  • Capra A; Cockcroft Institute, Sci-Tech Daresbury, Warrington, UK.
  • Carruth C; TRIUMF, 4004 Wesbrook Mall, Vancouver, British Columbia, Canada.
  • Cesar CL; Department of Physics, University of California at Berkeley, Berkeley, CA, USA.
  • Charlton M; Instituto de Fisica, Universidade Federal do Rio de Janeiro, Rio de Janeiro, Brazil.
  • Cohen S; Department of Physics, College of Science, Swansea University, Swansea, UK.
  • Collister R; Department of Physics, Ben-Gurion University of the Negev, Beer-Sheva, Israel.
  • Eriksson S; TRIUMF, 4004 Wesbrook Mall, Vancouver, British Columbia, Canada.
  • Evans A; Department of Physics, College of Science, Swansea University, Swansea, UK.
  • Evetts N; Department of Physics and Astronomy, University of Calgary, Calgary, Alberta, Canada.
  • Fajans J; Department of Physics and Astronomy, University of British Columbia, Vancouver, British Columbia, Canada.
  • Friesen T; Department of Physics, University of California at Berkeley, Berkeley, CA, USA.
  • Fujiwara MC; Department of Physics and Astronomy, Aarhus University, Aarhus, Denmark.
  • Gill DR; TRIUMF, 4004 Wesbrook Mall, Vancouver, British Columbia, Canada.
  • Hangst JS; TRIUMF, 4004 Wesbrook Mall, Vancouver, British Columbia, Canada.
  • Hardy WN; Department of Physics and Astronomy, Aarhus University, Aarhus, Denmark. jeffrey.hangst@cern.ch.
  • Hayden ME; Department of Physics and Astronomy, University of British Columbia, Vancouver, British Columbia, Canada.
  • Isaac CA; Department of Physics, Simon Fraser University, Burnaby, British Columbia, Canada.
  • Johnson MA; Department of Physics, College of Science, Swansea University, Swansea, UK.
  • Jones JM; School of Physics and Astronomy, University of Manchester, Manchester, UK.
  • Jones SA; Cockcroft Institute, Sci-Tech Daresbury, Warrington, UK.
  • Jonsell S; Department of Physics, College of Science, Swansea University, Swansea, UK.
  • Khramov A; Department of Physics and Astronomy, Aarhus University, Aarhus, Denmark.
  • Knapp P; Department of Physics, College of Science, Swansea University, Swansea, UK.
  • Kurchaninov L; Department of Physics, Stockholm University, Stockholm, Sweden.
  • Madsen N; TRIUMF, 4004 Wesbrook Mall, Vancouver, British Columbia, Canada.
  • Maxwell D; Department of Physics, College of Science, Swansea University, Swansea, UK.
  • McKenna JTK; TRIUMF, 4004 Wesbrook Mall, Vancouver, British Columbia, Canada.
  • Menary S; Department of Physics, College of Science, Swansea University, Swansea, UK.
  • Momose T; Department of Physics, College of Science, Swansea University, Swansea, UK.
  • Munich JJ; TRIUMF, 4004 Wesbrook Mall, Vancouver, British Columbia, Canada.
  • Olchanski K; Department of Physics and Astronomy, York University, Toronto, Ontario, Canada.
  • Olin A; Department of Physics and Astronomy, University of British Columbia, Vancouver, British Columbia, Canada.
  • Pusa P; Department of Physics, Simon Fraser University, Burnaby, British Columbia, Canada.
  • Rasmussen CØ; TRIUMF, 4004 Wesbrook Mall, Vancouver, British Columbia, Canada.
  • Robicheaux F; TRIUMF, 4004 Wesbrook Mall, Vancouver, British Columbia, Canada.
  • Sacramento RL; Department of Physics and Astronomy, University of Victoria, Victoria, British Columbia, Canada.
  • Sameed M; Department of Physics, University of Liverpool, Liverpool, UK.
  • Sarid E; Department of Physics and Astronomy, Aarhus University, Aarhus, Denmark.
  • Silveira DM; Department of Physics and Astronomy, Purdue University, West Lafayette, IN, USA.
  • Stutter G; Instituto de Fisica, Universidade Federal do Rio de Janeiro, Rio de Janeiro, Brazil.
  • So C; Department of Physics, College of Science, Swansea University, Swansea, UK.
  • Tharp TD; School of Physics and Astronomy, University of Manchester, Manchester, UK.
  • Thompson RI; Soreq NRC, Yavne, Israel.
  • van der Werf DP; Instituto de Fisica, Universidade Federal do Rio de Janeiro, Rio de Janeiro, Brazil.
  • Wurtele JS; Department of Physics and Astronomy, Aarhus University, Aarhus, Denmark.
Nature ; 557(7703): 71-75, 2018 05.
Article en En | MEDLINE | ID: mdl-29618820
ABSTRACT
In 1928, Dirac published an equation 1 that combined quantum mechanics and special relativity. Negative-energy solutions to this equation, rather than being unphysical as initially thought, represented a class of hitherto unobserved and unimagined particles-antimatter. The existence of particles of antimatter was confirmed with the discovery of the positron 2 (or anti-electron) by Anderson in 1932, but it is still unknown why matter, rather than antimatter, survived after the Big Bang. As a result, experimental studies of antimatter3-7, including tests of fundamental symmetries such as charge-parity and charge-parity-time, and searches for evidence of primordial antimatter, such as antihelium nuclei, have high priority in contemporary physics research. The fundamental role of the hydrogen atom in the evolution of the Universe and in the historical development of our understanding of quantum physics makes its antimatter counterpart-the antihydrogen atom-of particular interest. Current standard-model physics requires that hydrogen and antihydrogen have the same energy levels and spectral lines. The laser-driven 1S-2S transition was recently observed 8 in antihydrogen. Here we characterize one of the hyperfine components of this transition using magnetically trapped atoms of antihydrogen and compare it to model calculations for hydrogen in our apparatus. We find that the shape of the spectral line agrees very well with that expected for hydrogen and that the resonance frequency agrees with that in hydrogen to about 5 kilohertz out of 2.5 × 1015 hertz. This is consistent with charge-parity-time invariance at a relative precision of 2 × 10-12-two orders of magnitude more precise than the previous determination 8 -corresponding to an absolute energy sensitivity of 2 × 10-20 GeV.

Texto completo: 1 Banco de datos: MEDLINE Tipo de estudio: Prognostic_studies Idioma: En Año: 2018 Tipo del documento: Article

Texto completo: 1 Banco de datos: MEDLINE Tipo de estudio: Prognostic_studies Idioma: En Año: 2018 Tipo del documento: Article