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Glöggler LT, Gusakova N, Rienäcker B, Camper A, Caravita R, Huck S, Volponi M, Wolz T, Penasa L, Krumins V, Gustafsson FP, Comparat D, Auzins M, Bergmann B, Burian P, Brusa RS, Castelli F, Cerchiari G, Ciuryło R, Consolati G, Doser M, Graczykowski Ł, Grosbart M, Guatieri F, Haider S, Janik MA, Kasprowicz G, Khatri G, Kłosowski Ł, Kornakov G, Lappo L, Linek A, Malamant J, Mariazzi S, Petracek V, Piwiński M, Pospíšil S, Povolo L, Prelz F, Rangwala SA, Rauschendorfer T, Rawat BS, Rodin V, Røhne OM, Sandaker H, Smolyanskiy P, Sowiński T, Tefelski D, Vafeiadis T, Welsch CP, Zawada M, Zielinski J, Zurlo N. Positronium Laser Cooling via the 1^{3}S-2^{3}P Transition with a Broadband Laser Pulse. PHYSICAL REVIEW LETTERS 2024; 132:083402. [PMID: 38457696 DOI: 10.1103/physrevlett.132.083402] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 10/13/2023] [Accepted: 01/18/2024] [Indexed: 03/10/2024]
Abstract
We report on laser cooling of a large fraction of positronium (Ps) in free flight by strongly saturating the 1^{3}S-2^{3}P transition with a broadband, long-pulsed 243 nm alexandrite laser. The ground state Ps cloud is produced in a magnetic and electric field-free environment. We observe two different laser-induced effects. The first effect is an increase in the number of atoms in the ground state after the time Ps has spent in the long-lived 2^{3}P states. The second effect is one-dimensional Doppler cooling of Ps, reducing the cloud's temperature from 380(20) to 170(20) K. We demonstrate a 58(9)% increase in the fraction of Ps atoms with v_{1D}<3.7×10^{4} ms^{-1}.
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Affiliation(s)
- L T Glöggler
- Physics Department, CERN, 1211 Geneva 23, Switzerland
| | - N Gusakova
- Physics Department, CERN, 1211 Geneva 23, Switzerland
- Department of Physics, NTNU, Norwegian University of Science and Technology, Trondheim, Norway
| | - B Rienäcker
- Department of Physics, University of Liverpool, Liverpool L69 3BX, United Kingdom
| | - A Camper
- Department of Physics, University of Oslo, Sem Sælandsvei 24, 0371 Oslo, Norway
| | - R Caravita
- TIFPA/INFN Trento, via Sommarive 14, 38123 Povo, Trento, Italy
| | - S Huck
- Physics Department, CERN, 1211 Geneva 23, Switzerland
- Institute for Experimental Physics, Universität Hamburg, 22607 Hamburg, Germany
| | - M Volponi
- Physics Department, CERN, 1211 Geneva 23, Switzerland
- TIFPA/INFN Trento, via Sommarive 14, 38123 Povo, Trento, Italy
- Department of Physics, University of Trento, via Sommarive 14, 38123 Povo, Trento, Italy
| | - T Wolz
- Physics Department, CERN, 1211 Geneva 23, Switzerland
| | - L Penasa
- TIFPA/INFN Trento, via Sommarive 14, 38123 Povo, Trento, Italy
- Department of Physics, University of Trento, via Sommarive 14, 38123 Povo, Trento, Italy
| | - V Krumins
- Physics Department, CERN, 1211 Geneva 23, Switzerland
- University of Latvia, Department of Physics Raina boulevard 19, LV-1586 Riga, Latvia
| | | | - D Comparat
- Université Paris-Saclay, CNRS, Laboratoire Aimé Cotton, 91405 Orsay, France
| | - M Auzins
- University of Latvia, Department of Physics Raina boulevard 19, LV-1586 Riga, Latvia
| | - B Bergmann
- Institute of Experimental and Applied Physics, Czech Technical University in Prague, Husova 240/5, 110 00 Prague 1, Czech Republic
| | - P Burian
- Institute of Experimental and Applied Physics, Czech Technical University in Prague, Husova 240/5, 110 00 Prague 1, Czech Republic
| | - R S Brusa
- TIFPA/INFN Trento, via Sommarive 14, 38123 Povo, Trento, Italy
- Department of Physics, University of Trento, via Sommarive 14, 38123 Povo, Trento, Italy
| | - F Castelli
- INFN Milano, via Celoria 16, 20133 Milano, Italy
- Department of Physics "Aldo Pontremoli," University of Milano, via Celoria 16, 20133 Milano, Italy
| | - G Cerchiari
- Institut für Experimentalphysik, University of Innsbruck, Technikerstrasse 25, 6020 Innsbruck, Austria
| | - R Ciuryło
- Institute of Physics, Faculty of Physics, Astronomy, and Informatics, Nicolaus Copernicus University in Torun, Grudziadzka 5, 87-100 Torun, Poland
| | - G Consolati
- INFN Milano, via Celoria 16, 20133 Milano, Italy
- Department of Aerospace Science and Technology, Politecnico di Milano, via La Masa 34, 20156 Milano, Italy
| | - M Doser
- Physics Department, CERN, 1211 Geneva 23, Switzerland
| | - Ł Graczykowski
- Warsaw University of Technology, Faculty of Physics, ul. Koszykowa 75, 00-662 Warsaw, Poland
| | - M Grosbart
- Physics Department, CERN, 1211 Geneva 23, Switzerland
| | - F Guatieri
- TIFPA/INFN Trento, via Sommarive 14, 38123 Povo, Trento, Italy
- Department of Physics, University of Trento, via Sommarive 14, 38123 Povo, Trento, Italy
| | - S Haider
- Physics Department, CERN, 1211 Geneva 23, Switzerland
| | - M A Janik
- Warsaw University of Technology, Faculty of Physics, ul. Koszykowa 75, 00-662 Warsaw, Poland
| | - G Kasprowicz
- Warsaw University of Technology, Faculty of Electronics and Information Technology, ul. Nowowiejska 15/19, 00-665 Warsaw, Poland
| | - G Khatri
- Physics Department, CERN, 1211 Geneva 23, Switzerland
| | - Ł Kłosowski
- Institute of Physics, Faculty of Physics, Astronomy, and Informatics, Nicolaus Copernicus University in Torun, Grudziadzka 5, 87-100 Torun, Poland
| | - G Kornakov
- Warsaw University of Technology, Faculty of Physics, ul. Koszykowa 75, 00-662 Warsaw, Poland
| | - L Lappo
- Warsaw University of Technology, Faculty of Physics, ul. Koszykowa 75, 00-662 Warsaw, Poland
| | - A Linek
- Institute of Physics, Faculty of Physics, Astronomy, and Informatics, Nicolaus Copernicus University in Torun, Grudziadzka 5, 87-100 Torun, Poland
| | - J Malamant
- Department of Physics, University of Oslo, Sem Sælandsvei 24, 0371 Oslo, Norway
| | - S Mariazzi
- TIFPA/INFN Trento, via Sommarive 14, 38123 Povo, Trento, Italy
- Department of Physics, University of Trento, via Sommarive 14, 38123 Povo, Trento, Italy
| | - V Petracek
- Czech Technical University, Prague, Brehova 7, 11519 Prague 1, Czech Republic
| | - M Piwiński
- Institute of Physics, Faculty of Physics, Astronomy, and Informatics, Nicolaus Copernicus University in Torun, Grudziadzka 5, 87-100 Torun, Poland
| | - S Pospíšil
- Institute of Experimental and Applied Physics, Czech Technical University in Prague, Husova 240/5, 110 00 Prague 1, Czech Republic
| | - L Povolo
- TIFPA/INFN Trento, via Sommarive 14, 38123 Povo, Trento, Italy
- Department of Physics, University of Trento, via Sommarive 14, 38123 Povo, Trento, Italy
| | - F Prelz
- INFN Milano, via Celoria 16, 20133 Milano, Italy
| | - S A Rangwala
- Raman Research Institute, C. V. Raman Avenue, Sadashivanagar, Bangalore 560080, India
| | - T Rauschendorfer
- Physics Department, CERN, 1211 Geneva 23, Switzerland
- Felix Bloch Institute for Solid State Physics, Universität Leipzig, 04103 Leipzig, Germany
| | - B S Rawat
- Department of Physics, University of Liverpool, Liverpool L69 3BX, United Kingdom
- The Cockcroft Institute, Daresbury, Warrington WA4 4AD, United Kingdom
| | - V Rodin
- Department of Physics, University of Liverpool, Liverpool L69 3BX, United Kingdom
| | - O M Røhne
- Department of Physics, University of Oslo, Sem Sælandsvei 24, 0371 Oslo, Norway
| | - H Sandaker
- Department of Physics, University of Oslo, Sem Sælandsvei 24, 0371 Oslo, Norway
| | - P Smolyanskiy
- Institute of Experimental and Applied Physics, Czech Technical University in Prague, Husova 240/5, 110 00 Prague 1, Czech Republic
| | - T Sowiński
- Institute of Physics, Polish Academy of Sciences, Aleja Lotnikow 32/46, PL-02668 Warsaw, Poland
| | - D Tefelski
- Warsaw University of Technology, Faculty of Physics, ul. Koszykowa 75, 00-662 Warsaw, Poland
| | - T Vafeiadis
- Physics Department, CERN, 1211 Geneva 23, Switzerland
| | - C P Welsch
- Department of Physics, University of Liverpool, Liverpool L69 3BX, United Kingdom
- The Cockcroft Institute, Daresbury, Warrington WA4 4AD, United Kingdom
| | - M Zawada
- Institute of Physics, Faculty of Physics, Astronomy, and Informatics, Nicolaus Copernicus University in Torun, Grudziadzka 5, 87-100 Torun, Poland
| | - J Zielinski
- Warsaw University of Technology, Faculty of Physics, ul. Koszykowa 75, 00-662 Warsaw, Poland
| | - N Zurlo
- INFN Pavia, via Bassi 6, 27100 Pavia, Italy
- Department of Civil, Environmental, Architectural Engineering and Mathematics, University of Brescia, via Branze 43, 25123 Brescia, Italy
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Charry J, Varella MTDN, Reyes A. Binding Matter with Antimatter: The Covalent Positron Bond. Angew Chem Int Ed Engl 2018; 57:8859-8864. [DOI: 10.1002/anie.201800914] [Citation(s) in RCA: 13] [Impact Index Per Article: 2.2] [Reference Citation Analysis] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Received: 01/22/2018] [Indexed: 11/09/2022]
Affiliation(s)
- Jorge Charry
- Universidad Nacional de Colombia Chemistry; Av. cra 30 #45-03 Bogota, 00000 Colombia
| | - Márcio T. do N. Varella
- Instituto de Física; Universidade de São Paulo; Rua do Matão 1731 05508-090 São Paulo, SP Brazil
| | - Andrés Reyes
- Universidad Nacional de Colombia Chemistry; Av. cra 30 #45-03 Bogota, 00000 Colombia
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Doser M, Aghion S, Amsler C, Bonomi G, Brusa RS, Caccia M, Caravita R, Castelli F, Cerchiari G, Comparat D, Consolati G, Demetrio A, Di Noto L, Evans C, Fanì M, Ferragut R, Fesel J, Fontana A, Gerber S, Giammarchi M, Gligorova A, Guatieri F, Haider S, Hinterberger A, Holmestad H, Kellerbauer A, Khalidova O, Krasnický D, Lagomarsino V, Lansonneur P, Lebrun P, Malbrunot C, Mariazzi S, Marton J, Matveev V, Mazzotta Z, Müller SR, Nebbia G, Nedelec P, Oberthaler M, Pacifico N, Pagano D, Penasa L, Petracek V, Prelz F, Prevedelli M, Rienaecker B, Robert J, Røhne OM, Rotondi A, Sandaker H, Santoro R, Smestad L, Sorrentino F, Testera G, Tietje IC, Widmann E, Yzombard P, Zimmer C, Zmeskal J, Zurlo N. AEgIS at ELENA: outlook for physics with a pulsed cold antihydrogen beam. PHILOSOPHICAL TRANSACTIONS. SERIES A, MATHEMATICAL, PHYSICAL, AND ENGINEERING SCIENCES 2018; 376:20170274. [PMID: 29459413 PMCID: PMC5829176 DOI: 10.1098/rsta.2017.0274] [Citation(s) in RCA: 3] [Impact Index Per Article: 0.5] [Reference Citation Analysis] [Abstract] [Key Words] [Grants] [Track Full Text] [Subscribe] [Scholar Register] [Accepted: 12/05/2017] [Indexed: 06/08/2023]
Abstract
The efficient production of cold antihydrogen atoms in particle traps at CERN's Antiproton Decelerator has opened up the possibility of performing direct measurements of the Earth's gravitational acceleration on purely antimatter bodies. The goal of the AEgIS collaboration is to measure the value of g for antimatter using a pulsed source of cold antihydrogen and a Moiré deflectometer/Talbot-Lau interferometer. The same antihydrogen beam is also very well suited to measuring precisely the ground-state hyperfine splitting of the anti-atom. The antihydrogen formation mechanism chosen by AEgIS is resonant charge exchange between cold antiprotons and Rydberg positronium. A series of technical developments regarding positrons and positronium (Ps formation in a dedicated room-temperature target, spectroscopy of the n=1-3 and n=3-15 transitions in Ps, Ps formation in a target at 10 K inside the 1 T magnetic field of the experiment) as well as antiprotons (high-efficiency trapping of [Formula: see text], radial compression to sub-millimetre radii of mixed [Formula: see text] plasmas in 1 T field, high-efficiency transfer of [Formula: see text] to the antihydrogen production trap using an in-flight launch and recapture procedure) were successfully implemented. Two further critical steps that are germane mainly to charge exchange formation of antihydrogen-cooling of antiprotons and formation of a beam of antihydrogen-are being addressed in parallel. The coming of ELENA will allow, in the very near future, the number of trappable antiprotons to be increased by more than a factor of 50. For the antihydrogen production scheme chosen by AEgIS, this will be reflected in a corresponding increase of produced antihydrogen atoms, leading to a significant reduction of measurement times and providing a path towards high-precision measurements.This article is part of the Theo Murphy meeting issue 'Antiproton physics in the ELENA era'.
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Affiliation(s)
- M Doser
- Physics Department, CERN, 1211 Geneva 23, Switzerland
| | - S Aghion
- Politecnico of Milano, Piazza Leonardo da Vinci 32, 20133 Milano, Italy
- INFN Milano, via Celoria 16, 20133 Milano, Italy
| | - C Amsler
- Stefan Meyer Institute for Subatomic Physics, Austrian Academy of Sciences, Boltzmanngasse 3, 1090 Vienna, Austria
| | - G Bonomi
- Department of Mechanical and Industrial Engineering, University of Brescia, via Branze 38, 25123 Brescia, Italy
- INFN Pavia, via Bassi 6, 27100 Pavia, Italy
| | - R S Brusa
- Department of Physics, University of Trento, via Sommarive 14, 38123 Povo, Trento, Italy
- TIFPA/INFN Trento, via Sommarive 14, 38123 Povo, Trento, Italy
| | - M Caccia
- INFN Milano, via Celoria 16, 20133 Milano, Italy
- Department of Science, University of Insubria, via Valleggio 11, 22100 Como, Italy
| | - R Caravita
- Department of Physics, University of Genova, via Dodecaneso 33, 16146 Genova, Italy
- INFN Genova, via Dodecaneso 33, 16146 Genova, Italy
| | - F Castelli
- INFN Milano, via Celoria 16, 20133 Milano, Italy
- Department of Physics, University of Milano, via Celoria 16, 20133 Milano, Italy
| | - G Cerchiari
- Max Planck Institute for Nuclear Physics, Saupfercheckweg 1, 69117 Heidelberg, Germany
| | - D Comparat
- Laboratoire Aimé Cotton, Université Paris-Sud, ENS Cachan, CNRS, Université Paris-Saclay, 91405 Orsay Cedex, France
| | - G Consolati
- Politecnico of Milano, Piazza Leonardo da Vinci 32, 20133 Milano, Italy
- INFN Milano, via Celoria 16, 20133 Milano, Italy
| | - A Demetrio
- Kirchhoff-Institute for Physics, Heidelberg University, Im Neuenheimer Feld 227, 69120 Heidelberg, Germany
| | - L Di Noto
- Department of Physics, University of Genova, via Dodecaneso 33, 16146 Genova, Italy
- INFN Genova, via Dodecaneso 33, 16146 Genova, Italy
| | - C Evans
- Politecnico of Milano, Piazza Leonardo da Vinci 32, 20133 Milano, Italy
- INFN Milano, via Celoria 16, 20133 Milano, Italy
| | - M Fanì
- Physics Department, CERN, 1211 Geneva 23, Switzerland
- Department of Physics, University of Genova, via Dodecaneso 33, 16146 Genova, Italy
- INFN Genova, via Dodecaneso 33, 16146 Genova, Italy
| | - R Ferragut
- Politecnico of Milano, Piazza Leonardo da Vinci 32, 20133 Milano, Italy
- INFN Milano, via Celoria 16, 20133 Milano, Italy
| | - J Fesel
- Physics Department, CERN, 1211 Geneva 23, Switzerland
| | - A Fontana
- INFN Pavia, via Bassi 6, 27100 Pavia, Italy
| | - S Gerber
- Physics Department, CERN, 1211 Geneva 23, Switzerland
| | - M Giammarchi
- INFN Milano, via Celoria 16, 20133 Milano, Italy
| | - A Gligorova
- Stefan Meyer Institute for Subatomic Physics, Austrian Academy of Sciences, Boltzmanngasse 3, 1090 Vienna, Austria
| | - F Guatieri
- Department of Physics, University of Trento, via Sommarive 14, 38123 Povo, Trento, Italy
- TIFPA/INFN Trento, via Sommarive 14, 38123 Povo, Trento, Italy
| | - S Haider
- Physics Department, CERN, 1211 Geneva 23, Switzerland
| | | | - H Holmestad
- Department of Physics, University of Oslo, Sem Slandsvei 24, 0371 Oslo, Norway
| | - A Kellerbauer
- Max Planck Institute for Nuclear Physics, Saupfercheckweg 1, 69117 Heidelberg, Germany
| | - O Khalidova
- Physics Department, CERN, 1211 Geneva 23, Switzerland
| | - D Krasnický
- INFN Genova, via Dodecaneso 33, 16146 Genova, Italy
| | - V Lagomarsino
- Department of Physics, University of Genova, via Dodecaneso 33, 16146 Genova, Italy
- INFN Genova, via Dodecaneso 33, 16146 Genova, Italy
| | - P Lansonneur
- Institute of Nuclear Physics, CNRS/IN2p3, University of Lyon 1, 69622 Villeurbanne, France
| | - P Lebrun
- Institute of Nuclear Physics, CNRS/IN2p3, University of Lyon 1, 69622 Villeurbanne, France
| | - C Malbrunot
- Physics Department, CERN, 1211 Geneva 23, Switzerland
- Stefan Meyer Institute for Subatomic Physics, Austrian Academy of Sciences, Boltzmanngasse 3, 1090 Vienna, Austria
| | - S Mariazzi
- INFN Padova, via Marzolo 8, 35131 Padova, Italy
| | - J Marton
- Stefan Meyer Institute for Subatomic Physics, Austrian Academy of Sciences, Boltzmanngasse 3, 1090 Vienna, Austria
| | - V Matveev
- Institute for Nuclear Research of the Russian Academy of Science, Moscow 117312, Russia
- Joint Institute for Nuclear Research, 141980 Dubna, Russia
| | - Z Mazzotta
- INFN Milano, via Celoria 16, 20133 Milano, Italy
- Department of Physics, University of Milano, via Celoria 16, 20133 Milano, Italy
| | - S R Müller
- Kirchhoff-Institute for Physics, Heidelberg University, Im Neuenheimer Feld 227, 69120 Heidelberg, Germany
| | - G Nebbia
- INFN Padova, via Marzolo 8, 35131 Padova, Italy
| | - P Nedelec
- Institute of Nuclear Physics, CNRS/IN2p3, University of Lyon 1, 69622 Villeurbanne, France
| | - M Oberthaler
- Kirchhoff-Institute for Physics, Heidelberg University, Im Neuenheimer Feld 227, 69120 Heidelberg, Germany
| | - N Pacifico
- Physics Department, CERN, 1211 Geneva 23, Switzerland
| | - D Pagano
- Department of Mechanical and Industrial Engineering, University of Brescia, via Branze 38, 25123 Brescia, Italy
- INFN Pavia, via Bassi 6, 27100 Pavia, Italy
| | - L Penasa
- Department of Physics, University of Trento, via Sommarive 14, 38123 Povo, Trento, Italy
- TIFPA/INFN Trento, via Sommarive 14, 38123 Povo, Trento, Italy
| | - V Petracek
- Czech Technical University in Prague, Brehová 7, 11519 Prague 1, Czech Republic
| | - F Prelz
- INFN Milano, via Celoria 16, 20133 Milano, Italy
| | - M Prevedelli
- University of Bologna, Viale Berti Pichat 6/2, 40126 Bologna, Italy
| | - B Rienaecker
- Physics Department, CERN, 1211 Geneva 23, Switzerland
| | - J Robert
- Laboratoire Aimé Cotton, Université Paris-Sud, ENS Cachan, CNRS, Université Paris-Saclay, 91405 Orsay Cedex, France
| | - O M Røhne
- Department of Physics, University of Oslo, Sem Slandsvei 24, 0371 Oslo, Norway
| | - A Rotondi
- INFN Pavia, via Bassi 6, 27100 Pavia, Italy
- Department of Physics, University of Pavia, via Bassi 6, 27100 Pavia, Italy
| | - H Sandaker
- Department of Physics, University of Oslo, Sem Slandsvei 24, 0371 Oslo, Norway
| | - R Santoro
- INFN Milano, via Celoria 16, 20133 Milano, Italy
- Department of Science, University of Insubria, via Valleggio 11, 22100 Como, Italy
| | - L Smestad
- Physics Department, CERN, 1211 Geneva 23, Switzerland
- The Research Council of Norway, PO Box 564, 1327 Lysaker, Norway
| | - F Sorrentino
- INFN Genova, via Dodecaneso 33, 16146 Genova, Italy
| | - G Testera
- INFN Genova, via Dodecaneso 33, 16146 Genova, Italy
| | - I C Tietje
- Physics Department, CERN, 1211 Geneva 23, Switzerland
| | - E Widmann
- Stefan Meyer Institute for Subatomic Physics, Austrian Academy of Sciences, Boltzmanngasse 3, 1090 Vienna, Austria
| | - P Yzombard
- Max Planck Institute for Nuclear Physics, Saupfercheckweg 1, 69117 Heidelberg, Germany
| | - C Zimmer
- Physics Department, CERN, 1211 Geneva 23, Switzerland
- Max Planck Institute for Nuclear Physics, Saupfercheckweg 1, 69117 Heidelberg, Germany
- Department of Physics, Heidelberg University, Im Neuenheimer Feld 226, 69120 Heidelberg, Germany
| | - J Zmeskal
- Stefan Meyer Institute for Subatomic Physics, Austrian Academy of Sciences, Boltzmanngasse 3, 1090 Vienna, Austria
| | - N Zurlo
- INFN Pavia, via Bassi 6, 27100 Pavia, Italy
- Department of Civil Engineering, University of Brescia, via Branze 43, 25123 Brescia, Italy
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Kadyrov AS, Bray I, Charlton M, Fabrikant II. Quantum suppression of antihydrogen formation in positronium-antiproton scattering. Nat Commun 2017; 8:1544. [PMID: 29146898 PMCID: PMC5691179 DOI: 10.1038/s41467-017-01721-y] [Citation(s) in RCA: 18] [Impact Index Per Article: 2.6] [Reference Citation Analysis] [Abstract] [Track Full Text] [Download PDF] [Figures] [Journal Information] [Subscribe] [Scholar Register] [Received: 02/16/2017] [Accepted: 10/10/2017] [Indexed: 11/08/2022] Open
Abstract
The interaction of antiprotons with low-energy positronium atoms is a fundamental three-body problem whose significance is its utility for formation of antihydrogen. Particular importance resides in understanding processes involving excited positronium states. Until recently such studies were performed using classical techniques. However, they become inapplicable in the low-energy domain. Here we report the results of comprehensive quantum calculations, which include initial excited positronium states with principal quantum numbers up to n i = 5. Contrary to expectation from earlier work, there are only muted increases in the cross-sections for antihydrogen formation for n i > 3. We interpret this in terms of quantum suppression of the reaction at higher angular momenta. Furthermore, the cross-sections for elastic scattering are around two orders of magnitude higher, which we attribute to the degeneracy of the positronium states. We outline some experimental consequences of our results.
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Affiliation(s)
- A S Kadyrov
- Curtin Institute for Computation and Department of Physics, Astronomy and Medical Radiation Science, Curtin University, GPO Box U1987, Perth, WA, 6845, Australia.
| | - I Bray
- Curtin Institute for Computation and Department of Physics, Astronomy and Medical Radiation Science, Curtin University, GPO Box U1987, Perth, WA, 6845, Australia
| | - M Charlton
- Department of Physics, College of Science, Swansea University, Swansea, SA2 8PP, UK
| | - I I Fabrikant
- Department of Physics and Astronomy, University of Nebraska, Lincoln, NE, 68588-0299, USA
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Jones ACL, Moxom J, Rutbeck-Goldman HJ, Osorno KA, Cecchini GG, Fuentes-Garcia M, Greaves RG, Adams DJ, Tom HWK, Mills AP, Leventhal M. Focusing of a Rydberg Positronium Beam with an Ellipsoidal Electrostatic Mirror. PHYSICAL REVIEW LETTERS 2017; 119:053201. [PMID: 28949762 DOI: 10.1103/physrevlett.119.053201] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.1] [Reference Citation Analysis] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 01/01/2017] [Indexed: 06/07/2023]
Abstract
Slow atoms in Rydberg states can exhibit specular reflection from a cylindrical surface upon which an azimuthally periodic potential is imposed. We have constructed a concave mirror of this type, in the shape of a truncated oblate ellipsoid of revolution, which has a focal length of (1.50±0.01) m measured optically. When placed near the center of a long vacuum pipe, this structure brings a beam of n=32 positronium (Ps) atoms to a focus on a position sensitive detector at a distance of (6.03±0.03) m from the Ps source. The intensity at the focus implies an overall reflection efficiency of ∼30%. The focal spot diameter (32±1) mm full width at half maximum is independent of the atoms' flight times from 20 to 60 μs, thus indicating that the mirror is achromatic to a good approximation. Mirrors based on this principle would be of use in a variety of experiments, allowing for improved collection efficiency and tailored transport or imaging of beams of slow Rydberg atoms and molecules.
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Affiliation(s)
- A C L Jones
- Department of Physics and Astronomy, University of California, Riverside, California 92521, USA
| | - J Moxom
- Department of Physics and Astronomy, University of California, Riverside, California 92521, USA
| | - H J Rutbeck-Goldman
- Department of Physics and Astronomy, University of California, Riverside, California 92521, USA
| | - K A Osorno
- Department of Physics and Astronomy, University of California, Riverside, California 92521, USA
| | - G G Cecchini
- Department of Physics and Astronomy, University of California, Riverside, California 92521, USA
| | - M Fuentes-Garcia
- Department of Physics and Astronomy, University of California, Riverside, California 92521, USA
| | - R G Greaves
- Department of Physics and Astronomy, University of California, Riverside, California 92521, USA
| | - D J Adams
- Department of Physics and Astronomy, University of California, Riverside, California 92521, USA
| | - H W K Tom
- Department of Physics and Astronomy, University of California, Riverside, California 92521, USA
| | - A P Mills
- Department of Physics and Astronomy, University of California, Riverside, California 92521, USA
| | - M Leventhal
- Department of Astronomy University of Maryland, College Park, Maryland 20742, USA
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Jones ACL, Rutbeck-Goldman HJ, Hisakado TH, Piñeiro AM, Tom HWK, Mills AP, Barbiellini B, Kuriplach J. Angle-Resolved Spectroscopy of Positronium Emission from a Cu(110) Surface. PHYSICAL REVIEW LETTERS 2016; 117:216402. [PMID: 27911545 DOI: 10.1103/physrevlett.117.216402] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.1] [Reference Citation Analysis] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 07/11/2016] [Indexed: 06/06/2023]
Abstract
The affinity A_{Ps} of positronium (Ps) atoms for a metal is the negative of the maximum kinetic energy with which Ps is emitted into vacuum when thermalized positrons in a metal encounter the surface. When this quantity is measured by ground state Ps time of flight (TOF), the precision is severely limited by the short triplet state lifetime of 142 ns. By quickly converting the emitted Ps atoms into long-lived Rydberg states, we are able to dramatically increase the TOF to allow precision measurements of A_{Ps}. From our measurements made on a Cu(110) sample at T=128 K, we find A_{Ps}(128 K)=(-2.476±0.010_{stat}±0.013_{syst}) eV, compared with the result A_{Ps}(128 K)=(-2.545±0.010_{num}±0.010_{syst}) eV found using highly accurate generalized gradient approximations for both electrons and positrons within density functional theory. Such precision opens up opportunities in the quest for an improved density functional.
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Affiliation(s)
- A C L Jones
- Department of Physics and Astronomy, University of California Riverside, Riverside, California 92521, USA
| | - H J Rutbeck-Goldman
- Department of Physics and Astronomy, University of California Riverside, Riverside, California 92521, USA
| | - T H Hisakado
- Department of Physics and Astronomy, University of California Riverside, Riverside, California 92521, USA
| | - A M Piñeiro
- Department of Physics and Astronomy, University of California Riverside, Riverside, California 92521, USA
| | - H W K Tom
- Department of Physics and Astronomy, University of California Riverside, Riverside, California 92521, USA
| | - A P Mills
- Department of Physics and Astronomy, University of California Riverside, Riverside, California 92521, USA
| | - B Barbiellini
- Department of Physics, Northeastern University, Boston, Massachusetts 02115, USA
| | - J Kuriplach
- Department of Low Temperature Physics, Faculty of Mathematics and Physics, Charles University, V Holešovičkách 2, CZ-180 00 Prague, Czech Republic
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8
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Jones ACL, Piñeiro AM, Roeder EE, Rutbeck-Goldman HJ, Tom HWK, Mills AP. Large-area field-ionization detector for the study of Rydberg atoms. THE REVIEW OF SCIENTIFIC INSTRUMENTS 2016; 87:113307. [PMID: 27910370 DOI: 10.1063/1.4967305] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 06/06/2023]
Abstract
We describe here the development and characterization of a micro-channel plate (MCP) based detector designed for the efficient collection and detection of Rydberg positronium (Ps) atoms for use in a time-of-flight apparatus. The designed detector collects Rydberg atoms over a large area (∼4 times greater than the active area of the MCP), ionizing incident atoms and then collecting and focusing the freed positrons onto the MCP. Here we discuss the function, design, and optimization of the device. The detector has an efficiency for Rydberg Ps that is two times larger than that of the γ-ray scintillation detector based scheme it has been designed to replace, with half the background signal. In principle, detectors of the type described here could be readily employed for the detection of any Rydberg atom species, provided a sufficient field can be applied to achieve an ionization rate of ≥108/s. In such cases, the best time resolution would be achieved by collecting ionized electrons rather than the positive ions.
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Affiliation(s)
- A C L Jones
- Department of Physics and Astronomy, University of California, Riverside, California 92521, USA
| | - A M Piñeiro
- Department of Physics and Astronomy, University of California, Riverside, California 92521, USA
| | - E E Roeder
- Department of Physics and Astronomy, University of California, Riverside, California 92521, USA
| | - H J Rutbeck-Goldman
- Department of Physics and Astronomy, University of California, Riverside, California 92521, USA
| | - H W K Tom
- Department of Physics and Astronomy, University of California, Riverside, California 92521, USA
| | - A P Mills
- Department of Physics and Astronomy, University of California, Riverside, California 92521, USA
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9
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Deller A, Alonso AM, Cooper BS, Hogan SD, Cassidy DB. Electrostatically Guided Rydberg Positronium. PHYSICAL REVIEW LETTERS 2016; 117:073202. [PMID: 27563960 DOI: 10.1103/physrevlett.117.073202] [Citation(s) in RCA: 3] [Impact Index Per Article: 0.4] [Reference Citation Analysis] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 06/10/2016] [Indexed: 06/06/2023]
Abstract
We report experiments in which positronium (Ps) atoms were guided using inhomogeneous electric fields. Ps atoms in Rydberg-Stark states with principal quantum number n=10 and electric dipole moments up to 610 D were prepared via two-color two-photon optical excitation in the presence of a 670 V cm^{-1} electric field. The Ps atoms were created at the entrance of a 0.4 m long electrostatic quadrupole guide, and were detected at the end of the guide via annihilation gamma radiation. When the lasers were tuned to excite low-field-seeking Stark states, a fivefold increase in the number of atoms reaching the end of the guide was observed, whereas no signal was detected when high-field-seeking states were produced. The data are consistent with the calculated geometrical guide acceptance.
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Affiliation(s)
- A Deller
- Department of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT, United Kingdom
| | - A M Alonso
- Department of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT, United Kingdom
| | - B S Cooper
- Department of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT, United Kingdom
| | - S D Hogan
- Department of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT, United Kingdom
| | - D B Cassidy
- Department of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT, United Kingdom
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10
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Hogan SD. Rydberg-Stark deceleration of atoms and molecules. EPJ TECHNIQUES AND INSTRUMENTATION 2016; 3:2. [PMID: 32355605 PMCID: PMC7175735 DOI: 10.1140/epjti/s40485-015-0028-4] [Citation(s) in RCA: 11] [Impact Index Per Article: 1.4] [Reference Citation Analysis] [Abstract] [Key Words] [Grants] [Track Full Text] [Subscribe] [Scholar Register] [Received: 10/27/2015] [Accepted: 12/27/2015] [Indexed: 06/06/2023]
Abstract
The large electric dipole moments associated with highly excited Rydberg states of atoms and molecules make gas-phase samples in these states very well suited to deceleration and trapping using inhomogeneous electric fields. The methods of Rydberg-Stark deceleration with which this can be achieved are reviewed here. Using these techniques, the longitudinal motion of beams of atoms and molecules moving at speeds as high as 2500 m/s have been manipulated, with changes in kinetic energy of up to |Δ E kin|=1.3×10-20 J (|Δ E kin|/e=80 meV or |Δ E kin|/h c=650 cm -1) achieved, while decelerated and trapped samples with number densities of 106- 107 cm -3 and translational temperatures of ∼150 mK have been prepared. Applications of these samples in areas of research at the interface between physics and physical chemistry are discussed.
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Affiliation(s)
- Stephen D. Hogan
- Department of Physics and Astronomy, University College London, Gower Street, London, WC1E 6BT UK
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11
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Kellerbauer A, Aghion S, Amsler C, Ariga A, Ariga T, Bonomi G, Bräunig P, Bremer J, Brusa RS, Cabaret L, Caccia M, Caravita R, Castelli F, Cerchiari G, Chlouba K, Cialdi S, Comparat D, Consolati G, Demetrio A, Di Noto L, Doser M, Dudarev A, Ereditato A, Evans C, Ferragut R, Fesel J, Fontana A, Gerber S, Giammarchi M, Gligorova A, Guatieri F, Haider S, Holmestad H, Huse T, Jordan E, Kimura M, Koettig T, Krasnický D, Lagomarsino V, Lansonneur P, Lebrun P, Lehner S, Liberadzka J, Malbrunot C, Mariazzi S, Matveev V, Mazzotta Z, Nebbia G, Nédélec P, Oberthaler M, Pacifico N, Pagano D, Penasa L, Petráček V, Pistillo C, Prelz F, Prevedelli M, Ravelli L, Rienäcker B, Røhne O, Rotondi A, Sacerdoti M, Sandaker H, Santoro R, Scampoli P, Smestad L, Sorrentino F, Špaček M, Storey J, Strojek I, Testera G, Tietje I, Widmann E, Yzombard P, Zavatarelli S, Zmeskal J, Zurlo N. Probing antimatter gravity – The AEGIS experiment at CERN. EPJ WEB OF CONFERENCES 2016. [DOI: 10.1051/epjconf/201612602016] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.1] [Reference Citation Analysis] [Track Full Text] [Journal Information] [Subscribe] [Scholar Register] [Indexed: 11/14/2022] Open
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12
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Alonso AM, Cooper BS, Deller A, Hogan SD, Cassidy DB. Controlling Positronium Annihilation with Electric Fields. PHYSICAL REVIEW LETTERS 2015; 115:183401. [PMID: 26565466 DOI: 10.1103/physrevlett.115.183401] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.1] [Reference Citation Analysis] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 09/02/2015] [Indexed: 06/05/2023]
Abstract
We show that the annihilation dynamics of excited positronium (Ps) atoms can be controlled using parallel electric and magnetic fields. To achieve this, Ps atoms were optically excited to n=2 sublevels in fields that were adjusted to control the amount of short-lived and long-lived character of the resulting mixed states. Inclusion of the former offers a practical approach to detection via annihilation radiation, whereas the increased lifetimes due to the latter can be exploited to optimize resonance-enhanced two-photon excitation processes (e.g., 1^{3}S→2^{3}P→nS/nD), either by minimizing losses through intermediate state decay, or by making it possible to separate the excitation laser pulses in time. In addition, photoexcitation of mixed states with a 2^{3}S_{1} component represents an efficient route to producing long-lived pure 2^{3}S_{1} atoms via single-photon excitation.
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Affiliation(s)
- A M Alonso
- Department of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT, United Kingdom
| | - B S Cooper
- Department of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT, United Kingdom
| | - A Deller
- Department of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT, United Kingdom
| | - S D Hogan
- Department of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT, United Kingdom
| | - D B Cassidy
- Department of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT, United Kingdom
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13
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Kadyrov AS, Rawlins CM, Stelbovics AT, Bray I, Charlton M. Antihydrogen Formation via Antiproton Scattering with Excited Positronium. PHYSICAL REVIEW LETTERS 2015; 114:183201. [PMID: 26000999 DOI: 10.1103/physrevlett.114.183201] [Citation(s) in RCA: 1] [Impact Index Per Article: 0.1] [Reference Citation Analysis] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 11/20/2014] [Indexed: 06/04/2023]
Abstract
Utilizing the two-center convergent close-coupling method, we find a several order of magnitude enhancement in the formation of antihydrogen via antiproton scattering with positronium in an excited state over the ground state. The effect is greatest at the lowest energies considered, which encompass those achievable in experiment. This suggests a practical approach to creating neutral antimatter for testing its interaction with gravity and for spectroscopic measurements.
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Affiliation(s)
- A S Kadyrov
- Curtin Institute for Computation and Department of Physics, Astronomy and Medical Radiation Sciences, Curtin University, Perth, Western Australia 6102, Australia
| | - C M Rawlins
- Curtin Institute for Computation and Department of Physics, Astronomy and Medical Radiation Sciences, Curtin University, Perth, Western Australia 6102, Australia
| | - A T Stelbovics
- Curtin Institute for Computation and Department of Physics, Astronomy and Medical Radiation Sciences, Curtin University, Perth, Western Australia 6102, Australia
| | - I Bray
- Curtin Institute for Computation and Department of Physics, Astronomy and Medical Radiation Sciences, Curtin University, Perth, Western Australia 6102, Australia
| | - M Charlton
- Department of Physics, College of Science, Swansea University, SA28PP, United Kingdom
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14
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Wall TE, Alonso AM, Cooper BS, Deller A, Hogan SD, Cassidy DB. Selective production of Rydberg-stark states of positronium. PHYSICAL REVIEW LETTERS 2015; 114:173001. [PMID: 25978227 DOI: 10.1103/physrevlett.114.173001] [Citation(s) in RCA: 2] [Impact Index Per Article: 0.2] [Reference Citation Analysis] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 02/04/2015] [Indexed: 06/04/2023]
Abstract
Rydberg positronium (Ps) atoms have been prepared in selected Stark states via two-step (1s→2p→nd/ns) optical excitation. Two methods have been used to achieve Stark-state selection: a field ionization filter that transmits the outermost states with positive Stark shifts, and state-selected photoexcitation in a strong electric field. The former is demonstrated for n=17 and 18 while the latter is performed for n=11 in a homogeneous electric field of 1.9 kV/cm. The observed spectral intensities and their dependence on the polarization of the laser radiation are in agreement with calculations that include the perturbations of the intermediate n=2 manifold. Our results pave the way for the generation of Rydberg Ps atoms with large electric dipole moments that are required for the realization of schemes to control their motion using inhomogeneous electric fields, an essential feature of some proposed Ps free-fall measurements requiring focused beams of long-lived atoms.
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Affiliation(s)
- T E Wall
- Department of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT, United Kingdom
| | - A M Alonso
- Department of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT, United Kingdom
| | - B S Cooper
- Department of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT, United Kingdom
| | - A Deller
- Department of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT, United Kingdom
| | - S D Hogan
- Department of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT, United Kingdom
| | - D B Cassidy
- Department of Physics and Astronomy, University College London, Gower Street, London WC1E 6BT, United Kingdom
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15
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Jones ACL, Goldman HJ, Zhai Q, Feng P, Tom HWK, Mills AP. Monoenergetic positronium emission from metal-organic framework crystals. PHYSICAL REVIEW LETTERS 2015; 114:153201. [PMID: 25933312 DOI: 10.1103/physrevlett.114.153201] [Citation(s) in RCA: 2] [Impact Index Per Article: 0.2] [Reference Citation Analysis] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 01/26/2015] [Indexed: 06/04/2023]
Abstract
Recently it has been discovered that positronium (Ps), after forming in metal-organic framework (MOF) crystals, is emitted into vacuum with a high efficiency and low energy that can only be explained by its propagating as delocalized Bloch states. We show that the Ps atoms are emitted from MOFs in a series of narrow energy peaks consistent with Ps at Bloch-state energy minima being emitted adiabatically into the vacuum. This implies that the Ps emission energy spectra can be directly compared with calculations to obtain detailed information about the Ps band structure in the MOF crystal. The narrow energy width of the lowest energy Ps peak from one MOF sample (2-Methylimidazole zinc salt ZIF-8) suggests it originates from a polaronic Ps surface state. Other peaks can be assigned to Ps with an effective mass of about twice that of bare Ps. Given the immense catalog of available MOF crystals, it should be possible to tune the Ps properties to make vastly improved sources with high production efficiency and a narrow energy spread, for use in fundamental physics experiments.
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Affiliation(s)
- A C L Jones
- Department of Physics and Astronomy, University of California, Riverside, California 92521, USA
| | - H J Goldman
- Department of Physics and Astronomy, University of California, Riverside, California 92521, USA
| | - Q Zhai
- Materials Science and Engineering Program and Department of Chemistry, University of California, Riverside, California 92521, USA
| | - P Feng
- Materials Science and Engineering Program and Department of Chemistry, University of California, Riverside, California 92521, USA
| | - H W K Tom
- Department of Physics and Astronomy, University of California, Riverside, California 92521, USA
| | - A P Mills
- Department of Physics and Astronomy, University of California, Riverside, California 92521, USA
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16
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Abstract
The creation of cold antihydrogen atoms by the controlled combination of positrons and antiprotons has opened up a new window on fundamental physics. More recently, techniques have been developed that allow some antihydrogen atoms to be created at low enough kinetic energies that they can be held inside magnetic minimum neutral atom traps. With confinement times of many minutes possible, it has become feasible to perform experiments to probe the properties of the antiatom for the first time. We review the experimental progress in this area, outline some of the motivation for studying basic aspects of antimatter physics and provide an outlook of where we might expect this field to go in the coming years.
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17
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Vogelsang J, Diepold M, Antognini A, Dax A, Götzfried J, Hänsch TW, Kottmann F, Krauth JJ, Liu YW, Nebel T, Nez F, Schuhmann K, Taqqu D, Pohl R. Multipass laser cavity for efficient transverse illumination of an elongated volume. OPTICS EXPRESS 2014; 22:13050-13062. [PMID: 24921502 DOI: 10.1364/oe.22.013050] [Citation(s) in RCA: 3] [Impact Index Per Article: 0.3] [Reference Citation Analysis] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Indexed: 06/03/2023]
Abstract
A multipass laser cavity is presented which can be used to illuminate an elongated volume from a transverse direction. The illuminated volume can also have a very large transverse cross section. Convenient access to the illuminated volume is granted. The multipass cavity is very robust against misalignment, and no active stabilization is needed. The scheme is suitable for example in beam experiments, where the beam path must not be blocked by a laser mirror, or if the illuminated volume must be very large. This cavity was used for the muonic-hydrogen experiment in which 6 μm laser light illuminated a volume of 7 × 25 × 176 mm3, using mirrors that are only 12 mm in height. We present our measurement of the intensity distribution inside the multipass cavity and show that this is in good agreement with our simulation.
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18
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19
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Cassidy DB, Hisakado TH, Tom HWK, Mills AP. Positronium hyperfine interval measured via saturated absorption spectroscopy. PHYSICAL REVIEW LETTERS 2012; 109:073401. [PMID: 23006369 DOI: 10.1103/physrevlett.109.073401] [Citation(s) in RCA: 4] [Impact Index Per Article: 0.3] [Reference Citation Analysis] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 05/10/2012] [Indexed: 06/01/2023]
Abstract
We report Doppler-free measurements of the positronium (Ps) Lyman-α transition using saturated absorption spectroscopy. In addition to a Lamb dip at wavelength λ(L) = 243.0218 ± 0.0005 nm, we also observed a crossover resonance at λ(C) = 243.0035 ± 0.0005 nm, arising from the excitation of 1(3)S(1) atoms to Zeeman mixed 2P states, followed by stimulated emission to the 1(1)S(0) ground state. Since (λ(L)-λ(C)) is related to the Ps hyperfine interval E(hfs), this observation constitutes the first optical measurement of this quantity and yields E(hfs) = 198.4 ± 4.2 GHz. We describe improvements to the methodology that could lead to the ∼ppm level of precision required to address the long-standing discrepancy between QED calculations and precision experiments using microwave radiation to induce transitions between Zeeman shifted triplet Ps states.
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Affiliation(s)
- D B Cassidy
- Department of Physics and Astronomy, University of California, Riverside, 92521-0413, USA
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20
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Cui N, Macovei M, Hatsagortsyan KZ, Keitel CH. Manipulating the annihilation dynamics of positronium via collective radiation. PHYSICAL REVIEW LETTERS 2012; 108:243401. [PMID: 23004269 DOI: 10.1103/physrevlett.108.243401] [Citation(s) in RCA: 0] [Impact Index Per Article: 0] [Reference Citation Analysis] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 10/14/2011] [Indexed: 06/01/2023]
Abstract
A method is investigated to manipulate the annihilation dynamics of a dense gas of positronium atoms employing superradiance and subradiance regimes of the cooperative spontaneous emission of the system. The corresponding annihilation dynamics is explored in two setups with regard to its fundamental novel properties and controlled by the gas density and by the intensity of a driving strong resonant laser field. In particular, the method allows us to increase the annihilation lifetime of an ensemble of positronium atoms by trapping the atoms in the excited state via collective radiative effects in the resonant laser field. In the second setup, the effect is enhanced by employing a cavity field. The maximum lifetime increase is by a factor of about 200 for para-positronium and by a factor of about 100 for ortho-positronium.
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Affiliation(s)
- Ni Cui
- Max-Planck-Institut für Kernphysik, Saupfercheckweg 1, D-69117 Heidelberg, Germany.
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21
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Cassidy DB, Hisakado TH, Tom HWK, Mills AP. Optical spectroscopy of molecular positronium. PHYSICAL REVIEW LETTERS 2012; 108:133402. [PMID: 22540698 DOI: 10.1103/physrevlett.108.133402] [Citation(s) in RCA: 7] [Impact Index Per Article: 0.6] [Reference Citation Analysis] [Abstract] [Track Full Text] [Subscribe] [Scholar Register] [Received: 01/11/2012] [Indexed: 05/31/2023]
Abstract
We report optical spectroscopic measurements of molecular positronium (Ps(2)), performed via a previously unobserved L=1 excited state. Ps(2) molecules created in a porous silica film, and also in vacuum from an Al(111) crystal, were resonantly excited and then photoionized by pulsed lasers, providing conclusive evidence for the production of this molecular matter-antimatter system and its excited state. Future experiments making use of the photoionized vacuum L=1 Ps(2) could provide a source of Ps(+) ions, as well as other multipositronic systems, such as Ps(2)H(-) or Ps(2)O.
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Affiliation(s)
- D B Cassidy
- Department of Physics and Astronomy, University of California, Riverside, California 92521-0413, USA
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