GSTDTAP  > 气候变化
DOI10.3354/cr01466
Observation of the 1S-2S transition in trapped antihydrogen
Ahmadi, M.1; Alves, B. X. R.2; Baker, C. J. .3; Bertsche, W.4,5; Butler, E.6; Capra, A.7; Carruth, C.8; Cesar, C. L.9; Charlton, M.3; Cohen, S.10; Collister, R.7; Eriksson, S.3; Evans, A.11; Evetts, N.12; Fajans, J.8; Friesen, T.2; Fujiwara, M. C.7; Gill, D. R.7; Gutierrez, A.13; Hangst, J. S.2; Hardy, W. N.12; Hayden, M. E.14; Isaac, C. A.3; Ishida, A.15; Ohnson, M. A. J.4,5; Ones, S. A. J.3; Onsell, S. J.16; Kurchaninov, L.7; Madsen, N.3; Mathers, M.17; Maxwell, D.3; McKenna, J. T. K.7; Menary, S.17; Michan, J. M.7,18; Momose, T.12; Munich, J. J. .14; Nolan, P.1; Olchanski, K.7; Olin, A.7,19; Pusa, P.1; Rasmussen, C. O.2; Robicheaux, F.20; Sacramento, R. L.9; Sameed, M.3; Sarid, E.21; Silveira, D. M.9; Stracka, S.22,23; Stutter, G.2; So, C.11; Tharp, T. D.24; Thompson, J. E.17; Thompson, R. I.11; van der Werf, D. P.3,25; Wurtele, J. S.8
2017-01-26
发表期刊NATURE
ISSN0028-0836
EISSN1476-4687
出版年2017
卷号541期号:7638页码:506-510
文章类型Article
语种英语
国家England; Denmark; Wales; Switzerland; Canada; USA; Brazil; Israel; Japan; Sweden; Italy; France
英文摘要

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 Hansch1 to a precision of a few parts in 10(15). Recent technological advances have allowed us to focus on antihydrogen-the antimatter equivalent of hydrogen(2-4). 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 x 10(-10).


领域地球科学 ; 气候变化 ; 资源环境
收录类别SCI-E
WOS记录号WOS:000396116600045
WOS关键词CHARGE ; SPECTROSCOPY ; LIMIT
WOS类目Multidisciplinary Sciences
WOS研究方向Science & Technology - Other Topics
引用统计
文献类型期刊论文
条目标识符http://119.78.100.173/C666/handle/2XK7JSWQ/15227
专题气候变化
作者单位1.Univ Liverpool, Dept Phys, Liverpool L69 7ZE, Merseyside, England;
2.Aarhus Univ, Dept Phys & Astron, DK-8000 Aarhus C, Denmark;
3.Swansea Univ, Dept Phys, Coll Sci, Swansea SA2 8PP, W Glam, Wales;
4.Univ Manchester, Sch Phys & Astron, Manchester M12 9PL, Lancs, England;
5.Sci Tech Daresbury, Cockcroft Inst, Warrington WA4 4AD, Cheshire, England;
6.CERN, Phys Dept, CH-1211 Geneva 23, Switzerland;
7.TRIUMF, 4004 Wesbrook Mall, Vancouver, BC V6T 2A3, Canada;
8.Univ Calif Berkeley, Dept Phys, Berkeley, CA 94720 USA;
9.Univ Fed Rio de Janeiro, Inst Fis, BR-21941 Rio De Janeiro, Brazil;
10.Ben Gurion Univ Negev, Dept Phys, IL-84105 Beer Sheva, Israel;
11.Univ Calgary, Dept Phys & Astron, Calgary, AB T2N 1N4, Canada;
12.Univ British Columbia, Dept Phys & Astron, Vancouver, BC V6T 1Z1, Canada;
13.UCL, Dept Med Phys & Biomed Engn, London WC1E 6BT, England;
14.Simon Fraser Univ, Dept Phys, Burnaby, BC V5A 1S6, Canada;
15.Univ Tokyo, Dept Phys, Bunkyo Ku, 7-3-1 Hongo, Tokyo 1130033, Japan;
16.Stockholm Univ, Dept Phys, SE-10691 Stockholm, Sweden;
17.York Univ, Dept Phys & Astron, Toronto, ON M3J 1P3, Canada;
18.Ecole Polytech Fed Lausanne, Swiss Plasma Ctr, CH-1015 Lausanne, Switzerland;
19.Univ Victoria, Dept Phys & Astron, Victoria, BC V8P 5C2, Canada;
20.Purdue Univ, Dept Phys & Astron, W Lafayette, IN 47907 USA;
21.Soreq NRC, IL-81800 Yavne, Israel;
22.Univ Pisa, Largo Pontecorvo 3, I-56127 Pisa, Italy;
23.Sez INFN Pisa, Largo Pontecorvo 3, I-56127 Pisa, Italy;
24.Marquette Univ, Dept Phys, POB 1881, Milwaukee, WI 53201 USA;
25.CEA Saclay, IRFU, F-91191 Gif Sur Yvette, France
推荐引用方式
GB/T 7714
Ahmadi, M.,Alves, B. X. R.,Baker, C. J. .,et al. Observation of the 1S-2S transition in trapped antihydrogen[J]. NATURE,2017,541(7638):506-510.
APA Ahmadi, M..,Alves, B. X. R..,Baker, C. J. ..,Bertsche, W..,Butler, E..,...&Wurtele, J. S..(2017).Observation of the 1S-2S transition in trapped antihydrogen.NATURE,541(7638),506-510.
MLA Ahmadi, M.,et al."Observation of the 1S-2S transition in trapped antihydrogen".NATURE 541.7638(2017):506-510.
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