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An improved limit on the charge of antihydrogen from stochastic acceleration

Antimatter continues to intrigue physicists because of its apparent absence in the observable Universe. Current theory requires that matter and antimatter appeared in equal quantities after the Big Bang, but the Standard Model of particle physics offers no quantitative explanation for the apparent d...

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Detalles Bibliográficos
Autores principales: Ahmadi, M, Baquero-Ruiz, M, Bertsche, W, Butler, E, Capra, A, Carruth, C, Cesar, C L, Charlton, M, Charman, A E, Eriksson, S, Evans, L T, 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, Jones, S A, Jonsell, S, Kurchaninov, L, Madsen, N, Maxwell, D, McKenna, J T K, Menary, S, Michan, J M, Momose, T, Munich, J J, Nolan, P, Olchanski, K, Olin, A, Povilus, A, Pusa, P, Rasmussen, C Ø, Robicheaux, F, Sacramento, R L, Sameed, M, Sarid, E, Silveira, D M, So, C, Tharp, T D, Thompson, R I, van der Werf, D P, Wurtele, J S, Zhmoginov, A I
Lenguaje:eng
Publicado: 2016
Materias:
Acceso en línea:https://dx.doi.org/10.1038/nature16491
http://cds.cern.ch/record/2262866
_version_ 1780954222090518528
author Ahmadi, M
Baquero-Ruiz, M
Bertsche, W
Butler, E
Capra, A
Carruth, C
Cesar, C L
Charlton, M
Charman, A E
Eriksson, S
Evans, L T
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
Jones, S A
Jonsell, S
Kurchaninov, L
Madsen, N
Maxwell, D
McKenna, J T K
Menary, S
Michan, J M
Momose, T
Munich, J J
Nolan, P
Olchanski, K
Olin, A
Povilus, A
Pusa, P
Rasmussen, C Ø
Robicheaux, F
Sacramento, R L
Sameed, M
Sarid, E
Silveira, D M
So, C
Tharp, T D
Thompson, R I
van der Werf, D P
Wurtele, J S
Zhmoginov, A I
author_facet Ahmadi, M
Baquero-Ruiz, M
Bertsche, W
Butler, E
Capra, A
Carruth, C
Cesar, C L
Charlton, M
Charman, A E
Eriksson, S
Evans, L T
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
Jones, S A
Jonsell, S
Kurchaninov, L
Madsen, N
Maxwell, D
McKenna, J T K
Menary, S
Michan, J M
Momose, T
Munich, J J
Nolan, P
Olchanski, K
Olin, A
Povilus, A
Pusa, P
Rasmussen, C Ø
Robicheaux, F
Sacramento, R L
Sameed, M
Sarid, E
Silveira, D M
So, C
Tharp, T D
Thompson, R I
van der Werf, D P
Wurtele, J S
Zhmoginov, A I
author_sort Ahmadi, M
collection CERN
description Antimatter continues to intrigue physicists because of its apparent absence in the observable Universe. Current theory requires that matter and antimatter appeared in equal quantities after the Big Bang, but the Standard Model of particle physics offers no quantitative explanation for the apparent disappearance of half the Universe. It has recently become possible to study trapped atoms of antihydrogen to search for possible, as yet unobserved, differences in the physical behaviour of matter and antimatter. Here we consider the charge neutrality of the antihydrogen atom. By applying stochastic acceleration to trapped antihydrogen atoms, we determine an experimental bound on the antihydrogen charge, Qe, of |Q| < 0.71 parts per billion (one standard deviation), in which e is the elementary charge. This bound is a factor of 20 less than that determined from the best previous measurement of the antihydrogen charge. The electrical charge of atoms and molecules of normal matter is known to be no greater than about 10(-21)e for a diverse range of species including H2, He and SF6. Charge-parity-time symmetry and quantum anomaly cancellation demand that the charge of antihydrogen be similarly small. Thus, our measurement constitutes an improved limit and a test of fundamental aspects of the Standard Model. If we assume charge superposition and use the best measured value of the antiproton charge, then we can place a new limit on the positron charge anomaly (the relative difference between the positron and elementary charge) of about one part per billion (one standard deviation), a 25-fold reduction compared to the current best measurement
id oai-inspirehep.net-1426912
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2016
record_format invenio
spelling oai-inspirehep.net-14269122019-09-30T06:29:59Zdoi:10.1038/nature16491http://cds.cern.ch/record/2262866engAhmadi, MBaquero-Ruiz, MBertsche, WButler, ECapra, ACarruth, CCesar, C LCharlton, MCharman, A EEriksson, SEvans, L TEvetts, NFajans, JFriesen, TFujiwara, M CGill, D RGutierrez, AHangst, J SHardy, W NHayden, M EIsaac, C AIshida, AJones, S AJonsell, SKurchaninov, LMadsen, NMaxwell, DMcKenna, J T KMenary, SMichan, J MMomose, TMunich, J JNolan, POlchanski, KOlin, APovilus, APusa, PRasmussen, C ØRobicheaux, FSacramento, R LSameed, MSarid, ESilveira, D MSo, CTharp, T DThompson, R Ivan der Werf, D PWurtele, J SZhmoginov, A IAn improved limit on the charge of antihydrogen from stochastic accelerationPhysics in GeneralAntimatter continues to intrigue physicists because of its apparent absence in the observable Universe. Current theory requires that matter and antimatter appeared in equal quantities after the Big Bang, but the Standard Model of particle physics offers no quantitative explanation for the apparent disappearance of half the Universe. It has recently become possible to study trapped atoms of antihydrogen to search for possible, as yet unobserved, differences in the physical behaviour of matter and antimatter. Here we consider the charge neutrality of the antihydrogen atom. By applying stochastic acceleration to trapped antihydrogen atoms, we determine an experimental bound on the antihydrogen charge, Qe, of |Q| < 0.71 parts per billion (one standard deviation), in which e is the elementary charge. This bound is a factor of 20 less than that determined from the best previous measurement of the antihydrogen charge. The electrical charge of atoms and molecules of normal matter is known to be no greater than about 10(-21)e for a diverse range of species including H2, He and SF6. Charge-parity-time symmetry and quantum anomaly cancellation demand that the charge of antihydrogen be similarly small. Thus, our measurement constitutes an improved limit and a test of fundamental aspects of the Standard Model. If we assume charge superposition and use the best measured value of the antiproton charge, then we can place a new limit on the positron charge anomaly (the relative difference between the positron and elementary charge) of about one part per billion (one standard deviation), a 25-fold reduction compared to the current best measurementoai:inspirehep.net:14269122016
spellingShingle Physics in General
Ahmadi, M
Baquero-Ruiz, M
Bertsche, W
Butler, E
Capra, A
Carruth, C
Cesar, C L
Charlton, M
Charman, A E
Eriksson, S
Evans, L T
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
Jones, S A
Jonsell, S
Kurchaninov, L
Madsen, N
Maxwell, D
McKenna, J T K
Menary, S
Michan, J M
Momose, T
Munich, J J
Nolan, P
Olchanski, K
Olin, A
Povilus, A
Pusa, P
Rasmussen, C Ø
Robicheaux, F
Sacramento, R L
Sameed, M
Sarid, E
Silveira, D M
So, C
Tharp, T D
Thompson, R I
van der Werf, D P
Wurtele, J S
Zhmoginov, A I
An improved limit on the charge of antihydrogen from stochastic acceleration
title An improved limit on the charge of antihydrogen from stochastic acceleration
title_full An improved limit on the charge of antihydrogen from stochastic acceleration
title_fullStr An improved limit on the charge of antihydrogen from stochastic acceleration
title_full_unstemmed An improved limit on the charge of antihydrogen from stochastic acceleration
title_short An improved limit on the charge of antihydrogen from stochastic acceleration
title_sort improved limit on the charge of antihydrogen from stochastic acceleration
topic Physics in General
url https://dx.doi.org/10.1038/nature16491
http://cds.cern.ch/record/2262866
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