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Observations of cold antihydrogen
ATRAP's e/sup +/ cooling of p in a nested Penning trap has led to reports of cold H produced during such cooling by the ATHENA and ATRAP collaborations. To observe H, ATHENA uses coincident annihilation detection and ATRAP uses field ionization followed by p storage. Advantages of ATRAP's...
Autores principales: | , , , , , , , , , , , , , , |
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Lenguaje: | eng |
Publicado: |
2004
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Materias: | |
Acceso en línea: | https://dx.doi.org/10.1016/S0168-583X(03)01777-4 http://cds.cern.ch/record/818506 |
_version_ | 1780905484128092160 |
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author | Tan, J N Bowden, N S Gabrielse, G Oxley, P Speck, A Storry, C H Wessels, M Grzonka, D Oelert, W Schepers, G Sefzick, T Walz, J Pittner, H Hänsch, T W Hessels, E A |
author_facet | Tan, J N Bowden, N S Gabrielse, G Oxley, P Speck, A Storry, C H Wessels, M Grzonka, D Oelert, W Schepers, G Sefzick, T Walz, J Pittner, H Hänsch, T W Hessels, E A |
author_sort | Tan, J N |
collection | CERN |
description | ATRAP's e/sup +/ cooling of p in a nested Penning trap has led to reports of cold H produced during such cooling by the ATHENA and ATRAP collaborations. To observe H, ATHENA uses coincident annihilation detection and ATRAP uses field ionization followed by p storage. Advantages of ATRAP's field ionization method include the complete absence of any background events, and the first way to measure which H states are produced. ATRAP enhances the H production rate by driving many cycles of e/sup +/ cooling in the nested trap, with more H counted in an hour than the sum of all the other antimatter atoms ever reported. The number of H counted per incident high energy p is also higher than ever observed. The first measured distribution of H states is made using a pre-ionizing electric field between separated production and detection regions. The high rate and the high Rydberg states suggest that the H is formed via three-body recombination, as expected. (22 refs). |
id | cern-818506 |
institution | Organización Europea para la Investigación Nuclear |
language | eng |
publishDate | 2004 |
record_format | invenio |
spelling | cern-8185062019-09-30T06:29:59Zdoi:10.1016/S0168-583X(03)01777-4http://cds.cern.ch/record/818506engTan, J NBowden, N SGabrielse, GOxley, PSpeck, AStorry, C HWessels, MGrzonka, DOelert, WSchepers, GSefzick, TWalz, JPittner, HHänsch, T WHessels, E AObservations of cold antihydrogenOther Fields of PhysicsATRAP's e/sup +/ cooling of p in a nested Penning trap has led to reports of cold H produced during such cooling by the ATHENA and ATRAP collaborations. To observe H, ATHENA uses coincident annihilation detection and ATRAP uses field ionization followed by p storage. Advantages of ATRAP's field ionization method include the complete absence of any background events, and the first way to measure which H states are produced. ATRAP enhances the H production rate by driving many cycles of e/sup +/ cooling in the nested trap, with more H counted in an hour than the sum of all the other antimatter atoms ever reported. The number of H counted per incident high energy p is also higher than ever observed. The first measured distribution of H states is made using a pre-ionizing electric field between separated production and detection regions. The high rate and the high Rydberg states suggest that the H is formed via three-body recombination, as expected. (22 refs).oai:cds.cern.ch:8185062004 |
spellingShingle | Other Fields of Physics Tan, J N Bowden, N S Gabrielse, G Oxley, P Speck, A Storry, C H Wessels, M Grzonka, D Oelert, W Schepers, G Sefzick, T Walz, J Pittner, H Hänsch, T W Hessels, E A Observations of cold antihydrogen |
title | Observations of cold antihydrogen |
title_full | Observations of cold antihydrogen |
title_fullStr | Observations of cold antihydrogen |
title_full_unstemmed | Observations of cold antihydrogen |
title_short | Observations of cold antihydrogen |
title_sort | observations of cold antihydrogen |
topic | Other Fields of Physics |
url | https://dx.doi.org/10.1016/S0168-583X(03)01777-4 http://cds.cern.ch/record/818506 |
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