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Further Evidence for Low Energy Protonium Production in Vacuum

We describe an experiment performed in the ATHENA apparatus in which there is evidence that the antiproton-proton bound state, protonium, has been produced at very low energies in vacuum following the interaction of cold antiprotons with a trapped cloud of molecular hydrogen ions. The latter were co...

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Autores principales: Lodi Rizzini, Evandro, Venturelli, Luca, Zurlo, Nicola, Charlton, Michael, Amsler, Claude, Bonomi, Germano, Canali, Carlo, Carraro, Carlo, Fontana, Andrea, Genova, Pablo, Hayano, Ryugo, Jorgensen, Lars Varming, Kellerbauer, Alban, Lagomarsino, Vittorio, Landua, R, Macrì, Mario, Manuzio, Giulio, Montagna, Paolo, Regenfus, Christian, Rotondi, Alberto, Testera, Gemma, Variola, Alessandro, van der Werf, Dirk Peter
Lenguaje:eng
Publicado: 2012
Materias:
Acceso en línea:http://cds.cern.ch/record/1462974
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author Lodi Rizzini, Evandro
Venturelli, Luca
Zurlo, Nicola
Charlton, Michael
Amsler, Claude,
Bonomi, Germano
Canali, Carlo
Carraro, Carlo
Fontana, Andrea
Genova, Pablo
Hayano, Ryugo
Jorgensen, Lars Varming
Kellerbauer, Alban
Lagomarsino, Vittorio
Landua, R
Macrì, Mario
Manuzio, Giulio
Montagna, Paolo
Regenfus, Christian
Rotondi, Alberto
Testera, Gemma
Variola, Alessandro
van der Werf, Dirk Peter
author_facet Lodi Rizzini, Evandro
Venturelli, Luca
Zurlo, Nicola
Charlton, Michael
Amsler, Claude,
Bonomi, Germano
Canali, Carlo
Carraro, Carlo
Fontana, Andrea
Genova, Pablo
Hayano, Ryugo
Jorgensen, Lars Varming
Kellerbauer, Alban
Lagomarsino, Vittorio
Landua, R
Macrì, Mario
Manuzio, Giulio
Montagna, Paolo
Regenfus, Christian
Rotondi, Alberto
Testera, Gemma
Variola, Alessandro
van der Werf, Dirk Peter
author_sort Lodi Rizzini, Evandro
collection CERN
description We describe an experiment performed in the ATHENA apparatus in which there is evidence that the antiproton-proton bound state, protonium, has been produced at very low energies in vacuum following the interaction of cold antiprotons with a trapped cloud of molecular hydrogen ions. The latter were confined in a centrifugally separated belt outside a positron plasma used for antihydrogen formation. Studies have been performed at low positron plasma temperatures in which the protonium annihilation signal has been identified along with that from antihydrogen, and we discuss how their contributions can be disentangled. With the positron plasma heated to around 10,000 K the ions become distributed in the positrons, and the majority of the annihilation signal can be explained in terms of protonium formationion, as antihydrogen creation is heavily suppressed. In this case we compare the observed protonium formation rate with expectations from theory and find reasonable accord, when experimental systematics are taken into account. The effect on the annihilation signals of the passage of an electron current through a pre-loaded positron plasma has been studied in detail, and the results are presented here for the first time.
id cern-1462974
institution Organización Europea para la Investigación Nuclear
language eng
publishDate 2012
record_format invenio
spelling cern-14629742019-09-30T06:29:59Zhttp://cds.cern.ch/record/1462974engLodi Rizzini, EvandroVenturelli, LucaZurlo, NicolaCharlton, MichaelAmsler, Claude,Bonomi, GermanoCanali, CarloCarraro, CarloFontana, AndreaGenova, PabloHayano, RyugoJorgensen, Lars VarmingKellerbauer, AlbanLagomarsino, VittorioLandua, RMacrì, MarioManuzio, GiulioMontagna, PaoloRegenfus, ChristianRotondi, AlbertoTestera, GemmaVariola, Alessandrovan der Werf, Dirk PeterFurther Evidence for Low Energy Protonium Production in VacuumNuclear Physics - ExperimentWe describe an experiment performed in the ATHENA apparatus in which there is evidence that the antiproton-proton bound state, protonium, has been produced at very low energies in vacuum following the interaction of cold antiprotons with a trapped cloud of molecular hydrogen ions. The latter were confined in a centrifugally separated belt outside a positron plasma used for antihydrogen formation. Studies have been performed at low positron plasma temperatures in which the protonium annihilation signal has been identified along with that from antihydrogen, and we discuss how their contributions can be disentangled. With the positron plasma heated to around 10,000 K the ions become distributed in the positrons, and the majority of the annihilation signal can be explained in terms of protonium formationion, as antihydrogen creation is heavily suppressed. In this case we compare the observed protonium formation rate with expectations from theory and find reasonable accord, when experimental systematics are taken into account. The effect on the annihilation signals of the passage of an electron current through a pre-loaded positron plasma has been studied in detail, and the results are presented here for the first time.CERN-PH-EP-2012-215oai:cds.cern.ch:14629742012-09-03
spellingShingle Nuclear Physics - Experiment
Lodi Rizzini, Evandro
Venturelli, Luca
Zurlo, Nicola
Charlton, Michael
Amsler, Claude,
Bonomi, Germano
Canali, Carlo
Carraro, Carlo
Fontana, Andrea
Genova, Pablo
Hayano, Ryugo
Jorgensen, Lars Varming
Kellerbauer, Alban
Lagomarsino, Vittorio
Landua, R
Macrì, Mario
Manuzio, Giulio
Montagna, Paolo
Regenfus, Christian
Rotondi, Alberto
Testera, Gemma
Variola, Alessandro
van der Werf, Dirk Peter
Further Evidence for Low Energy Protonium Production in Vacuum
title Further Evidence for Low Energy Protonium Production in Vacuum
title_full Further Evidence for Low Energy Protonium Production in Vacuum
title_fullStr Further Evidence for Low Energy Protonium Production in Vacuum
title_full_unstemmed Further Evidence for Low Energy Protonium Production in Vacuum
title_short Further Evidence for Low Energy Protonium Production in Vacuum
title_sort further evidence for low energy protonium production in vacuum
topic Nuclear Physics - Experiment
url http://cds.cern.ch/record/1462974
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