Modelling the behavior of the positron plasma temperature in antihydrogen experimentation
Abstract Antihydrogen is now routinely produced at CERN by overlapping clouds of positrons and antiprotons. The mechanisms responsible for antihydrogen formation (radiative capture and the three-body reaction) are both dependent on the temperature of the positrons (Te), though with a different weigh...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Lodi-Rizzini, E. [verfasserIn] |
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| Format: |
Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2014 |
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| Schlagwörter: |
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| Anmerkung: |
© Springer International Publishing Switzerland 2014 |
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| Übergeordnetes Werk: |
Enthalten in: Hyperfine interactions - Springer International Publishing, 1975, 228(2014), 1-3 vom: 06. Aug., Seite 53-60 |
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| Übergeordnetes Werk: |
volume:228 ; year:2014 ; number:1-3 ; day:06 ; month:08 ; pages:53-60 |
| Links: |
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| DOI / URN: |
10.1007/s10751-014-1071-2 |
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OLC2076424741 |
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| 520 | |a Abstract Antihydrogen is now routinely produced at CERN by overlapping clouds of positrons and antiprotons. The mechanisms responsible for antihydrogen formation (radiative capture and the three-body reaction) are both dependent on the temperature of the positrons (Te), though with a different weight. Here we present a simple model of the behavior of the positron temperature based on the main processes involved during antihydrogen synthesis, namely: antiproton–positron collisions, positron heating due to plasma expansion and cooling via the emission of synchrotron radiation. The time evolution of Te has been simulated by changing the relevant parameters of the mechanisms involved in order to highlight the importance of the different (competing) effects. | ||
| 650 | 4 | |a Antiproton | |
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| 650 | 4 | |a Antihydrogen | |
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| 700 | 1 | |a Zurlo, N. |4 aut | |
| 700 | 1 | |a Charlton, M. |4 aut | |
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10.1007/s10751-014-1071-2 doi (DE-627)OLC2076424741 (DE-He213)s10751-014-1071-2-p DE-627 ger DE-627 rakwb eng 530 VZ 33.00 bkl Lodi-Rizzini, E. verfasserin aut Modelling the behavior of the positron plasma temperature in antihydrogen experimentation 2014 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer International Publishing Switzerland 2014 Abstract Antihydrogen is now routinely produced at CERN by overlapping clouds of positrons and antiprotons. The mechanisms responsible for antihydrogen formation (radiative capture and the three-body reaction) are both dependent on the temperature of the positrons (Te), though with a different weight. Here we present a simple model of the behavior of the positron temperature based on the main processes involved during antihydrogen synthesis, namely: antiproton–positron collisions, positron heating due to plasma expansion and cooling via the emission of synchrotron radiation. The time evolution of Te has been simulated by changing the relevant parameters of the mechanisms involved in order to highlight the importance of the different (competing) effects. Antiproton Positron Antihydrogen Antimatter Temperature Mascagna, V. aut Venturelli, L. aut Zurlo, N. aut Charlton, M. aut Enthalten in Hyperfine interactions Springer International Publishing, 1975 228(2014), 1-3 vom: 06. Aug., Seite 53-60 (DE-627)129438685 (DE-600)194471-X (DE-576)014809028 0304-3843 nnns volume:228 year:2014 number:1-3 day:06 month:08 pages:53-60 https://doi.org/10.1007/s10751-014-1071-2 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_70 GBV_ILN_2279 33.00 VZ AR 228 2014 1-3 06 08 53-60 |
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10.1007/s10751-014-1071-2 doi (DE-627)OLC2076424741 (DE-He213)s10751-014-1071-2-p DE-627 ger DE-627 rakwb eng 530 VZ 33.00 bkl Lodi-Rizzini, E. verfasserin aut Modelling the behavior of the positron plasma temperature in antihydrogen experimentation 2014 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer International Publishing Switzerland 2014 Abstract Antihydrogen is now routinely produced at CERN by overlapping clouds of positrons and antiprotons. The mechanisms responsible for antihydrogen formation (radiative capture and the three-body reaction) are both dependent on the temperature of the positrons (Te), though with a different weight. Here we present a simple model of the behavior of the positron temperature based on the main processes involved during antihydrogen synthesis, namely: antiproton–positron collisions, positron heating due to plasma expansion and cooling via the emission of synchrotron radiation. The time evolution of Te has been simulated by changing the relevant parameters of the mechanisms involved in order to highlight the importance of the different (competing) effects. Antiproton Positron Antihydrogen Antimatter Temperature Mascagna, V. aut Venturelli, L. aut Zurlo, N. aut Charlton, M. aut Enthalten in Hyperfine interactions Springer International Publishing, 1975 228(2014), 1-3 vom: 06. Aug., Seite 53-60 (DE-627)129438685 (DE-600)194471-X (DE-576)014809028 0304-3843 nnns volume:228 year:2014 number:1-3 day:06 month:08 pages:53-60 https://doi.org/10.1007/s10751-014-1071-2 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_70 GBV_ILN_2279 33.00 VZ AR 228 2014 1-3 06 08 53-60 |
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10.1007/s10751-014-1071-2 doi (DE-627)OLC2076424741 (DE-He213)s10751-014-1071-2-p DE-627 ger DE-627 rakwb eng 530 VZ 33.00 bkl Lodi-Rizzini, E. verfasserin aut Modelling the behavior of the positron plasma temperature in antihydrogen experimentation 2014 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer International Publishing Switzerland 2014 Abstract Antihydrogen is now routinely produced at CERN by overlapping clouds of positrons and antiprotons. The mechanisms responsible for antihydrogen formation (radiative capture and the three-body reaction) are both dependent on the temperature of the positrons (Te), though with a different weight. Here we present a simple model of the behavior of the positron temperature based on the main processes involved during antihydrogen synthesis, namely: antiproton–positron collisions, positron heating due to plasma expansion and cooling via the emission of synchrotron radiation. The time evolution of Te has been simulated by changing the relevant parameters of the mechanisms involved in order to highlight the importance of the different (competing) effects. Antiproton Positron Antihydrogen Antimatter Temperature Mascagna, V. aut Venturelli, L. aut Zurlo, N. aut Charlton, M. aut Enthalten in Hyperfine interactions Springer International Publishing, 1975 228(2014), 1-3 vom: 06. Aug., Seite 53-60 (DE-627)129438685 (DE-600)194471-X (DE-576)014809028 0304-3843 nnns volume:228 year:2014 number:1-3 day:06 month:08 pages:53-60 https://doi.org/10.1007/s10751-014-1071-2 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_70 GBV_ILN_2279 33.00 VZ AR 228 2014 1-3 06 08 53-60 |
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10.1007/s10751-014-1071-2 doi (DE-627)OLC2076424741 (DE-He213)s10751-014-1071-2-p DE-627 ger DE-627 rakwb eng 530 VZ 33.00 bkl Lodi-Rizzini, E. verfasserin aut Modelling the behavior of the positron plasma temperature in antihydrogen experimentation 2014 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer International Publishing Switzerland 2014 Abstract Antihydrogen is now routinely produced at CERN by overlapping clouds of positrons and antiprotons. The mechanisms responsible for antihydrogen formation (radiative capture and the three-body reaction) are both dependent on the temperature of the positrons (Te), though with a different weight. Here we present a simple model of the behavior of the positron temperature based on the main processes involved during antihydrogen synthesis, namely: antiproton–positron collisions, positron heating due to plasma expansion and cooling via the emission of synchrotron radiation. The time evolution of Te has been simulated by changing the relevant parameters of the mechanisms involved in order to highlight the importance of the different (competing) effects. Antiproton Positron Antihydrogen Antimatter Temperature Mascagna, V. aut Venturelli, L. aut Zurlo, N. aut Charlton, M. aut Enthalten in Hyperfine interactions Springer International Publishing, 1975 228(2014), 1-3 vom: 06. Aug., Seite 53-60 (DE-627)129438685 (DE-600)194471-X (DE-576)014809028 0304-3843 nnns volume:228 year:2014 number:1-3 day:06 month:08 pages:53-60 https://doi.org/10.1007/s10751-014-1071-2 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_70 GBV_ILN_2279 33.00 VZ AR 228 2014 1-3 06 08 53-60 |
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10.1007/s10751-014-1071-2 doi (DE-627)OLC2076424741 (DE-He213)s10751-014-1071-2-p DE-627 ger DE-627 rakwb eng 530 VZ 33.00 bkl Lodi-Rizzini, E. verfasserin aut Modelling the behavior of the positron plasma temperature in antihydrogen experimentation 2014 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Springer International Publishing Switzerland 2014 Abstract Antihydrogen is now routinely produced at CERN by overlapping clouds of positrons and antiprotons. The mechanisms responsible for antihydrogen formation (radiative capture and the three-body reaction) are both dependent on the temperature of the positrons (Te), though with a different weight. Here we present a simple model of the behavior of the positron temperature based on the main processes involved during antihydrogen synthesis, namely: antiproton–positron collisions, positron heating due to plasma expansion and cooling via the emission of synchrotron radiation. The time evolution of Te has been simulated by changing the relevant parameters of the mechanisms involved in order to highlight the importance of the different (competing) effects. Antiproton Positron Antihydrogen Antimatter Temperature Mascagna, V. aut Venturelli, L. aut Zurlo, N. aut Charlton, M. aut Enthalten in Hyperfine interactions Springer International Publishing, 1975 228(2014), 1-3 vom: 06. Aug., Seite 53-60 (DE-627)129438685 (DE-600)194471-X (DE-576)014809028 0304-3843 nnns volume:228 year:2014 number:1-3 day:06 month:08 pages:53-60 https://doi.org/10.1007/s10751-014-1071-2 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY GBV_ILN_70 GBV_ILN_2279 33.00 VZ AR 228 2014 1-3 06 08 53-60 |
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Abstract Antihydrogen is now routinely produced at CERN by overlapping clouds of positrons and antiprotons. The mechanisms responsible for antihydrogen formation (radiative capture and the three-body reaction) are both dependent on the temperature of the positrons (Te), though with a different weight. Here we present a simple model of the behavior of the positron temperature based on the main processes involved during antihydrogen synthesis, namely: antiproton–positron collisions, positron heating due to plasma expansion and cooling via the emission of synchrotron radiation. The time evolution of Te has been simulated by changing the relevant parameters of the mechanisms involved in order to highlight the importance of the different (competing) effects. © Springer International Publishing Switzerland 2014 |
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Abstract Antihydrogen is now routinely produced at CERN by overlapping clouds of positrons and antiprotons. The mechanisms responsible for antihydrogen formation (radiative capture and the three-body reaction) are both dependent on the temperature of the positrons (Te), though with a different weight. Here we present a simple model of the behavior of the positron temperature based on the main processes involved during antihydrogen synthesis, namely: antiproton–positron collisions, positron heating due to plasma expansion and cooling via the emission of synchrotron radiation. The time evolution of Te has been simulated by changing the relevant parameters of the mechanisms involved in order to highlight the importance of the different (competing) effects. © Springer International Publishing Switzerland 2014 |
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Abstract Antihydrogen is now routinely produced at CERN by overlapping clouds of positrons and antiprotons. The mechanisms responsible for antihydrogen formation (radiative capture and the three-body reaction) are both dependent on the temperature of the positrons (Te), though with a different weight. Here we present a simple model of the behavior of the positron temperature based on the main processes involved during antihydrogen synthesis, namely: antiproton–positron collisions, positron heating due to plasma expansion and cooling via the emission of synchrotron radiation. The time evolution of Te has been simulated by changing the relevant parameters of the mechanisms involved in order to highlight the importance of the different (competing) effects. © Springer International Publishing Switzerland 2014 |
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<?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>01000caa a22002652 4500</leader><controlfield tag="001">OLC2076424741</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20230503074033.0</controlfield><controlfield tag="007">tu</controlfield><controlfield tag="008">200820s2014 xx ||||| 00| ||eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1007/s10751-014-1071-2</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)OLC2076424741</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-He213)s10751-014-1071-2-p</subfield></datafield><datafield tag="040" ind1=" " ind2=" "><subfield code="a">DE-627</subfield><subfield code="b">ger</subfield><subfield code="c">DE-627</subfield><subfield code="e">rakwb</subfield></datafield><datafield tag="041" ind1=" " ind2=" "><subfield code="a">eng</subfield></datafield><datafield tag="082" ind1="0" ind2="4"><subfield code="a">530</subfield><subfield code="q">VZ</subfield></datafield><datafield tag="084" ind1=" " ind2=" "><subfield code="a">33.00</subfield><subfield code="2">bkl</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Lodi-Rizzini, E.</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Modelling the behavior of the positron plasma temperature in antihydrogen experimentation</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2014</subfield></datafield><datafield tag="336" ind1=" " ind2=" "><subfield code="a">Text</subfield><subfield code="b">txt</subfield><subfield code="2">rdacontent</subfield></datafield><datafield tag="337" ind1=" " ind2=" "><subfield code="a">ohne Hilfsmittel zu benutzen</subfield><subfield code="b">n</subfield><subfield code="2">rdamedia</subfield></datafield><datafield tag="338" ind1=" " ind2=" "><subfield code="a">Band</subfield><subfield code="b">nc</subfield><subfield code="2">rdacarrier</subfield></datafield><datafield tag="500" ind1=" " ind2=" "><subfield code="a">© Springer International Publishing Switzerland 2014</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">Abstract Antihydrogen is now routinely produced at CERN by overlapping clouds of positrons and antiprotons. The mechanisms responsible for antihydrogen formation (radiative capture and the three-body reaction) are both dependent on the temperature of the positrons (Te), though with a different weight. Here we present a simple model of the behavior of the positron temperature based on the main processes involved during antihydrogen synthesis, namely: antiproton–positron collisions, positron heating due to plasma expansion and cooling via the emission of synchrotron radiation. 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