Effect of halo on high power laser pulse wake in underdense plasma
Strong disturbance in the wake of the laser pulses propagating in underdense plasma and consequent unstable electron acceleration by the wakefield can be provoked by pulse's halo, which always exists as a result of an imperfect optical focusing. When the power in the halo part exceeds a critica...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
Pathak, Naveen [verfasserIn] |
|---|
| Format: |
Artikel |
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| Sprache: |
Englisch |
| Erschienen: |
2016 |
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| Rechteinformationen: |
Nutzungsrecht: © Author(s) |
|---|
| Übergeordnetes Werk: |
Enthalten in: Physics of plasmas - Melville, NY : AIP, 1994, 23(2016), 11 |
|---|---|
| Übergeordnetes Werk: |
volume:23 ; year:2016 ; number:11 |
| Links: |
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| DOI / URN: |
10.1063/1.4968240 |
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OLC1985755807 |
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| 520 | |a Strong disturbance in the wake of the laser pulses propagating in underdense plasma and consequent unstable electron acceleration by the wakefield can be provoked by pulse's halo, which always exists as a result of an imperfect optical focusing. When the power in the halo part exceeds a critical level for the self-focusing, it evolves in the plasma as an independent mode, which later gets coupled with the propagation of the central Gaussian spot of the pulse resulting in a novel instability. Here, this instability is investigated numerically via fully relativistic 3D particle-in-cell simulations and is shown to be partially suppressed by using plasma channels for pulse guiding. | ||
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10.1063/1.4968240 doi PQ20161201 (DE-627)OLC1985755807 (DE-599)GBVOLC1985755807 (PRQ)scitation_primary_10_1063_1_49682400 (KEY)0178548620160000023001100000effectofhaloonhighpowerlaserpulsewakeinunderdensep DE-627 ger DE-627 rakwb eng 530 DE-600 Pathak, Naveen verfasserin aut Effect of halo on high power laser pulse wake in underdense plasma 2016 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier Strong disturbance in the wake of the laser pulses propagating in underdense plasma and consequent unstable electron acceleration by the wakefield can be provoked by pulse's halo, which always exists as a result of an imperfect optical focusing. When the power in the halo part exceeds a critical level for the self-focusing, it evolves in the plasma as an independent mode, which later gets coupled with the propagation of the central Gaussian spot of the pulse resulting in a novel instability. Here, this instability is investigated numerically via fully relativistic 3D particle-in-cell simulations and is shown to be partially suppressed by using plasma channels for pulse guiding. Nutzungsrecht: © Author(s) Zhidkov, Alexei oth Masuda, Shinichi oth Hosokai, Tomonao oth Kodama, Ryosuke oth Enthalten in Physics of plasmas Melville, NY : AIP, 1994 23(2016), 11 (DE-627)171342119 (DE-600)1179425-2 (DE-576)038876949 1070-664X nnns volume:23 year:2016 number:11 http://dx.doi.org/10.1063/1.4968240 Volltext http://dx.doi.org/10.1063/1.4968240 GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OPC-AST SSG-OPC-GEO SSG-OPC-GGO GBV_ILN_47 GBV_ILN_70 AR 23 2016 11 |
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10.1063/1.4968240 doi PQ20161201 (DE-627)OLC1985755807 (DE-599)GBVOLC1985755807 (PRQ)scitation_primary_10_1063_1_49682400 (KEY)0178548620160000023001100000effectofhaloonhighpowerlaserpulsewakeinunderdensep DE-627 ger DE-627 rakwb eng 530 DE-600 Pathak, Naveen verfasserin aut Effect of halo on high power laser pulse wake in underdense plasma 2016 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier Strong disturbance in the wake of the laser pulses propagating in underdense plasma and consequent unstable electron acceleration by the wakefield can be provoked by pulse's halo, which always exists as a result of an imperfect optical focusing. When the power in the halo part exceeds a critical level for the self-focusing, it evolves in the plasma as an independent mode, which later gets coupled with the propagation of the central Gaussian spot of the pulse resulting in a novel instability. Here, this instability is investigated numerically via fully relativistic 3D particle-in-cell simulations and is shown to be partially suppressed by using plasma channels for pulse guiding. Nutzungsrecht: © Author(s) Zhidkov, Alexei oth Masuda, Shinichi oth Hosokai, Tomonao oth Kodama, Ryosuke oth Enthalten in Physics of plasmas Melville, NY : AIP, 1994 23(2016), 11 (DE-627)171342119 (DE-600)1179425-2 (DE-576)038876949 1070-664X nnns volume:23 year:2016 number:11 http://dx.doi.org/10.1063/1.4968240 Volltext http://dx.doi.org/10.1063/1.4968240 GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OPC-AST SSG-OPC-GEO SSG-OPC-GGO GBV_ILN_47 GBV_ILN_70 AR 23 2016 11 |
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10.1063/1.4968240 doi PQ20161201 (DE-627)OLC1985755807 (DE-599)GBVOLC1985755807 (PRQ)scitation_primary_10_1063_1_49682400 (KEY)0178548620160000023001100000effectofhaloonhighpowerlaserpulsewakeinunderdensep DE-627 ger DE-627 rakwb eng 530 DE-600 Pathak, Naveen verfasserin aut Effect of halo on high power laser pulse wake in underdense plasma 2016 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier Strong disturbance in the wake of the laser pulses propagating in underdense plasma and consequent unstable electron acceleration by the wakefield can be provoked by pulse's halo, which always exists as a result of an imperfect optical focusing. When the power in the halo part exceeds a critical level for the self-focusing, it evolves in the plasma as an independent mode, which later gets coupled with the propagation of the central Gaussian spot of the pulse resulting in a novel instability. Here, this instability is investigated numerically via fully relativistic 3D particle-in-cell simulations and is shown to be partially suppressed by using plasma channels for pulse guiding. Nutzungsrecht: © Author(s) Zhidkov, Alexei oth Masuda, Shinichi oth Hosokai, Tomonao oth Kodama, Ryosuke oth Enthalten in Physics of plasmas Melville, NY : AIP, 1994 23(2016), 11 (DE-627)171342119 (DE-600)1179425-2 (DE-576)038876949 1070-664X nnns volume:23 year:2016 number:11 http://dx.doi.org/10.1063/1.4968240 Volltext http://dx.doi.org/10.1063/1.4968240 GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OPC-AST SSG-OPC-GEO SSG-OPC-GGO GBV_ILN_47 GBV_ILN_70 AR 23 2016 11 |
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10.1063/1.4968240 doi PQ20161201 (DE-627)OLC1985755807 (DE-599)GBVOLC1985755807 (PRQ)scitation_primary_10_1063_1_49682400 (KEY)0178548620160000023001100000effectofhaloonhighpowerlaserpulsewakeinunderdensep DE-627 ger DE-627 rakwb eng 530 DE-600 Pathak, Naveen verfasserin aut Effect of halo on high power laser pulse wake in underdense plasma 2016 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier Strong disturbance in the wake of the laser pulses propagating in underdense plasma and consequent unstable electron acceleration by the wakefield can be provoked by pulse's halo, which always exists as a result of an imperfect optical focusing. When the power in the halo part exceeds a critical level for the self-focusing, it evolves in the plasma as an independent mode, which later gets coupled with the propagation of the central Gaussian spot of the pulse resulting in a novel instability. Here, this instability is investigated numerically via fully relativistic 3D particle-in-cell simulations and is shown to be partially suppressed by using plasma channels for pulse guiding. Nutzungsrecht: © Author(s) Zhidkov, Alexei oth Masuda, Shinichi oth Hosokai, Tomonao oth Kodama, Ryosuke oth Enthalten in Physics of plasmas Melville, NY : AIP, 1994 23(2016), 11 (DE-627)171342119 (DE-600)1179425-2 (DE-576)038876949 1070-664X nnns volume:23 year:2016 number:11 http://dx.doi.org/10.1063/1.4968240 Volltext http://dx.doi.org/10.1063/1.4968240 GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OPC-AST SSG-OPC-GEO SSG-OPC-GGO GBV_ILN_47 GBV_ILN_70 AR 23 2016 11 |
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10.1063/1.4968240 doi PQ20161201 (DE-627)OLC1985755807 (DE-599)GBVOLC1985755807 (PRQ)scitation_primary_10_1063_1_49682400 (KEY)0178548620160000023001100000effectofhaloonhighpowerlaserpulsewakeinunderdensep DE-627 ger DE-627 rakwb eng 530 DE-600 Pathak, Naveen verfasserin aut Effect of halo on high power laser pulse wake in underdense plasma 2016 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier Strong disturbance in the wake of the laser pulses propagating in underdense plasma and consequent unstable electron acceleration by the wakefield can be provoked by pulse's halo, which always exists as a result of an imperfect optical focusing. When the power in the halo part exceeds a critical level for the self-focusing, it evolves in the plasma as an independent mode, which later gets coupled with the propagation of the central Gaussian spot of the pulse resulting in a novel instability. Here, this instability is investigated numerically via fully relativistic 3D particle-in-cell simulations and is shown to be partially suppressed by using plasma channels for pulse guiding. Nutzungsrecht: © Author(s) Zhidkov, Alexei oth Masuda, Shinichi oth Hosokai, Tomonao oth Kodama, Ryosuke oth Enthalten in Physics of plasmas Melville, NY : AIP, 1994 23(2016), 11 (DE-627)171342119 (DE-600)1179425-2 (DE-576)038876949 1070-664X nnns volume:23 year:2016 number:11 http://dx.doi.org/10.1063/1.4968240 Volltext http://dx.doi.org/10.1063/1.4968240 GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-PHY SSG-OPC-AST SSG-OPC-GEO SSG-OPC-GGO GBV_ILN_47 GBV_ILN_70 AR 23 2016 11 |
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Effect of halo on high power laser pulse wake in underdense plasma |
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Strong disturbance in the wake of the laser pulses propagating in underdense plasma and consequent unstable electron acceleration by the wakefield can be provoked by pulse's halo, which always exists as a result of an imperfect optical focusing. When the power in the halo part exceeds a critical level for the self-focusing, it evolves in the plasma as an independent mode, which later gets coupled with the propagation of the central Gaussian spot of the pulse resulting in a novel instability. Here, this instability is investigated numerically via fully relativistic 3D particle-in-cell simulations and is shown to be partially suppressed by using plasma channels for pulse guiding. |
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Strong disturbance in the wake of the laser pulses propagating in underdense plasma and consequent unstable electron acceleration by the wakefield can be provoked by pulse's halo, which always exists as a result of an imperfect optical focusing. When the power in the halo part exceeds a critical level for the self-focusing, it evolves in the plasma as an independent mode, which later gets coupled with the propagation of the central Gaussian spot of the pulse resulting in a novel instability. Here, this instability is investigated numerically via fully relativistic 3D particle-in-cell simulations and is shown to be partially suppressed by using plasma channels for pulse guiding. |
| abstract_unstemmed |
Strong disturbance in the wake of the laser pulses propagating in underdense plasma and consequent unstable electron acceleration by the wakefield can be provoked by pulse's halo, which always exists as a result of an imperfect optical focusing. When the power in the halo part exceeds a critical level for the self-focusing, it evolves in the plasma as an independent mode, which later gets coupled with the propagation of the central Gaussian spot of the pulse resulting in a novel instability. Here, this instability is investigated numerically via fully relativistic 3D particle-in-cell simulations and is shown to be partially suppressed by using plasma channels for pulse guiding. |
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Effect of halo on high power laser pulse wake in underdense plasma |
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<?xml version="1.0" encoding="UTF-8"?><collection xmlns="http://www.loc.gov/MARC21/slim"><record><leader>01000caa a2200265 4500</leader><controlfield tag="001">OLC1985755807</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20230714231641.0</controlfield><controlfield tag="007">tu</controlfield><controlfield tag="008">161202s2016 xx ||||| 00| ||eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1063/1.4968240</subfield><subfield code="2">doi</subfield></datafield><datafield tag="028" ind1="5" ind2="2"><subfield code="a">PQ20161201</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)OLC1985755807</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-599)GBVOLC1985755807</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(PRQ)scitation_primary_10_1063_1_49682400</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(KEY)0178548620160000023001100000effectofhaloonhighpowerlaserpulsewakeinunderdensep</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">DE-600</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Pathak, Naveen</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">Effect of halo on high power laser pulse wake in underdense plasma</subfield></datafield><datafield tag="264" ind1=" " ind2="1"><subfield code="c">2016</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="520" ind1=" " ind2=" "><subfield code="a">Strong disturbance in the wake of the laser pulses propagating in underdense plasma and consequent unstable electron acceleration by the wakefield can be provoked by pulse's halo, which always exists as a result of an imperfect optical focusing. When the power in the halo part exceeds a critical level for the self-focusing, it evolves in the plasma as an independent mode, which later gets coupled with the propagation of the central Gaussian spot of the pulse resulting in a novel instability. Here, this instability is investigated numerically via fully relativistic 3D particle-in-cell simulations and is shown to be partially suppressed by using plasma channels for pulse guiding.</subfield></datafield><datafield tag="540" ind1=" " ind2=" "><subfield code="a">Nutzungsrecht: © Author(s)</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Zhidkov, Alexei</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Masuda, Shinichi</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Hosokai, Tomonao</subfield><subfield code="4">oth</subfield></datafield><datafield tag="700" ind1="1" ind2=" "><subfield code="a">Kodama, Ryosuke</subfield><subfield code="4">oth</subfield></datafield><datafield tag="773" ind1="0" ind2="8"><subfield code="i">Enthalten in</subfield><subfield code="t">Physics of plasmas</subfield><subfield code="d">Melville, NY : AIP, 1994</subfield><subfield code="g">23(2016), 11</subfield><subfield code="w">(DE-627)171342119</subfield><subfield code="w">(DE-600)1179425-2</subfield><subfield code="w">(DE-576)038876949</subfield><subfield code="x">1070-664X</subfield><subfield code="7">nnns</subfield></datafield><datafield tag="773" ind1="1" ind2="8"><subfield code="g">volume:23</subfield><subfield code="g">year:2016</subfield><subfield code="g">number:11</subfield></datafield><datafield tag="856" ind1="4" ind2="1"><subfield code="u">http://dx.doi.org/10.1063/1.4968240</subfield><subfield code="3">Volltext</subfield></datafield><datafield tag="856" ind1="4" ind2="2"><subfield code="u">http://dx.doi.org/10.1063/1.4968240</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_USEFLAG_A</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SYSFLAG_A</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_OLC</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OLC-PHY</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OPC-AST</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OPC-GEO</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">SSG-OPC-GGO</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_47</subfield></datafield><datafield tag="912" ind1=" " ind2=" "><subfield code="a">GBV_ILN_70</subfield></datafield><datafield tag="951" ind1=" " ind2=" "><subfield code="a">AR</subfield></datafield><datafield tag="952" ind1=" " ind2=" "><subfield code="d">23</subfield><subfield code="j">2016</subfield><subfield code="e">11</subfield></datafield></record></collection>
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