On very short and intense laser–plasma interactions
Abstract We briefly report on some results regarding the impact of very short and intense laser pulses on a cold, low-density plasma initially at rest, and the consequent acceleration of plasma electrons to relativistic energies. Locally and for short times the pulse can be described by a transverse...
Ausführliche Beschreibung
Autor*in: |
Fiore, Gaetano [verfasserIn] |
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Format: |
Artikel |
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Sprache: |
Englisch |
Erschienen: |
2016 |
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Anmerkung: |
© Università degli Studi di Napoli "Federico II" 2016 |
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Übergeordnetes Werk: |
Enthalten in: Ricerche di matematica - Springer Milan, 1952, 65(2016), 2 vom: 06. Apr., Seite 491-503 |
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Übergeordnetes Werk: |
volume:65 ; year:2016 ; number:2 ; day:06 ; month:04 ; pages:491-503 |
Links: |
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DOI / URN: |
10.1007/s11587-016-0270-3 |
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Katalog-ID: |
OLC2055583085 |
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10.1007/s11587-016-0270-3 doi (DE-627)OLC2055583085 (DE-He213)s11587-016-0270-3-p DE-627 ger DE-627 rakwb eng 510 VZ Fiore, Gaetano verfasserin aut On very short and intense laser–plasma interactions 2016 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Università degli Studi di Napoli "Federico II" 2016 Abstract We briefly report on some results regarding the impact of very short and intense laser pulses on a cold, low-density plasma initially at rest, and the consequent acceleration of plasma electrons to relativistic energies. Locally and for short times the pulse can be described by a transverse plane electromagnetic travelling-wave and the motion of the electrons by a purely Magneto-Fluido-Dynamical model with a very simple dependence on the transverse electromagnetic potential, while the ions can be regarded as at rest; the Lorentz–Maxwell and continuity equations are reduced to the Hamilton equations of a Hamiltonian system with 1 degree of freedom, in the case of a plasma with constant initial density, or a collection of such systems otherwise. We can thus describe both the well-known wakefield behind the pulse and the recently predicted slingshot effect, i.e. the backward expulsion of high energy electrons just after the laser pulse has hit the surface of the plasma. Nonlinear PDEs Laser–plasma interactions Laser-driven acceleration Enthalten in Ricerche di matematica Springer Milan, 1952 65(2016), 2 vom: 06. Apr., Seite 491-503 (DE-627)129853259 (DE-600)280837-7 (DE-576)015154122 0035-5038 nnns volume:65 year:2016 number:2 day:06 month:04 pages:491-503 https://doi.org/10.1007/s11587-016-0270-3 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-MAT SSG-OPC-MAT GBV_ILN_62 GBV_ILN_2010 AR 65 2016 2 06 04 491-503 |
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10.1007/s11587-016-0270-3 doi (DE-627)OLC2055583085 (DE-He213)s11587-016-0270-3-p DE-627 ger DE-627 rakwb eng 510 VZ Fiore, Gaetano verfasserin aut On very short and intense laser–plasma interactions 2016 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Università degli Studi di Napoli "Federico II" 2016 Abstract We briefly report on some results regarding the impact of very short and intense laser pulses on a cold, low-density plasma initially at rest, and the consequent acceleration of plasma electrons to relativistic energies. Locally and for short times the pulse can be described by a transverse plane electromagnetic travelling-wave and the motion of the electrons by a purely Magneto-Fluido-Dynamical model with a very simple dependence on the transverse electromagnetic potential, while the ions can be regarded as at rest; the Lorentz–Maxwell and continuity equations are reduced to the Hamilton equations of a Hamiltonian system with 1 degree of freedom, in the case of a plasma with constant initial density, or a collection of such systems otherwise. We can thus describe both the well-known wakefield behind the pulse and the recently predicted slingshot effect, i.e. the backward expulsion of high energy electrons just after the laser pulse has hit the surface of the plasma. Nonlinear PDEs Laser–plasma interactions Laser-driven acceleration Enthalten in Ricerche di matematica Springer Milan, 1952 65(2016), 2 vom: 06. Apr., Seite 491-503 (DE-627)129853259 (DE-600)280837-7 (DE-576)015154122 0035-5038 nnns volume:65 year:2016 number:2 day:06 month:04 pages:491-503 https://doi.org/10.1007/s11587-016-0270-3 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-MAT SSG-OPC-MAT GBV_ILN_62 GBV_ILN_2010 AR 65 2016 2 06 04 491-503 |
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10.1007/s11587-016-0270-3 doi (DE-627)OLC2055583085 (DE-He213)s11587-016-0270-3-p DE-627 ger DE-627 rakwb eng 510 VZ Fiore, Gaetano verfasserin aut On very short and intense laser–plasma interactions 2016 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Università degli Studi di Napoli "Federico II" 2016 Abstract We briefly report on some results regarding the impact of very short and intense laser pulses on a cold, low-density plasma initially at rest, and the consequent acceleration of plasma electrons to relativistic energies. Locally and for short times the pulse can be described by a transverse plane electromagnetic travelling-wave and the motion of the electrons by a purely Magneto-Fluido-Dynamical model with a very simple dependence on the transverse electromagnetic potential, while the ions can be regarded as at rest; the Lorentz–Maxwell and continuity equations are reduced to the Hamilton equations of a Hamiltonian system with 1 degree of freedom, in the case of a plasma with constant initial density, or a collection of such systems otherwise. We can thus describe both the well-known wakefield behind the pulse and the recently predicted slingshot effect, i.e. the backward expulsion of high energy electrons just after the laser pulse has hit the surface of the plasma. Nonlinear PDEs Laser–plasma interactions Laser-driven acceleration Enthalten in Ricerche di matematica Springer Milan, 1952 65(2016), 2 vom: 06. Apr., Seite 491-503 (DE-627)129853259 (DE-600)280837-7 (DE-576)015154122 0035-5038 nnns volume:65 year:2016 number:2 day:06 month:04 pages:491-503 https://doi.org/10.1007/s11587-016-0270-3 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-MAT SSG-OPC-MAT GBV_ILN_62 GBV_ILN_2010 AR 65 2016 2 06 04 491-503 |
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10.1007/s11587-016-0270-3 doi (DE-627)OLC2055583085 (DE-He213)s11587-016-0270-3-p DE-627 ger DE-627 rakwb eng 510 VZ Fiore, Gaetano verfasserin aut On very short and intense laser–plasma interactions 2016 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Università degli Studi di Napoli "Federico II" 2016 Abstract We briefly report on some results regarding the impact of very short and intense laser pulses on a cold, low-density plasma initially at rest, and the consequent acceleration of plasma electrons to relativistic energies. Locally and for short times the pulse can be described by a transverse plane electromagnetic travelling-wave and the motion of the electrons by a purely Magneto-Fluido-Dynamical model with a very simple dependence on the transverse electromagnetic potential, while the ions can be regarded as at rest; the Lorentz–Maxwell and continuity equations are reduced to the Hamilton equations of a Hamiltonian system with 1 degree of freedom, in the case of a plasma with constant initial density, or a collection of such systems otherwise. We can thus describe both the well-known wakefield behind the pulse and the recently predicted slingshot effect, i.e. the backward expulsion of high energy electrons just after the laser pulse has hit the surface of the plasma. Nonlinear PDEs Laser–plasma interactions Laser-driven acceleration Enthalten in Ricerche di matematica Springer Milan, 1952 65(2016), 2 vom: 06. Apr., Seite 491-503 (DE-627)129853259 (DE-600)280837-7 (DE-576)015154122 0035-5038 nnns volume:65 year:2016 number:2 day:06 month:04 pages:491-503 https://doi.org/10.1007/s11587-016-0270-3 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-MAT SSG-OPC-MAT GBV_ILN_62 GBV_ILN_2010 AR 65 2016 2 06 04 491-503 |
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10.1007/s11587-016-0270-3 doi (DE-627)OLC2055583085 (DE-He213)s11587-016-0270-3-p DE-627 ger DE-627 rakwb eng 510 VZ Fiore, Gaetano verfasserin aut On very short and intense laser–plasma interactions 2016 Text txt rdacontent ohne Hilfsmittel zu benutzen n rdamedia Band nc rdacarrier © Università degli Studi di Napoli "Federico II" 2016 Abstract We briefly report on some results regarding the impact of very short and intense laser pulses on a cold, low-density plasma initially at rest, and the consequent acceleration of plasma electrons to relativistic energies. Locally and for short times the pulse can be described by a transverse plane electromagnetic travelling-wave and the motion of the electrons by a purely Magneto-Fluido-Dynamical model with a very simple dependence on the transverse electromagnetic potential, while the ions can be regarded as at rest; the Lorentz–Maxwell and continuity equations are reduced to the Hamilton equations of a Hamiltonian system with 1 degree of freedom, in the case of a plasma with constant initial density, or a collection of such systems otherwise. We can thus describe both the well-known wakefield behind the pulse and the recently predicted slingshot effect, i.e. the backward expulsion of high energy electrons just after the laser pulse has hit the surface of the plasma. Nonlinear PDEs Laser–plasma interactions Laser-driven acceleration Enthalten in Ricerche di matematica Springer Milan, 1952 65(2016), 2 vom: 06. Apr., Seite 491-503 (DE-627)129853259 (DE-600)280837-7 (DE-576)015154122 0035-5038 nnns volume:65 year:2016 number:2 day:06 month:04 pages:491-503 https://doi.org/10.1007/s11587-016-0270-3 lizenzpflichtig Volltext GBV_USEFLAG_A SYSFLAG_A GBV_OLC SSG-OLC-MAT SSG-OPC-MAT GBV_ILN_62 GBV_ILN_2010 AR 65 2016 2 06 04 491-503 |
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Abstract We briefly report on some results regarding the impact of very short and intense laser pulses on a cold, low-density plasma initially at rest, and the consequent acceleration of plasma electrons to relativistic energies. Locally and for short times the pulse can be described by a transverse plane electromagnetic travelling-wave and the motion of the electrons by a purely Magneto-Fluido-Dynamical model with a very simple dependence on the transverse electromagnetic potential, while the ions can be regarded as at rest; the Lorentz–Maxwell and continuity equations are reduced to the Hamilton equations of a Hamiltonian system with 1 degree of freedom, in the case of a plasma with constant initial density, or a collection of such systems otherwise. We can thus describe both the well-known wakefield behind the pulse and the recently predicted slingshot effect, i.e. the backward expulsion of high energy electrons just after the laser pulse has hit the surface of the plasma. © Università degli Studi di Napoli "Federico II" 2016 |
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Abstract We briefly report on some results regarding the impact of very short and intense laser pulses on a cold, low-density plasma initially at rest, and the consequent acceleration of plasma electrons to relativistic energies. Locally and for short times the pulse can be described by a transverse plane electromagnetic travelling-wave and the motion of the electrons by a purely Magneto-Fluido-Dynamical model with a very simple dependence on the transverse electromagnetic potential, while the ions can be regarded as at rest; the Lorentz–Maxwell and continuity equations are reduced to the Hamilton equations of a Hamiltonian system with 1 degree of freedom, in the case of a plasma with constant initial density, or a collection of such systems otherwise. We can thus describe both the well-known wakefield behind the pulse and the recently predicted slingshot effect, i.e. the backward expulsion of high energy electrons just after the laser pulse has hit the surface of the plasma. © Università degli Studi di Napoli "Federico II" 2016 |
abstract_unstemmed |
Abstract We briefly report on some results regarding the impact of very short and intense laser pulses on a cold, low-density plasma initially at rest, and the consequent acceleration of plasma electrons to relativistic energies. Locally and for short times the pulse can be described by a transverse plane electromagnetic travelling-wave and the motion of the electrons by a purely Magneto-Fluido-Dynamical model with a very simple dependence on the transverse electromagnetic potential, while the ions can be regarded as at rest; the Lorentz–Maxwell and continuity equations are reduced to the Hamilton equations of a Hamiltonian system with 1 degree of freedom, in the case of a plasma with constant initial density, or a collection of such systems otherwise. We can thus describe both the well-known wakefield behind the pulse and the recently predicted slingshot effect, i.e. the backward expulsion of high energy electrons just after the laser pulse has hit the surface of the plasma. © Università degli Studi di Napoli "Federico II" 2016 |
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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">OLC2055583085</controlfield><controlfield tag="003">DE-627</controlfield><controlfield tag="005">20230401113442.0</controlfield><controlfield tag="007">tu</controlfield><controlfield tag="008">200819s2016 xx ||||| 00| ||eng c</controlfield><datafield tag="024" ind1="7" ind2=" "><subfield code="a">10.1007/s11587-016-0270-3</subfield><subfield code="2">doi</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-627)OLC2055583085</subfield></datafield><datafield tag="035" ind1=" " ind2=" "><subfield code="a">(DE-He213)s11587-016-0270-3-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">510</subfield><subfield code="q">VZ</subfield></datafield><datafield tag="100" ind1="1" ind2=" "><subfield code="a">Fiore, Gaetano</subfield><subfield code="e">verfasserin</subfield><subfield code="4">aut</subfield></datafield><datafield tag="245" ind1="1" ind2="0"><subfield code="a">On very short and intense laser–plasma interactions</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="500" ind1=" " ind2=" "><subfield code="a">© Università degli Studi di Napoli "Federico II" 2016</subfield></datafield><datafield tag="520" ind1=" " ind2=" "><subfield code="a">Abstract We briefly report on some results regarding the impact of very short and intense laser pulses on a cold, low-density plasma initially at rest, and the consequent acceleration of plasma electrons to relativistic energies. Locally and for short times the pulse can be described by a transverse plane electromagnetic travelling-wave and the motion of the electrons by a purely Magneto-Fluido-Dynamical model with a very simple dependence on the transverse electromagnetic potential, while the ions can be regarded as at rest; the Lorentz–Maxwell and continuity equations are reduced to the Hamilton equations of a Hamiltonian system with 1 degree of freedom, in the case of a plasma with constant initial density, or a collection of such systems otherwise. We can thus describe both the well-known wakefield behind the pulse and the recently predicted slingshot effect, i.e. the backward expulsion of high energy electrons just after the laser pulse has hit the surface of the plasma.</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Nonlinear PDEs</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Laser–plasma interactions</subfield></datafield><datafield tag="650" ind1=" " ind2="4"><subfield code="a">Laser-driven acceleration</subfield></datafield><datafield tag="773" ind1="0" ind2="8"><subfield code="i">Enthalten in</subfield><subfield code="t">Ricerche di matematica</subfield><subfield code="d">Springer Milan, 1952</subfield><subfield code="g">65(2016), 2 vom: 06. 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