Molecular-Orbital K X-Ray Formation in Heavy-Ion Collisions
In order to complete the identification of molecular-orbital K x-ray spectra, we have worked out the expected spectral yields and compared them with experimental spectra produced by 30- and 60-MeV Br and 82- MeV I beams. Independently, we have determined the dominant mechanism of molecular-orbital K...
Ausführliche Beschreibung
Gespeichert in:
| Autor*in: |
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| Format: |
E-Artikel |
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| Erschienen: |
1974 |
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| Umfang: |
Online-Ressource 4 |
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| Reproduktion: |
APS Digital Backfile Archive 1893-2003 |
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| Übergeordnetes Werk: |
Enthalten in: Physical review letters - College Park, Md. : APS, 1958, 32(1974), 23, Seite 1279-1282 |
| Übergeordnetes Werk: |
volume:32 ; year:1974 ; number:23 ; pages:1279-1282 ; extent:4 |
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| 520 | |a In order to complete the identification of molecular-orbital K x-ray spectra, we have worked out the expected spectral yields and compared them with experimental spectra produced by 30- and 60-MeV Br and 82- MeV I beams. Independently, we have determined the dominant mechanism of molecular-orbital K x-ray production in 30-MeV Br + Br collisions by diluting the Br density in a solid target. | ||
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(DE-627)NLEJ251153959 (DE-601)aps:5434290101d6e3b3f8d0b180e1792598e1a7bbc2 DE-627 ger DE-627 rakwb Molecular-Orbital K X-Ray Formation in Heavy-Ion Collisions 1974 Online-Ressource 4 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier In order to complete the identification of molecular-orbital K x-ray spectra, we have worked out the expected spectral yields and compared them with experimental spectra produced by 30- and 60-MeV Br and 82- MeV I beams. Independently, we have determined the dominant mechanism of molecular-orbital K x-ray production in 30-MeV Br + Br collisions by diluting the Br density in a solid target. APS Digital Backfile Archive 1893-2003 Meyerhof, W. E. oth Saylor, T. K. oth Lazarus, S. M. oth Little, A. oth Triplett, B. B. oth Enthalten in Physical review letters College Park, Md. : APS, 1958 32(1974), 23, Seite 1279-1282 Online-Ressource (DE-627)NLEJ248237888 (DE-600)1472655-5 1079-7114 nnns volume:32 year:1974 number:23 pages:1279-1282 extent:4 https://www.tib.eu/de/suchen/id/aps%3A5434290101d6e3b3f8d0b180e1792598e1a7bbc2 Verlag Deutschlandweit zugänglich GBV_USEFLAG_U ZDB-1-APS GBV_NL_ARTICLE AR 32 1974 23 1279-1282 4 |
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(DE-627)NLEJ251153959 (DE-601)aps:5434290101d6e3b3f8d0b180e1792598e1a7bbc2 DE-627 ger DE-627 rakwb Molecular-Orbital K X-Ray Formation in Heavy-Ion Collisions 1974 Online-Ressource 4 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier In order to complete the identification of molecular-orbital K x-ray spectra, we have worked out the expected spectral yields and compared them with experimental spectra produced by 30- and 60-MeV Br and 82- MeV I beams. Independently, we have determined the dominant mechanism of molecular-orbital K x-ray production in 30-MeV Br + Br collisions by diluting the Br density in a solid target. APS Digital Backfile Archive 1893-2003 Meyerhof, W. E. oth Saylor, T. K. oth Lazarus, S. M. oth Little, A. oth Triplett, B. B. oth Enthalten in Physical review letters College Park, Md. : APS, 1958 32(1974), 23, Seite 1279-1282 Online-Ressource (DE-627)NLEJ248237888 (DE-600)1472655-5 1079-7114 nnns volume:32 year:1974 number:23 pages:1279-1282 extent:4 https://www.tib.eu/de/suchen/id/aps%3A5434290101d6e3b3f8d0b180e1792598e1a7bbc2 Verlag Deutschlandweit zugänglich GBV_USEFLAG_U ZDB-1-APS GBV_NL_ARTICLE AR 32 1974 23 1279-1282 4 |
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(DE-627)NLEJ251153959 (DE-601)aps:5434290101d6e3b3f8d0b180e1792598e1a7bbc2 DE-627 ger DE-627 rakwb Molecular-Orbital K X-Ray Formation in Heavy-Ion Collisions 1974 Online-Ressource 4 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier In order to complete the identification of molecular-orbital K x-ray spectra, we have worked out the expected spectral yields and compared them with experimental spectra produced by 30- and 60-MeV Br and 82- MeV I beams. Independently, we have determined the dominant mechanism of molecular-orbital K x-ray production in 30-MeV Br + Br collisions by diluting the Br density in a solid target. APS Digital Backfile Archive 1893-2003 Meyerhof, W. E. oth Saylor, T. K. oth Lazarus, S. M. oth Little, A. oth Triplett, B. B. oth Enthalten in Physical review letters College Park, Md. : APS, 1958 32(1974), 23, Seite 1279-1282 Online-Ressource (DE-627)NLEJ248237888 (DE-600)1472655-5 1079-7114 nnns volume:32 year:1974 number:23 pages:1279-1282 extent:4 https://www.tib.eu/de/suchen/id/aps%3A5434290101d6e3b3f8d0b180e1792598e1a7bbc2 Verlag Deutschlandweit zugänglich GBV_USEFLAG_U ZDB-1-APS GBV_NL_ARTICLE AR 32 1974 23 1279-1282 4 |
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(DE-627)NLEJ251153959 (DE-601)aps:5434290101d6e3b3f8d0b180e1792598e1a7bbc2 DE-627 ger DE-627 rakwb Molecular-Orbital K X-Ray Formation in Heavy-Ion Collisions 1974 Online-Ressource 4 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier In order to complete the identification of molecular-orbital K x-ray spectra, we have worked out the expected spectral yields and compared them with experimental spectra produced by 30- and 60-MeV Br and 82- MeV I beams. Independently, we have determined the dominant mechanism of molecular-orbital K x-ray production in 30-MeV Br + Br collisions by diluting the Br density in a solid target. APS Digital Backfile Archive 1893-2003 Meyerhof, W. E. oth Saylor, T. K. oth Lazarus, S. M. oth Little, A. oth Triplett, B. B. oth Enthalten in Physical review letters College Park, Md. : APS, 1958 32(1974), 23, Seite 1279-1282 Online-Ressource (DE-627)NLEJ248237888 (DE-600)1472655-5 1079-7114 nnns volume:32 year:1974 number:23 pages:1279-1282 extent:4 https://www.tib.eu/de/suchen/id/aps%3A5434290101d6e3b3f8d0b180e1792598e1a7bbc2 Verlag Deutschlandweit zugänglich GBV_USEFLAG_U ZDB-1-APS GBV_NL_ARTICLE AR 32 1974 23 1279-1282 4 |
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(DE-627)NLEJ251153959 (DE-601)aps:5434290101d6e3b3f8d0b180e1792598e1a7bbc2 DE-627 ger DE-627 rakwb Molecular-Orbital K X-Ray Formation in Heavy-Ion Collisions 1974 Online-Ressource 4 Text txt rdacontent Computermedien c rdamedia Online-Ressource cr rdacarrier In order to complete the identification of molecular-orbital K x-ray spectra, we have worked out the expected spectral yields and compared them with experimental spectra produced by 30- and 60-MeV Br and 82- MeV I beams. Independently, we have determined the dominant mechanism of molecular-orbital K x-ray production in 30-MeV Br + Br collisions by diluting the Br density in a solid target. APS Digital Backfile Archive 1893-2003 Meyerhof, W. E. oth Saylor, T. K. oth Lazarus, S. M. oth Little, A. oth Triplett, B. B. oth Enthalten in Physical review letters College Park, Md. : APS, 1958 32(1974), 23, Seite 1279-1282 Online-Ressource (DE-627)NLEJ248237888 (DE-600)1472655-5 1079-7114 nnns volume:32 year:1974 number:23 pages:1279-1282 extent:4 https://www.tib.eu/de/suchen/id/aps%3A5434290101d6e3b3f8d0b180e1792598e1a7bbc2 Verlag Deutschlandweit zugänglich GBV_USEFLAG_U ZDB-1-APS GBV_NL_ARTICLE AR 32 1974 23 1279-1282 4 |
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molecular-orbital k x-ray formation in heavy-ion collisions |
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Molecular-Orbital K X-Ray Formation in Heavy-Ion Collisions |
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In order to complete the identification of molecular-orbital K x-ray spectra, we have worked out the expected spectral yields and compared them with experimental spectra produced by 30- and 60-MeV Br and 82- MeV I beams. Independently, we have determined the dominant mechanism of molecular-orbital K x-ray production in 30-MeV Br + Br collisions by diluting the Br density in a solid target. |
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In order to complete the identification of molecular-orbital K x-ray spectra, we have worked out the expected spectral yields and compared them with experimental spectra produced by 30- and 60-MeV Br and 82- MeV I beams. Independently, we have determined the dominant mechanism of molecular-orbital K x-ray production in 30-MeV Br + Br collisions by diluting the Br density in a solid target. |
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In order to complete the identification of molecular-orbital K x-ray spectra, we have worked out the expected spectral yields and compared them with experimental spectra produced by 30- and 60-MeV Br and 82- MeV I beams. Independently, we have determined the dominant mechanism of molecular-orbital K x-ray production in 30-MeV Br + Br collisions by diluting the Br density in a solid target. |
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