2006
DOI: 10.1007/s10751-005-9217-x
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Laser Cooling and Spectroscopy of Relativistic C $$^{3+}$$ Beams at the ESR

Abstract: We report on the first laser cooling of a bunched beam of multiply charged C 3þ ions performed at the ESR (GSI) at a beam energy of E ¼ 1:47 GeV. Moderate bunching provided a force counteracting the decelerating laser force of one counterpropagating laser beam. This versatile type of laser cooling lead to longitudinally space-charge dominated beams with an unprecedented momentum spread of Áp=p % 10 À7 . Concerning the beam energy and charge state of the ion, the experiment depicts an important intermediate ste… Show more

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Cited by 14 publications
(5 citation statements)
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“…7 or 8 ), of high importance for the astrophysical community where they are used for diagnostics of hot plasmas in the interstellar medium and stellar atmospheres 9 . The wavelengths of the two transitions have also been determined during a previous laser-cooling experiment at the ESR 10 , but were in conflict with earlier results from plasma spectroscopy 11 and from interferometric measurements 9 . In this new measurement special emphasis is therefore placed on a careful calibration of all experimental components and a thorough analysis of the systematic uncertainties.…”
Section: Introductionmentioning
confidence: 59%
See 1 more Smart Citation
“…7 or 8 ), of high importance for the astrophysical community where they are used for diagnostics of hot plasmas in the interstellar medium and stellar atmospheres 9 . The wavelengths of the two transitions have also been determined during a previous laser-cooling experiment at the ESR 10 , but were in conflict with earlier results from plasma spectroscopy 11 and from interferometric measurements 9 . In this new measurement special emphasis is therefore placed on a careful calibration of all experimental components and a thorough analysis of the systematic uncertainties.…”
Section: Introductionmentioning
confidence: 59%
“…', the corresponding contribution to the error budget of the wavelength has been estimated by omitting the correction from the analysis. 11 1963 plasma spectroscopy 155.0774 (10) 154.8202(10) Theory: Yerokhin et al 8 2017 RCI a 155.080 (29) 154.827(36) Borschevsky 35 2014 FSCC b 155.075 154.820 Tupitsyn et al 10 2003 n/a 155.0739 (26) 154.8173(53) Johnson et al 36 1996 RMBPT c 155.078 154.819 Kim et al 37 1991…”
Section: Resonance Analysismentioning
confidence: 99%
“…7 or 8 ), of high importance for the astrophysical community where they are used for diagnostics of hot plasmas in the interstellar medium and stellar atmospheres 9 . The wavelengths of the two transitions have also been determined during a previous laser-cooling experiment at the ESR 10 , but were in conflict with earlier results from plasma spectroscopy 11 and from interferometric measurements 9 . In this new measurement special emphasis is therefore placed on a careful calibration of all experimental components and a thorough analysis of the systematic uncertainties.…”
Section: Introductionmentioning
confidence: 60%
“…Development of electron cooling schemes for ultra relativistic ion beams are underway at BNL [52], for example. The new HE-storage rings at the FAIR facility in Germany will in time enable experiments with laser cooling of highly relativistic beams [53].…”
Section: B Momentum Spread Requirements and Coulomb Crystals In Stormentioning
confidence: 99%