Abstract:We observed and directly measured the M1 transition between the two states of the fine structure splitting in the ground state of Ba 7+ with a visible spectrometer coupled to a compact electron beam ion trap. To validate the measurement accuracy, we demonstrated a calibration method using Ar + emissions from buffer gas. The wavenumber in vacuum was determined to be 23591.57 (15) cm −1 .
“…The total wavelength uncertainty of this observation and calibration scheme was approximately 2 pm, which was comparable to the uncertainty of the scheme that the measured lines were calibrated by the lines from the buffer gas observed by a similar resolution spectrograph [44,45], but larger than the uncertainty of the scheme that the calibration source was overlapped with the real image of the ion observed by a higher resolution spectrograph [42]. Compared to these two schemes, our scheme is more convenient and flexible.…”
“…The total wavelength uncertainty of this observation and calibration scheme was approximately 2 pm, which was comparable to the uncertainty of the scheme that the measured lines were calibrated by the lines from the buffer gas observed by a similar resolution spectrograph [44,45], but larger than the uncertainty of the scheme that the calibration source was overlapped with the real image of the ion observed by a higher resolution spectrograph [42]. Compared to these two schemes, our scheme is more convenient and flexible.…”
“…Typical emission line intensities of Ne and Ar + increased linearly with the amount of injected buffer gas. The emission line around 423 nm was related to the M1 transition between fine-structures in the ground configuration of Ba 7+ , which we reported in the previous paper [17]. We assigned the emission line of Ba 8+ around 500 nm to the 3 P 1 -3 P 2 transitions in the first excited electron configuration [Kr]4d 10 5s5p by comparing its wavelength with the energy levels of Ba 8+ previously investigated by extreme ultraviolet(EUV) emission spectroscopy [30].…”
Section: Emission Spectra Of Mixed Species Of Ba Hcis and Noble Gasesmentioning
confidence: 80%
“…The experiments involved injecting elemental Ba, I, Ne, and Ar into CoBIT. Ba atoms were injected by evaporating the cathode material (BaO) of the electron gun [17,18]. The Ne and Ar gases were introduced into CoBIT as buffer gases using a gas injector through a variable leak valve.…”
Section: Methodsmentioning
confidence: 99%
“…Γ q = γ q ) for several HCIs with an M1 transition that prominently emits at visible and near-visible wavelengths. Our previous papers [17,18] reported the simultaneous observation of emission lines of Ba 7+ and Ar + , and of Ba 6+ and neutral Ne. We also simulutaneously observed a near-infrared emission line of I 8+ and reference lines of neutral Ne [22], although the spectrum was not previously presented.…”
Section: Estimation Of the Survival Of Hcis In An Ebit With Buffer No...mentioning
confidence: 99%
“…The Freiberg and Heidelberg EBIT group succeeded in this simultaneous observation of the visible emission of Ar 13+ and the reference emission from Ar and Ar + by introducing a lot of Ar gas three times higher than usual [14][15][16]. Recently, we demonstrated a versatile calibration method for the visible and near-visible wavelength range using buffer noble gases different elements from objective HCIs [17,18]. This calibration method can be applied to various heavy HCIs, not only highly charged noble gas ions, and has since been adopted by the Shanghai EBIT group [19,20].…”
Spectral lines of buffer noble gases injected into an electron beam ion trap have recently been used as a reference to aid accurate determination of the wavelengths of optical transitions of highly charged ions. Simultaneous observation of emission lines of highly charged ions along with those of neutral atoms or singly charged ions represents a reliable method for wavelength calibration that suppresses systematic uncertainties. Here, we present visible and infrared emission spectra of buffer Ne and Ar gases in an electron beam ion trap and briefly review the buffer gas calibration method. The experimental conditions required for implementing the calibration method are discussed by investigating the dependence of the emission spectra of mixtures of highly charged ions and noble gases on electron beam’s parameters and gas pressure.
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