2007
DOI: 10.1134/s1054660x07080087
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First experiments on the observation of gamma resonance of a long-lived 109m Ag isomer using a gravitational gamma spectrometer

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Cited by 12 publications
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“…Given the importance of high f 0 and narrow linewidths, one can ask why we do not make the jump to very high frequencies such as those observed in Mössbauer spectroscopy. For example, a Mössbauer transition in 109 Ag has f 0 ≃ 2.1 × 10 19 Hz and a radiative decay time τ decay ≃ 60 s corresponding to a natural Q value ≃1.3 × 10 22 (Alpatov et al, 2007;Bayukov et al, 2009). Even with practical limitations, the performance of actual Mössbauer systems is still quite impressive.…”
Section: B High-frequency Clock Candidatesmentioning
confidence: 99%
“…Given the importance of high f 0 and narrow linewidths, one can ask why we do not make the jump to very high frequencies such as those observed in Mössbauer spectroscopy. For example, a Mössbauer transition in 109 Ag has f 0 ≃ 2.1 × 10 19 Hz and a radiative decay time τ decay ≃ 60 s corresponding to a natural Q value ≃1.3 × 10 22 (Alpatov et al, 2007;Bayukov et al, 2009). Even with practical limitations, the performance of actual Mössbauer systems is still quite impressive.…”
Section: B High-frequency Clock Candidatesmentioning
confidence: 99%
“…Given the importance of high f 0 and narrow linewidths, one can ask why we don't make the jump to very high frequencies such as those observed in Mössbauer spectroscopy. For example, a Mössbauer transition in 109 Ag has f 0 2.1 × 10 19 Hz and a radiative decay time τ decay 60 s corresponding to a natural Q value 1.3 × 10 22 (Alpatov et al, 2007;Bayukov et al, 2009). Even with practical limitations, the performance of actual Mössbauer systems is still quite impressive.…”
Section: B High-frequency Clock Candidatesmentioning
confidence: 99%