ConstantID

Shielded helion gyromagnetic ratio

Atomic & nuclearMeasured

γh′ = 2.037 894 6078(18) × 108 s−1 T−1

Value
2.037 894 6078 × 108 s−1 T−1
Standard uncertainty
0.18 s−1 T−1
Relative uncertainty
8.8 × 10−10 (883 parts per trillion)
Status
Measured
Symbol
γh′
Source
CODATA 2022 via NIST · NIST entry

Use in a calculation

# shielded helion gyromagnetic ratio, CODATA 2022 (NIST)
shielded_helion_gyromagnetic_ratio = 2.0378946078e8  # s^-1 T^-1, standard uncertainty 0.18

# SciPy: scipy.constants.physical_constants['shielded helion gyromag. ratio']

What it is

The ratio of magnetic moment to angular momentum for a helion in a helium-3 gas atom (spherical sample at 25 °C), screened by the atom's two electrons. In a magnetic field B the spin precesses at angular frequency γB; this is the basis of magnetic resonance.

How the value changed, 1998–2022

Each point is one CODATA adjustment, plotted as its difference from the 2022 value; the bars show one standard uncertainty (an arrowhead means the bar runs off the chart).

shielded helion gyromagnetic ratio: CODATA values 1998–2022 relative to the 2022 value, in parts per billion, with one-standard-uncertainty bars−150−100−500+50+100+150parts per billion1998200220062010201420182022

Relative uncertainty

shielded helion gyromagnetic ratio: relative standard uncertainty in each CODATA adjustment, logarithmic scale10⁻¹⁰10⁻⁹10⁻⁸10⁻⁷1998200220062010201420182022
CODATAValue (uncertainty)Relative uncertaintyChange from previous
20222.037 894 6078(18) × 1088.8 × 10−10 +1.6 σ of 2018
20182.037 894 569(24) × 1081.2 × 10−8 −0.6 σ of 2014
20142.037 894 585(27) × 1081.3 × 10−8 −1.5 σ of 2010
20102.037 894 659(51) × 1082.5 × 10−8 −1.3 σ of 2006
20062.037 894 730(56) × 1082.7 × 10−8 +0.2 σ of 2002
20022.037 894 70(18) × 1088.8 × 10−8 −0.8 σ of 1998
19982.037 894 764(85) × 1084.2 × 10−8

“Change from previous” is the shift in the value divided by the standard uncertainty of the previous adjustment. Earlier values are converted into the current unit where NIST changed it (for example J s to J Hz⁻¹).

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