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A determination of the molar gas constant R (and the Boltzmann constant k) by acoustic thermometry in helium Roberto M. Gavioso Fundamental constants meeting - Eltville - February 2015 Physikalisch-Technische Bundesanstalt

Gavioso INRiM molar gas constant R rev - BIPM · estimate of the molar mass flowing 100 sccm est. outgassing rate 1.4 x 10-11 mol m−2 s−1 • we have a direct measurement of pressure

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Page 1: Gavioso INRiM molar gas constant R rev - BIPM · estimate of the molar mass flowing 100 sccm est. outgassing rate 1.4 x 10-11 mol m−2 s−1 • we have a direct measurement of pressure

A determination of the molar gas constant R (and the Boltzmann constant k) by acoustic thermometry in helium

Roberto M. Gavioso

Fundamental constants meeting - Eltville - February 2015

Physikalisch-Technische Bundesanstalt

Page 2: Gavioso INRiM molar gas constant R rev - BIPM · estimate of the molar mass flowing 100 sccm est. outgassing rate 1.4 x 10-11 mol m−2 s−1 • we have a direct measurement of pressure

design feature 1: use a sphere and induce the geometrical defect which is needed to lift the degeneracy of microwave modes by a slight misalignment of the comprising hemispheres

design feature 2: use helium

experiment design (2007)

con: no geometrical perturbation models for acoustics and microwaves (not in 2007, neither in 2015). For ellipsoids these models became available in 2007 and 2009.

pro: the results of tests with small steel cavities made by 2007 suggested that this method might work satisfactorily by using a larger copper cavity.

cons:• contamination from common

impurities has a ten-fold effect with respect to argon;

• in a copper cavity, some acoustic perturbations have a larger effect (thermal accomodation)

pros: • less problems from isotopes• helium is calculable from theory

(thermodynamic, transport and electrical properties)

• in a copper cavity, some acoustic perturbations have a smaller effect (shell recoil)

He vs Arsphere vs ellipsoid

Page 3: Gavioso INRiM molar gas constant R rev - BIPM · estimate of the molar mass flowing 100 sccm est. outgassing rate 1.4 x 10-11 mol m−2 s−1 • we have a direct measurement of pressure

cavity: a copper sphere with an internal radius of 90 mm; the two comprising hemispheres have geometrical defects within a few microns.

the hemispheres can be micrometrically misaligned by a simple mechanical system.

we prepare the resonator for measurements by inducing (by trial and error) the minimum perturbationneeded to achieve useful fitting precision (and accuracy, as tested in synthetic fits)

example of fitting results - TE15 tripletsinglet 1 singlet 2 singlet 3

frequencies / MHz 9122.3364 9122.5251 9122.6960

halfwidths / MHz 0.0353 0.0351 0.0365

ur (fit) / ppm 0.034 0.022 0.026

this level of precision is achieved for five TM modes(TM11 to TM15) and 4 TE modes (TE13 to TE16)antennas are designed to minimize coupling with the cavity

design features and preparation of the resonator

frequency /GHz

Re(

S12

), Im

(S12

), |S

12| /

mu

TE15400 kHz

Page 4: Gavioso INRiM molar gas constant R rev - BIPM · estimate of the molar mass flowing 100 sccm est. outgassing rate 1.4 x 10-11 mol m−2 s−1 • we have a direct measurement of pressure

microwave determination of the mean cavity radius

0 2 4 6 8 10 1290.06922

90.06924

90.06926

90.06928

90.06930

90.06932

90.06934

90.06936

TE16TM12

skin by gExp

skin by est. Cu

skin + geometry skin + geometry + antennas and ducts

radi

us /

mm

frequency / GHz

TM11

-0.6

-0.4

-0.2

0.0

0.2

0.4

0.6

0.8

rela

tive

chan

ge /

ppm

perturbations and corrections: surface resistivity, two antennas (as waveguides), three ducts, geometry (ellipsoidal approximation)

• discrepancy of TM11 mode is due to perturbation from loop antennas (as demonstrated by substitution tests);

• approximating the shape of our assembled cavity with an ellipsoid works well: i) it reduces the dispersion of 8 modes TM12 to TE16 by a factor 5; the relative separation within the triplets gives shape factors which are consistent for the whole set of 11 mw modes and extremely stable as a function of p and T:

1 = (1.969 ± 0.005) × 10-4 2 = (1.018 ± 0.002) × 10-4

• applying (or not) the corresponding geometrical correction on both AC and MW fields changes the determined values of R and k by only 0.2 ppm

0 100 200 300 400 500 600 70090.06910

90.06915

90.06920

90.06925

90.06930 TM12 TM13 TM14 TM15 TE13 TE14 TE15 TE16

mean all modes as a function of p

mean radius measured in vacuum

radi

us /

mm

pressure / kPa

He ,273.16n p

0,273.16 13Tka p a p

a0 = (90.069 2765 ± 0.000 0003) mm

using from theory

kT/3 = (7.484 ± 0.029) × 10-12 Pa-1

uncertainty budget for microwave determination of the squared cavity radiussource u / nm ur / ppm comments

riproducibility upon change of antennas or underestimate of perturbation from loop

probes21 0.23

section 3.1upper limit to the thickness of a possible

dielectric layer on resonator surface 15 0.17

estimate of surface resistivity 10 0.11 section 3.2

total (quadrature sum) a0 23.2 0.26total squared radius a0

2 0.52

Page 5: Gavioso INRiM molar gas constant R rev - BIPM · estimate of the molar mass flowing 100 sccm est. outgassing rate 1.4 x 10-11 mol m−2 s−1 • we have a direct measurement of pressure

speed of sound in helium

perturbations and corrections: boundary layer 2nd order, shell effects, two microphones, three ducts, geometry (ellipsoidal approximation)

experimental datasets: i) (high p - measurement set) nine purely radial modes (0,2) to (0,10) between 170 kPa and 690 kPa, near 273.16 K;ii) (low p - thermal accomodation set) same modes between 60 kPa and 105 kPa to estimate h

• mode (0,2) and (0,3) were rejected, due to evidence of large perturbations from shell modes • mode (0,8), (0,9) and (0,10) were rejected, due to evidence of overlapping with neighbouring modes at low pressure

0 100 200 300 400 500 600 700-20

-15

-10

-5

0

5

10

(0,2) (0,3) (0,4) (0,5) (0,6) (0,7) (0,8) (0,9) (0,10)

106 x

2

g (0,n

) / f (0

,n)

p / kPa

relative excess halfwidths

overlapping

our determination of h fitted from low pressure data of modes (0, 4) to (0,7) is not precise and not repeatable, with two inconsistent estimates from two isotherms repeated at a distance of a few months: h1 = (0.393 ± 0.009) ; h1 = (0.413 ± 0.009); we account for such inconsistency with a relevant uncertainty contribution in our speed of sound measurement; we note that our first estimate is consistent with a recent accurate estimate obtained at LNE-CNAM: h1 = (0.3926 ± 0.001)

overlapping

shell

0 100 200 300 400 500 600 700-80

-70

-60

-50

-40

-30

-20

-10

0

10

20

106 x

(u2 (0

, n) -

u2 re

f) / u

2 ref

p / kPa

(0,2) (0,3) (0,4) (0,5) (0,6) (0,7) (0,8) (0,9) (0,10)

Page 6: Gavioso INRiM molar gas constant R rev - BIPM · estimate of the molar mass flowing 100 sccm est. outgassing rate 1.4 x 10-11 mol m−2 s−1 • we have a direct measurement of pressure

speed of sound in helium extrapolation to zero pressure

we use a single weighted linear fit with:

2 1 21 2 0 1, 273.16u p A p A p A A p

where:• A-1 is fixed to our best estimate h = 0.393;• A2 is fixed by theoretical calculated value of the acoustic

virial coefficients of helium with negligible additional uncertainty

• fitting weights are equal to the standard uncertainty of repeated measurements of each datum

uncertainty budget for squared speed of sound at zero pressure at 273.16 K 

source u / m2 s‐2 ur / ppm

dispersion of four radial acoustic modes 0.54 0.57

squared microwave radius 0.49 0.52

imperfect estimate of thermal accomodation coefficient h 0.41 0.43

thermal conductivity of helium 0.02 0.03

pressure 0.09 0.10

geometrical correction 0.07 0.08

ducts correction 0.10 0.11

microphone correction 0.05 0.05

total u02 0.85 0.90

18 20 22 24 26 28 30 32 34 36-2.0

-1.5

-1.0

-0.5

0.0

0.5

1.0

1.5

2.0

(0,7)

(0,6)

(0,5)

106 x

(u2 0 -

<u2 0>

) / <

u2 0>

frequency / kHz

(0,4)

concatenate fit

± 0.39 ppm

mode by mode fit

± 0.65 ppm

100 200 300 400 500 600 700-1.0

-0.5

0.0

0.5

1.0

1.5 (0,4) (0,5) (0,6) (0,7)

fit re

sidu

als

/ m2 s

-2

p / kPa

Page 7: Gavioso INRiM molar gas constant R rev - BIPM · estimate of the molar mass flowing 100 sccm est. outgassing rate 1.4 x 10-11 mol m−2 s−1 • we have a direct measurement of pressure

estimate of the molar mass

flowing 100 sccm

est. outgassing rate 1.4 x 10-11 mol m−2 s−1

• we have a direct measurement of pressure from the cavity by a dedicated duct• we continuosly flow at 100 sccm during measurements• we evaluate the rate of outgassing and its influence on our measurements by stopping the flow• we carefully sample just before entering the cavity and analyse by mass spectroscopy

uncertainty budget for molar mass to heat capacity ratio

source u / g mol‐1 ur / ppm

impurities in He 0.000 0013 0.32

possible variation 3He/4He isotopic composition 0.000 0007 0.17

maximum effect water vapor degassing if H2O or N2 0.000 0003 0.07

total M /  0.000 0015 0.37

Page 8: Gavioso INRiM molar gas constant R rev - BIPM · estimate of the molar mass flowing 100 sccm est. outgassing rate 1.4 x 10-11 mol m−2 s−1 • we have a direct measurement of pressure

temperature

± 140 K

cSPRTs

• we used three capsule-type cSPRTs calibrated before and after the measurements

QuantityEstimate

orrel. correction

u(T) / mK

ur(T) / ppm

Thermal gradients 0.084 0.31TTPW 273.1600 K 0.020 0.07

Immersion 0.17 mK 0.007 0.03Repeatability within calibration sequence 0.070 0.26

Self heating ‐ calibration 2.5 mK 0.006 0.02Short‐term repeatability 0.010 0.04

Self heating ‐measurement 2.4 mK 0.006 0.02Long term stability (correction) − 0.13 × 10‐6 0.030 0.11

Systematics R25/R100 bridges (correction) 0.31 × 10‐6 0.025 0.09Total (quadrature sum) TExp 273.160 05 K 0.115 0.42

Page 9: Gavioso INRiM molar gas constant R rev - BIPM · estimate of the molar mass flowing 100 sccm est. outgassing rate 1.4 x 10-11 mol m−2 s−1 • we have a direct measurement of pressure

• the present values of R and k are 1.47 parts in 106 larger than the corresponding 2010 CODATA values

Quantity Estimate ur / ppm

u02 (945 710.45 ± 0.85) m-2 s-2 0.90

M (4.002 6032 ± 0.000 0015) × 10-3 kg mol-1 0.37

T (273.160 05 ± 0.000 12) K 0.42

R (8.314 4743 ± 0.000 0088) J mol-1 K-1 1.06

k = R / NA (1.380 6508 ± 0.000 0015) × 10-23 J K-1 1.06

summarized budget of the uncertainty contributions to the determinations of R and k

Page 10: Gavioso INRiM molar gas constant R rev - BIPM · estimate of the molar mass flowing 100 sccm est. outgassing rate 1.4 x 10-11 mol m−2 s−1 • we have a direct measurement of pressure

8.31440 8.31445 8.31450 8.31455

NIST-88

CODATA-06

LNE-09

NPL-10

INRiM-10

LNE-11

NIM-11

CODATA-10

NPL-13

NIM-13

LNE-15

this work

R / J mol-1 K-1

1.380632 1.380640 1.380648 1.380656 1.380664

NIM-11

INRiM-10

NIM-13

NPL-10

LNE-09

NIST-88

CODATA-06

LNE-11

this work

LNE-15

NPL-13

CODATA-10

1023 x k / J K-1

(Left panel) values of the molar gas constant R determined by AGT in chronologicalorder from top to bottom. (Right panel) corresponding values of the Boltzmann constantk in order of decreasing uncertainty from top to bottom. CODATA 2006 andCODATA2010 re-adjusted values are marked with a distinctive symbol.

comparison with previous determinations of R and k