Radiation Pressure Measurement for Small Mass and Force Standard Using Voltage Balance Apparatus Developed at NMIJ

Author(s):  
Kazuaki Fujita ◽  
Yasuyuki Yamamoto ◽  
Kenichi Fujii
2020 ◽  
Vol 10 (1) ◽  
Author(s):  
Mikko Partanen ◽  
Hyeonwoo Lee ◽  
Kyunghwan Oh

AbstractIn contrast to current efforts to quantify the radiation pressure of light using nano-micromechanical resonators in cryogenic conditions, we proposed and experimentally demonstrated the radiation pressure measurement in ambient conditions by utilizing a macroscopic mechanical longitudinal oscillator with an effective mass of the order of 20 g. The light pressure on a mirror attached to the oscillator was recorded in a Michelson interferometer and results showed, within the experimental accuracy of 3.9%, a good agreement with the harmonic oscillator model without free parameters.


2021 ◽  
Vol 70 ◽  
pp. 1-5
Author(s):  
Kazuaki Fujita ◽  
Kenichi Fujii ◽  
Yasuyuki Yamamoto ◽  
Yuichi Ota ◽  
Naoki Kuramoto
Keyword(s):  

Measurement ◽  
2019 ◽  
Vol 131 ◽  
pp. 109-119 ◽  
Author(s):  
Patrick Pinot ◽  
Zaccaria Silvestri

1977 ◽  
Vol 4 (2) ◽  
pp. 177-191 ◽  
Author(s):  
Georges Michaud

In the absence of turbulence or convection one expects that, in stars, heavy elements would tend to settle gravitationally while light elements would go to the surface. Eddington (1930) however realized that this general tendency could be modified both by the electric field and by differential radiation pressure. In spite of their small mass, electrons do not all float on the surface of stars because an electric field is generated that keeps them from separating from the protons. Instead of settling gravitationally, heavy elements often concentrate on the surface because they absorb relatively much more photons than hydrogen or helium and are dragged to the surface by the radiative flux. Eddington concluded that turbulence was too strong for diffusion to be important in stars since the relation that diffusion predicts between surface abundances and stellar masses did not appear to be realized in most stars.


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