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Proton-to-electron mass ratio

 
Wikipedia: Proton-to-electron mass ratio

In physics, the proton-to-electron mass ratio, μ or β, is simply the rest mass of the proton divided by that of the electron. Because this ratio is a dimensionless quantity, its numerical value is the same in all systems of units, namely:

\ 1836.1526724718(80).[1]

The number enclosed in parentheses is the standard error. μ is known to a little better than 1 part in 5 billion.

Contents

Discussion

μ is a fundamental physical constant because:

\alpha_s=-\frac{2\pi}{\beta_0 \ln(E/\Lambda_{QCD})}
where β0 = -11 + 2n/3, with n being the number of quark flavors.

Does μ vary over time?

Astrophysicists have tried to find evidence that \ \mu has changed over the history of the universe. (The same question has also been asked of the fine structure constant.) One interesting cause of such change would be change over time in the strength of the strong force.

Astronomical searches for time-varying \ \mu have typically examined the Lyman and Werner transitions of molecular hydrogen which, given a sufficiently large redshift, occur in the optical region and so can be observed with ground-based spectrographs.

If \ \mu were to change, then the change in the wavelength \ \lambda_i of each rest frame wavelength can be parameterised as:

\ \lambda_i=\lambda_0[1+K_i(\Delta\mu/\mu)],

where \ \Delta\mu/\mu is the proportional change in \ \mu, and \ K_i is a constant which must be calculated within a theoretical (or semi-empirical) framework.

Reinhold et al. (2006) reported a potential 4 standard deviation variation in \ \mu by analysing the molecular hydrogen absorption spectra of quasars Q0405-443 and Q0347-373. They found that \ \Delta\mu/\mu = (2.4 \pm 0.6) \times 10^{-5}. King et al. (2008) reanalysed the spectral data of Reinhold et al. and collected new data on another quasar, Q0528-250. They estimated that \Delta\mu/\mu = (2.6 \pm 3.0) \times 10^{-6}, which is inconsistent with the estimates of Reinhold et al. (2006) and implies that \ \mu does not change over time.

Murphy et al. (2008) used the inversion transition of ammonia to conclude that | \Delta\mu/\mu |< 1.8 \times 10^{-6} at z=0.68.

Note that any comparison between values of Δμ / μ at substantially different redshifts will need a particular model to govern the evolution of Δμ / μ. That is, results consistent with zero change at low redshifts do not rule out significant change at high redshifts.

See also

Footnotes

References


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Wikipedia. This article is licensed under the Creative Commons Attribution/Share-Alike License. It uses material from the Wikipedia article "Proton-to-electron mass ratio" Read more