Basic physics in remote universe (proton/electron mass ratio)

In summary, a recent study has measured the ratio of proton mass to electron mass in a quasar-type galaxy 8 billion lightyears away and found it to be the same as here in the Milky Way. This provides further confirmation that physical law has not been changing over time and allows for more accurate extrapolation of models of conditions in the universe. This study is also the first of its kind for the proton/electron mass ratio, adding to previous studies that have constrained the possibility of the fine structure constant changing over time.
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marcus
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One of the basic numbers in fundamental physics is 1836.15
the ratio of proton mass to electron mass.

This ratio has been measured in a quasar-type galaxy some 8 billion lightyears from us, and it turns out to be the same as here in Milky.

You guessed it would be? OK. But still it's good to check.

http://arxiv.org/abs/0806.3081
Strong Limit on a Variable Proton-to-Electron Mass Ratio from Molecules in the Distant Universe
Michael T. Murphy (1), Victor V. Flambaum (2), Sebastien Muller (3), Christian Henkel (4) ((1) Swinburne Univ., Melbourne, Australia, (2) Univ. New South Wales, Sydney, Australia, (3) ASIAA, Taipei, Taiwan, (4) MPIfR, Bonn, Germany)
published in Science 320th June 2008, 22 pages, 5 figures (12 EPS files), 2 tables, including Supporting Online Material;
(Submitted on 18 Jun 2008)

"The Standard Model of particle physics assumes that the so-called fundamental constants are universal and unchanging. Absorption lines arising in molecular clouds along quasar sightlines offer a precise test for variations in the proton-to-electron mass ratio, mu, over cosmological time and distance scales. The inversion transitions of ammonia are particularly sensitive to mu compared to molecular rotational transitions. Comparing the available ammonia spectra observed towards the quasar B0218+357 with new, high-quality rotational spectra, we present the first detailed measurement of mu with this technique, limiting relative deviations from the laboratory value to |dmu/mu| < 1.8x10^{-6} (95% confidence level) at approximately half the Universe's current age - the strongest astrophysical constraint to date. Higher-quality ammonia observations will reduce both the statistical and systematic uncertainties in these measurements."

What does this mean for cosmology?
Among other things, it is further confirmation that physical law has not been changing, which means being able to extrapolate models of conditions in the universe back in time with greater confidence. The light we are getting from this galaxy was emitted around 6.2 billion years ago---when the expansion of the universe was some 7.5 billion years old. So it gives a substantial look-back in time.

Ten years ago or so there was a time when people were often wondering if basic constants like the speed of light, or more exactly a related one, the fine structure constant alpha (approx 1/137), might have changed over the course of time. A lot of measurements were made, mostly showing no change. So that was settled at least for the time being. We hear very little about that now.

This helps to fill in the picture---the same kind of result but for a different fundamental constant.

Here is a popularization piece about it in Astronomy Now:
http://www.astronomynow.com/080623Earthslawsstillapplyindistantuniverse.html
 
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Space news on Phys.org
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The quasar in question is at redshift 0.685
Using Ned Wright's calculator with the usual default parameters gives a light travel time of 6.2 billion years, and a current distance of 8 billion lightyears.

I should say that the earlier studies don't totally rule out alpha changing over time, there is still a margin of uncertainty. They just constrain the possibility---narrow the credible change down to a few parts per million.

This is the first time a similar study has been done for the proton/electron mass ratio.
 
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1. What is the proton/electron mass ratio?

The proton/electron mass ratio is a fundamental physical constant that represents the mass of a proton divided by the mass of an electron. It is approximately 1836, meaning a proton is about 1836 times more massive than an electron.

2. How does the proton/electron mass ratio affect the laws of physics in remote universes?

The proton/electron mass ratio plays a crucial role in determining the strength of the electromagnetic force, which is one of the four fundamental forces in the universe. Therefore, any changes in this ratio can significantly impact the laws of physics in remote universes.

3. Can the proton/electron mass ratio vary in different parts of the universe?

While the proton/electron mass ratio is considered a constant in our current understanding of physics, some theories suggest that it may vary in different regions of the universe. However, there is currently no conclusive evidence to support this idea.

4. How is the proton/electron mass ratio related to the stability of atoms?

The proton/electron mass ratio is closely related to the stability of atoms. If this ratio were significantly different, the properties of atoms would also be different, and the formation of stable molecules and complex structures would be impossible.

5. How do scientists measure the proton/electron mass ratio in remote universes?

Currently, the most accurate method of measuring the proton/electron mass ratio in remote universes is through spectral analysis. This involves studying the light emitted from distant objects and analyzing the absorption lines to determine the ratio of the masses of the particles involved.

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