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Proton-to-electron mass ratio

Proton-to-electron mass ratio is a science topic covered in the lgStudy science library. This page brings together a partial reference excerpt, illustrations, worked examples, real-world applications and a short study plan, so you can understand Proton-to-electron mass ratio rather than just read about it. In short: In physics, the proton-to-electron mass ratio (symbol μ or β) is the rest mass of the proton (a baryon found in atoms) divided by that of the electron (a lepton found in atoms), a dimensionless quantity, namely: μ = mp/⁠me = 1836.152673426(32). The number in parentheses is the measurement uncertainty on the last two digits, corresponding to a relative standard uncertainty of 1.7×10−11.

Key takeaways

  • Proton-to-electron mass ratio belongs to science; place it in that map before memorising details.
  • Learn the definition first, then one example that makes the definition concrete.
  • Connect Proton-to-electron mass ratio to a quantity you can measure, compute or draw — that is where exam questions come from.
  • Reproduce the core statement of Proton-to-electron mass ratio from memory before moving on to harder problems.

Reference excerpt

In physics, the proton-to-electron mass ratio (symbol μ or β) is the rest mass of the proton (a baryon found in atoms) divided by that of the electron (a lepton found in atoms), a dimensionless quantity, namely:

μ = mp/⁠me = 1836.152673426(32). The number in parentheses is the measurement uncertainty on the last two digits, corresponding to a relative standard uncertainty of 1.7×10−11.

Discussion μ is an important fundamental physical constant because:

Baryonic matter consists of quarks and particles made from quarks, like protons and neutrons. Free neutrons have a half-life of 613.9 seconds. Electrons and protons appear to be stable, to the best of current knowledge. (Theories of proton decay predict that the proton has a half life on the order of at least 1032 years. To date, there is no experimental evidence of proton decay.); Because they are stable, are components of all normal atoms, and determine their chemical properties, the proton is the most prevalent baryon, while the electron is the most prevalent lepton; The proton mass mp is composed primarily of gluons, and of the quarks (the up quark and down quark) making up the proton. Hence mp, and therefore the ratio μ, are easily measurable consequences of the strong force. In fact, in the chiral limit, mp is proportional to the QCD energy scale, ΛQCD. At a given energy scale, the strong coupling constant αs is related to the QCD scale (and thus μ) as

α s = − 2 π β 0 ln ⁡ ( E / Λ Q C D ) {\displaystyle \alpha _{s}=-{\frac {2\pi }{\beta _{0}\ln(E/\Lambda _{\rm {QCD}})}}}

where β0 = −11 + 2n/3, with n being the number of flavors of quarks.

Variation of μ over time

Astrophysicists have tried to find evidence that μ 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 μ have typically examined the Lyman series 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 μ were to change, then the change in the wavelength λi of each rest frame wavelength can be parameterised as:

λ i = λ 0 [ 1 + K i Δ μ μ ] , {\displaystyle \ \lambda _{i}=\lambda _{0}\left[1+K_{i}{\frac {\Delta \mu }{\mu }}\right],}

where Δμ/μ is the proportional change in μ and Ki 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 μ by analysing the molecular hydrogen absorption spectra of quasars Q0405-443 and Q0347-373. They found that Δμ/μ = (2.4 ± 0.6)×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 Δμ/μ = (2.6 ± 3.0)×10−6, different from the estimates of Reinhold et al. (2006). Murphy et al. (2008) used the inversion transition of ammonia to conclude that |Δμ/μ| < 1.8×10−6 at redshift z = 0.68. Kanekar (2011) used deeper observations of the inversion transitions of ammonia in the same system at z = 0.68 towards 0218+357 to obtain |Δμ/μ| < 3×10−7. Bagdonaite et al. (2013) used methanol transitions in the spiral lensing galaxy PKS 1830-211 to find ∆μ/μ = (0.0 ± 1.0) × 10−7 at z = 0.89. Kanekar et al. (2015) used near-simultaneous observations of multiple methanol transitions in the same lens, to find ∆μ/μ < 1.1 × 10−7 at z = 0.89. Using three methanol lines with similar frequencies to reduce systematic effects, Kanekar et al. (2015) obtained ∆μ/μ < 4 × 10−7. 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 lower redshifts do not rule out significant change at higher redshifts.

A mathematical coincidence In a famously brief two-sentence paper published in Physical Review in 1951, Friedrich Lenz observed that the best experimental value for the mass ratio at the time (1836.12 ± 0.05) coincided almost perfectly with the mathematical expression 6 π 5 {\displaystyle \pi ^{5}} . This is now believed to be a mathematical coincidence, since modern measurements with higher precision show the values are remarkably close but not identical: μ = m p / m e = 1836.152673426 ( 32 ) {\displaystyle \mu ={m_{p}}/{m_{e}}=1836.152673426(32)} while 6 π 5 ≈ 1836.118109 {\displaystyle 6\pi ^{5}\approx 1836.118109} .

See also Koide formula

Footnotes

… excerpt ends here. Continue reading the full article.

Worked examples

Example 1 — a first encounter with Proton-to-electron mass ratio

Start with the simplest possible case. Write down what Proton-to-electron mass ratio claims or describes in one sentence, then invent the smallest concrete situation in which that sentence is true. In science, the smallest case is usually a single object, a single equation or a single measurement. Check that every symbol or term in your sentence has a meaning in that case.

Example 2 — changing one variable

Take the situation from Example 1 and change exactly one quantity: double it, halve it, or set it to zero. Predict what should happen to Proton-to-electron mass ratio before you calculate. Comparing your prediction with the result is the fastest way to find out whether you understand the idea or only the words.

Example 3 — an exam-style question

Typical questions about Proton-to-electron mass ratio ask you to (a) state it precisely, (b) apply it to given data, and (c) explain a limitation. Practise writing all three answers in under five minutes; the third part is what separates a full-mark answer from an average one.

Applications of Proton-to-electron mass ratio

In research
Proton-to-electron mass ratio appears in science research whenever the underlying quantities have to be modelled precisely. Papers usually cite it as a starting assumption and then explore where it breaks down.
In technology and industry
Engineering practice reuses Proton-to-electron mass ratio in design rules, simulations and safety margins. Knowing the idea lets you read a specification sheet and understand why the numbers look the way they do.
In the classroom
Proton-to-electron mass ratio is common in secondary-school and first-year university syllabi. It links to neighbouring topics Dimensionless constants, Electron, Fundamental constants, so understanding it makes those chapters shorter.
In everyday life
Look for Proton-to-electron mass ratio outside the textbook — in sport, cooking, traffic, electronics or the sky above you. An example you found yourself is remembered far longer than one you were given.
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How to study Proton-to-electron mass ratio in 20 minutes

  1. Read the reference excerpt below once, without taking notes.
  2. Close the page and write down what Proton-to-electron mass ratio means in your own words.
  3. Compare your version with the excerpt and mark what you missed.
  4. Work through the three examples above with pen and paper.
  5. Explain Proton-to-electron mass ratio out loud to somebody else — or to Teacher Smith in the lgStudy chat.

Frequently asked questions

What is Proton-to-electron mass ratio in simple terms?

In physics, the proton-to-electron mass ratio (symbol μ or β) is the rest mass of the proton (a baryon found in atoms) divided by that of the electron (a lepton found in atoms), a dimensionless quantity, namely: μ = mp/⁠me = 1836.152673426(32). The number in parentheses is the measurement uncertain…

Why does Proton-to-electron mass ratio matter?

Because it connects several science ideas at once: it gives you a definition you can apply, a quantity you can calculate, and a way to check whether a result is plausible.

How should I study Proton-to-electron mass ratio?

Read the excerpt, restate it from memory, then work through the examples and applications listed on this page. The five-step study plan above takes about twenty minutes.

What does this page cover?

It gives you a compact reference excerpt plus original lgStudy explanations, examples, applications and study material on Proton-to-electron mass ratio.

Tags

  • Dimensionless constants
  • Electron
  • Fundamental constants
  • Proton

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