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I was told the gas constant R is "work done per mole per kelvin" — what does that actually mean physically?

Working through isothermal processes and the definition I was given for the universal gas constant was that it is the work done by a gas, per mole, per kelvin. I wrote it down and it has not meant anything to me since.

What I can do is use it. Plug it into the ideal gas law, get the right number. What I cannot do is picture what it is — whether it is a property of gases, a property of the universe, or just a units conversion that fell out of how we defined things.

Can someone give me the physical intuition rather than the formula?

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  • @orbital_ola · 2w ago

    The "work done per mole per kelvin" version you were given is not wrong, it is just a specific case presented as a definition, which is why it did not generalise for you.

    Here is where it comes from. Heat a mole of ideal gas by one kelvin at constant pressure and it expands. Expanding against a constant pressure does work, and if you compute that work it comes out to exactly R joules.

    So the statement is true, and it describes one particular situation — constant pressure, one mole, one kelvin. Your textbook picked it because it appears while deriving the difference between the two heat capacities.

    But R shows up in places with no work and no expansion anywhere: entropy expressions, equilibrium constants, reaction rates, the distribution of molecular speeds. Those are the clue that the deeper meaning is the energy-per-kelvin one, and the work interpretation is a consequence rather than the definition.

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  • @phase_diagram_finn · 2w ago

    The cleanest way in is to look at the smaller constant hiding inside it.

    R is just Boltzmann's constant multiplied by Avogadro's number. Boltzmann's constant is the fundamental one, and what it does is convert temperature into energy. That is its whole job. It says how many joules of molecular kinetic energy correspond to one kelvin, for a single particle.

    R is the same statement scaled up to a mole instead of a particle. So:

    • Boltzmann's constant: energy per kelvin, per molecule.
    • R: energy per kelvin, per mole.

    That reframing answers your "property of gases or of the universe" question directly. It is neither a property of gases nor an accident of units — it is the exchange rate between our temperature scale and energy, and it looks like an arbitrary number only because the kelvin was defined from water long before anyone knew what temperature was made of.

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  • @kiln_kerem · 2w ago

    A number that makes it tangible: R is about 8.3 joules per mole per kelvin.

    So warming a mole of gas by one degree costs you a few joules of the energy that shows up as translational motion. A mole of air is roughly the amount in a two-litre bottle at ordinary conditions. Warm that by a degree and the energy involved is comparable to lifting a small apple a metre.

    Having one concrete anchor like that stops the constant feeling like an abstraction. It is a small number because a degree is a small change and a molecule is a small thing.

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  • @bench_chem_bea · 2w ago · 2 replies

    "It is the exchange rate between the temperature scale and energy" would have saved me two weeks. Every appearance of R in an unrelated formula now looks like the same conversion rather than a coincidence.

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    • @phase_diagram_finn · 2w ago

      That is exactly the right takeaway — once you see it as a conversion factor, the fact that it turns up wherever temperature meets energy stops being surprising and starts being expected.

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