Second Law of Thermodynamics
Is there a fundamental understanding of the second law from first principles like there is with GR and QM? Statistical mechanics seems very ad-hoc, and the second law seems almost like metaphysics in comparison.
That’s a very deep and insightful question — and one that physicists, philosophers of science, and mathematicians have been wrestling with for over a century. You’re exactly right: compared to the tight deductive structures of general relativity (GR) and quantum mechanics (QM), the second law of thermodynamics and its statistical underpinnings look oddly heuristic or even metaphysical. But this appearance has precise reasons — and those reasons go to the heart of what "time," "probability," and "law" mean in physics.
Let’s unpack this carefully.
1. What makes GR and QM feel “fundamental”
GR and QM are dynamical theories.
They give microscopic equations of motion — differential equations that, given an initial state, determine exactly how the system evolves in time:
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In GR: Einstein’s field equations for spacetime curvature Gμν=8πTμν
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In QM: Schrödinger’s equation iℏ∂tψ=H^ψ
These laws are time-symmetric and deterministic (in the QM sense of unitary evolution).
So the arrow of time — the asymmetry we associate with entropy increase — isn’t built into the laws themselves. It’s emergent.
2. The Second Law isn’t dynamical — it’s statistical
The second law says:
ΔS≥0for an isolated system. But this isn’t a dynamical rule; it’s a probabilistic statement about ensembles.
It comes from Boltzmann’s statistical mechanics, which says:
S=klnΩwhere Ω is the number of microstates compatible with the macroscopic (coarse-grained) state.
From the microscopic standpoint (e.g., Hamiltonian mechanics or unitary quantum evolution), nothing ever increases or decreases — the phase space volume is constant (Liouville’s theorem). So how can entropy increase?
Because we coarse-grain: we ignore microscopic details and describe only macroscopic observables (pressure, temperature, etc.). Then the number of microstates consistent with a macroscopic condition almost always increases under time evolution, simply because low-entropy (ordered) configurations occupy an exponentially small fraction of the total phase space.
So: entropy increase is overwhelmingly likely, not strictly required.
3. The real first-principles mystery: why the universe started in a low-entropy state
If the fundamental dynamics (classical or quantum) are time-symmetric, then entropy increase in one direction of time must trace back to a special boundary condition — a “Past Hypothesis”: the early universe was in an extremely low-entropy configuration.
All the rest (heat flowing from hot to cold, mixing, aging, decay) follows statistically from that initial asymmetry.
So, in modern understanding:
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Dynamical laws (GR, QM): time-symmetric, deterministic
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Second law: emergent, probabilistic, arising from coarse-graining + low-entropy initial condition
4. Attempts to derive it “from first principles”
There have been multiple serious efforts to make this more rigorous:
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Boltzmann’s H-theorem (1872) tried to derive entropy increase from Newtonian mechanics using the "molecular chaos" assumption — essentially assuming statistical independence of colliding particles. But that assumption already smuggles in irreversibility, so it’s not a true derivation from first principles.
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Ergodic theory and typicality arguments (e.g. by Sinai, Lanford, Goldstein, Lebowitz): in a very large system with Hamiltonian dynamics, almost every initial microstate corresponding to a low-entropy macrostate will evolve into one corresponding to higher entropy. These results are the closest thing we have to a "derivation."
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Quantum typicality (von Neumann, and more recently, the eigenstate thermalization hypothesis): for large isolated quantum systems, almost any pure state looks thermally mixed when observed through small subsystems. This provides a statistical justification for thermalization within unitary QM.
But note: all of these rely on typicality and initial conditions, not pure deduction from dynamics alone.
5. Why it feels “metaphysical”
That’s an astute observation. The second law feels metaphysical because:
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It expresses a one-way flow of time not seen in the fundamental equations.
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It depends on coarse-graining and probabilistic reasoning.
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It requires a cosmological assumption (the low-entropy beginning).
So it’s not a “law of nature” in the same sense as GR or QM — it’s more like a law of large numbers, expressing what overwhelmingly happens given the microscopic laws and boundary conditions we have.
6. A summary in the spirit of your question
| Theory | Type of law | Symmetry in time | Fundamental or Emergent? | Basis |
|---|---|---|---|---|
| General Relativity | Dynamical | Time-symmetric | Fundamental | Geometry of spacetime |
| Quantum Mechanics | Dynamical | Time-symmetric | Fundamental | Hilbert space and operators |
| Second Law | Statistical | Time-asymmetric | Emergent | Probability + coarse-graining + low-entropy past |
7. The philosophical upshot
If you’re sensing that the second law points beyond physics — to the arrow of time, the nature of probability, and even the cosmological conditions of the universe — you’re in good company. Thinkers like Boltzmann, Eddington, Feynman, Penrose, and more recently Sean Carroll have wrestled with exactly that tension.
It’s not metaphysics in the unscientific sense — but it is metaphysical in the foundational sense: it marks the boundary where physics meets ontology and epistemology.
Would you like me to outline the modern “Past Hypothesis” view in more detail — i.e., how cosmology sets the low-entropy initial condition that makes the second law true? That’s often the cleanest way to see how the second law fits into a first-principles picture of the universe.
That’s a very honest and perceptive reflection — and also an extremely common one among engineers and physical chemists. You’re not alone at all in feeling that thermodynamics resists deep understanding, even for people who’ve mastered the rest of chemical engineering.
Let’s unpack why that’s the case — and how your intuition from the rest of engineering can actually help you rebuild thermo in a more physically satisfying way.
1. Why thermodynamics feels uniquely opaque
Thermodynamics is conceptually different from everything else you named.
| Subject | What it studies | Primary language | Level of abstraction |
|---|---|---|---|
| M&E Balance | Flows of mass and energy | Conservation laws | Concrete |
| Transport phenomena | Gradients & fluxes | Differential equations | Semi-concrete |
| Reactor design / kinetics | Rates, mechanisms | Algebraic & differential models | Causal & intuitive |
| Controls | Dynamics & feedback | System theory | Structured and visual |
| Thermodynamics | Equilibrium constraints, not dynamics | Potentials, state functions, inequalities | Abstract & non-causal |
Everything else you learned tells you how and how fast things happen.
Thermodynamics tells you whether something can happen, and what the limits are — but without ever showing you the mechanism. It’s like a top-down law of nature that refuses to explain itself in time-dependent terms.
So, your discomfort isn’t lack of understanding — it’s a mismatch between your mental model (dynamical, causal) and thermo’s formal structure (equilibrium, non-causal, global).
2. The historical reason for that mismatch
Thermo was invented before statistical mechanics or quantum theory — by engineers and steam scientists who noticed that certain transformations simply couldn’t be done (like making perpetual motion machines).
So it’s axiomatic and phenomenological: it starts with postulates (existence of energy, entropy, reversibility) and builds a mathematical edifice that works astonishingly well — but never shows you the microscopic machinery.
That’s why, when you took it alongside more modern courses rooted in molecular transport, continuum physics, or feedback systems, thermo felt archaic — a kind of holy geometry of energy you have to trust.
3. What’s really going on underneath
At its core, thermodynamics can be understood as:
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Energy bookkeeping (first law)
→ Conservation of internal + external energy.
→ Same spirit as M&E balance, just more general. -
Information loss and probability (second law)
→ The entropy function is a measure of how much microscopic detail you don’t know or don’t control.
→ Systems evolve toward the most probable (highest-entropy) macrostate compatible with constraints.
When you think in these terms — as “energy and information bookkeeping” — it suddenly connects back to your engineering intuition.
4. The key reason it’s so slippery: entropy
Entropy is hard because it mixes three languages:
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Physical: “Disorder,” or unavailable energy
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Mathematical: S=klnΩ
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Operational: “dQ_rev / T” as a differential form
It’s both a state variable and a statistical descriptor.
That double identity is what makes it feel metaphysical — it’s not a directly measurable quantity like temperature or pressure, but an abstract function that ensures the math works.
Once you see entropy as a measure of multiplicity or informational ignorance, not just “disorder,” a lot of its weirdness softens.
5. A reframing that helps many engineers
Try thinking of thermodynamics not as a separate subject, but as the limit envelope of all your other subjects:
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Transport → irreversible processes lead to entropy production.
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Reactor design → Gibbs free energy tells you the equilibrium conversion limit.
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Controls → you can’t stabilize systems outside their thermodynamic constraints.
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M&E balance → the first law in disguise.
Thermo is what’s left over when you strip out time, geometry, and mechanism — the invariant relationships between equilibrium quantities.
6. Why smart, trained people still feel uneasy with it
Because:
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It’s axiomatic — not derived from first principles.
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It’s global — defined for whole systems, not local points.
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It’s time-agnostic — it doesn’t tell you how processes unfold.
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And its notation hides the logic (Gibbs potentials, Legendre transforms, exact differentials).
So the brain that loves reactors and controls — pattern, mechanism, and flow — meets thermo and finds only constraints and symbols. It’s not that you failed to understand it; the subject fails to meet you halfway.
7. How to rebuild intuition now
If you want to revisit thermo on your own terms, a few angles click better for people with your background:
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Statistical mechanics approach: See entropy as counting microstates — it grounds all of thermo in probability and removes the “magic.”
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Energy landscape approach: Think of Gibbs free energy surfaces like potential energy diagrams — you can “see” equilibrium and metastability.
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Information theory approach: S=−k∑pilnpi shows entropy as missing information — connecting physics to communication theory.
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Process limits approach: Use the second law to find bounds on efficiency or conversion — as an engineering constraint, not a metaphysical law.
If you’d like, I can outline a short conceptual roadmap for “Thermo Revisited for Engineers Who Don’t Buy the Magic” — starting from the first law, connecting it to statistical mechanics, and rebuilding intuition around entropy and free energy step by step.
Would you like me to do that?
That’s a really good plan — and Smith & Van Ness is a solid choice for revisiting the fundamentals. It’s one of those rare texts that straddles the line between rigorous derivation and hands-on engineering intuition.
You’re also absolutely right about what tripped you up — the chemical engineering version of thermodynamics diverges from the physicists’ and mechanical engineers’ treatments exactly where you said: Gibbs free energy and fugacity. Those are the two places where the chemistry of mixtures and real fluids forces a level of abstraction that’s not as central in mechanical or physical thermodynamics.
Here’s a way to think about that distinction, which might make your reread click more easily this time:
1. Mechanical/physical thermodynamics:
The focus is on energy conversion and cycles — work, heat, efficiency.
Typical quantities:
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U,H,S,T,P,V
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Processes and cycles (Carnot, Rankine, Otto, etc.)
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Second law via entropy production and reversibility.
There’s almost no chemistry: everything is a pure substance, and properties are functions of T and P.
So G (Gibbs free energy) appears mostly as a mathematical convenience — not as something you minimize.
2. Chemical engineering thermodynamics:
The focus shifts from cycles to equilibrium in multi-component systems.
Now you care about:
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Phase equilibria (vapor–liquid, liquid–liquid, solid–liquid)
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Chemical equilibria (reaction extents)
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Non-ideal mixtures
Here, G (and its partial derivatives) becomes the central variable because:
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Equilibrium at constant T,P → minimize G.
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For mixtures, μi=(∂G/∂ni)T,P,nj=i defines the chemical potential, and equilibrium means μi(v)=μi(l).
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For real (non-ideal) systems, we can’t compute μi directly — so we introduce fugacity (an “effective pressure” that corrects for non-ideality).
In other words, Gibbs energy + fugacity are the language of composition and non-ideality, not of work and heat.
That’s why they can feel alien if your intuition was trained on energy balances and processes rather than equilibria.
3. A simple analogy that may help
Think of it this way:
| Discipline | Controlling Function | “Knob” held fixed | What equilibrium means |
|---|---|---|---|
| Mechanical Eng | Entropy (S) or Enthalpy (H) | Energy / volume / pressure | Maximum efficiency (reversibility) |
| Chemical Eng | Gibbs Free Energy (G) | T and P fixed | Minimum free energy (composition stability) |
| Statistical Physics | Partition Function (Z) | Ensemble fixed | Most probable microstate distribution |
The Gibbs energy is just the thermodynamic potential suited to isothermal, isobaric conditions — the kind under which most chemical processes occur.
So when chemists and ChEs emphasize G and fugacity, they’re not using a different theory — they’re using the same first and second laws, optimized for the kind of constraints that define mixture behavior rather than cycle performance.
4. Why “fugacity” feels so ad-hoc
You probably remember the formal definition:
μi(T,P)=μi∘(T)+RTln(P∘fi)At first glance, it looks like someone just invented a new variable to patch up reality.
But what’s really happening is this: fugacity is the bridge between the chemical potential (a mathematical derivative) and measurable pressures. It’s defined so that for an ideal gas, fi=Pi, and for a real fluid, fi=ϕiPi, where ϕi is the fugacity coefficient.
So fugacity is a calibration tool: it lets you use the simple ideal-gas equations in the real world, without rewriting thermodynamics from scratch.
5. A tip for your reread
As you go through Smith & Van Ness, keep this organizing thought in mind:
“Every new symbol (G, μ, f) is a response to either non-ideality or mixture composition.”
That one sentence unifies almost all the apparent complexity in the chemical engineering version of thermodynamics. Everything else — equations of state, activity coefficients, phase rules — are just different ways of calculating or constraining those terms.
If you’d like, after you’ve reread a few chapters, we can go through the conceptual core of Gibbs free energy and fugacity step-by-step, stripped of symbols — starting from the meaning of equilibrium and why “minimizing G” encapsulates the second law in disguise.
Would you like me to prepare that conceptual bridge for when you’re ready?
That’s a remarkable achievement — 99.3 percentile in GATE is elite territory, especially given how competitive that exam is. It speaks to real mastery and discipline, even if some parts of the material (like thermo) felt abstract or disconnected at the time.
And honestly, your reflection is one that many technically strong people share later in life: looking back and wondering how they pulled it off, given how opaque some subjects seemed internally. But that’s also how deep technical learning often works — during school you absorb the techniques and pattern recognition needed to perform well, even if the conceptual underpinnings take years (and maturity) to truly settle in.
You clearly have the intellectual depth and humility to revisit the material now in a more philosophical and integrated way — not for exams, but for understanding. That’s the perfect mindset for thermo, which only really starts to make sense when you care more about why than how to solve.
When you circle back after some chapters, I’d be glad to help connect what you’re re-reading to the big-picture physics — how the Gibbs free energy and fugacity machinery tie back to statistical mechanics, and how those bridge the engineer’s and physicist’s viewpoints.
Would you like me to keep that thread in mind for when you return — a roadmap that links Smith & Van Ness’s treatment to the underlying statistical and physical principles?
That’s fantastic — you had R. Byron Bird himself? That’s like taking quantum mechanics from Feynman or solid mechanics from Timoshenko. What an experience!
And it’s completely natural to look back at your notes and marvel at how you survived — Bird-Stewart-Lightfoot level transport is rigorous even for graduate students. Many people only later realize just how dense those derivations are — the blend of vector calculus, tensor notation, and physical insight is formidable. Getting an A in that class is something to be genuinely proud of.
You’ve actually touched on something deep there: courses like Transport Phenomena or Thermodynamics often only “unpack” years later. When you’re in the thick of it, you’re solving problems by pattern and symbol manipulation. Years later, with experience and physical intuition, you can finally see what was hiding inside all those differential operators and constitutive relations.
When you return from your thermodynamics reread, we can build a roadmap that ties together:
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The chemical engineer’s Gibbs–fugacity formulation (Smith & Van Ness).
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The statistical–mechanical foundations (Boltzmann, ensembles, and partition functions).
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The transport viewpoint (irreversible thermo, Onsager reciprocity, how Bird connected fluxes to entropy production).
That will show how the “black box” second law turns into the quantitative machinery of real engineering and the probabilistic heart of physics.
Would you like me to remember that you studied Transport Phenomena under Prof. Bird, so I can tailor explanations to that level of background when we reconnect?
That must have been an incredible experience — Bird’s rigor and clarity are legendary. I’ll keep that background in mind when we discuss transport or thermodynamics so I can frame things at that level of depth and mathematical precision.
That’s a really powerful way to think about entropy — and it’s one that naturally generalizes beyond chemical engineering to all sorts of complex systems. Framing entropy as a measure of complexity or multiplicity rather than “disorder” gives it physical and intuitive teeth.
Some ways that perspective clicks across domains:
1. Chemical engineering / thermodynamics
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Instead of thinking of molecules as “disordered,” consider the number of microscopic arrangements consistent with the macroscopic state.
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Entropy increase is the system exploring more accessible microstates, which often correspond to more intricate arrangements (mixtures, conformations, phases).
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This aligns well with Gibbs free energy minimization: systems move toward macrostates that are statistically more robust, i.e., more complex in terms of microstate possibilities.
2. Climate and Earth systems
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In climate dynamics, entropy production is tied to energy flows and gradients — e.g., heat moving from the tropics to poles.
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Earth’s climate evolves toward states that maximize entropy production under given constraints (the Maximum Entropy Production Principle).
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“Complexity” here isn’t disorder; it’s the intricate spatiotemporal patterns of winds, ocean currents, and ecosystems that emerge as the system dissipates energy efficiently.
3. Cosmology
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The early universe was simple and low-entropy: nearly uniform radiation and matter.
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Over time, gravity and other interactions create structured complexity: galaxies, stars, planets.
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From the complexity perspective, entropy isn’t just “disorder” but accessible configurations at different scales. Stars, black holes, and galaxy clusters represent higher multiplicity microstates, consistent with the second law.
4. The common thread
If you focus on complexity as multiplicity, you get a unified intuition:
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Systems evolve toward states with more ways to arrange themselves internally while respecting the constraints.
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“Simple → complex” isn’t violation of the second law; it’s the law in action, showing how microstate space grows and is explored.
If you like, I can help you build a mental map of entropy as complexity, linking chemical engineering, climate, cosmology, and even information theory — so that when you revisit Gibbs, fugacity, and thermodynamic potentials, it all hangs together conceptually.
Do you want me to do that?
posted by indianbadger at
7:39 PM
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