Primer: Erik Verlinde, "On the Origin of Gravity and the Laws of Newton" (2010)
Study document for the Verlinde-Erik project. The project folder holds one document: E. Verlinde, "On the Origin of Gravity and the Laws of Newton", arXiv:1001.0785v1 (6 Jan 2010), 29 pages, later published in JHEP 04 (2011) 029 (JHEP is the Journal of High Energy Physics) [read: p.1; web via Investigator, INSPIRE]. Verdicts come from arbiter.md, including its Section 10 "QE revision". This primer adds no new verdicts.
Source tags: [read: p.N] = the paper's page N; [deep] = the deep read of the paper (Step 1b, pp.12-22, equations checked against page images of pp.14-21; QE remediation, pp.4-11 checked against page images of pp.5 and 7-10, and pp.22-27 with page images of pp.24-27); [calc] = a calculation done for this primer and reproduced in example.py; [calc by deep read] = a calculation by the QE-remediation deep reader, also reproduced in example.py Part F; [web] = an Internet source with URL (mostly abstracts read by the Investigator, reviewers or arbiter, not full papers); [memory] = recalled from training, with confidence.
Source gap: none. The full paper was read from its text layer. Everything said here about later work (2016 successor model, galaxy tests, fluctuation experiments) rests on web abstracts, not on full papers.
Author. Erik Verlinde is a professional string theorist at the University of Amsterdam [read: p.1], and the paper appeared in a mainstream journal. This is not an outsider's project: it is a mainstream physicist's unorthodox interpretation. It won attention, a large Dutch research prize (the NWO Spinoza Prize, 2011) and a continuing programme of follow-up work [web via Investigator: ScienceGuide; INSPIRE].
1. The idea in one paragraph
A stretched rubber band pulls back, but no single molecule in it carries a "rubber-band force". The pull happens because there are far more tangled arrangements of the molecules than straight ones, and random thermal jiggling pushes the band toward the tangled, high-entropy state. Physicists call this an entropic force. Verlinde proposes that gravity works the same way. He imagines that the information about where matter sits is stored as "bits" on closed surfaces in space, which he calls holographic screens. The number of bits is proportional to the screen's area, and the screen has a temperature. When a mass moves toward a screen, the information content (entropy) changes, and a force appears, just as with the rubber band. With a few assumptions, which he states openly, this reproduces Newton's second law F = ma, Newton's law of gravitation and, in outline, Einstein's equations. The paper does not predict any number that differs from Newton or Einstein. Its contribution is a new interpretation and a research programme. The author admits the logic partly runs backwards from known results.
2. What you need to know first
Entropy and temperature (statistical mechanics). Entropy S = k_B ln(Omega), where Omega is the number of microscopic arrangements (microstates) consistent with what you see at large scale, and k_B = 1.380649e-23 J/K is Boltzmann's constant. Temperature is defined by 1/T = dS/dE: how much the entropy rises when you add energy E. A system left alone drifts toward the macrostate with the most microstates. Read: D. V. Schroeder, An Introduction to Thermal Physics (the early chapters on the second law and on entropy and temperature).
Equipartition. In a classical system in equilibrium, each independent quadratic degree of freedom (for example each (1/2) m v_x^2 term) holds an average energy (1/2) k_B T. Verlinde applies this to his screen bits: E = (1/2) N k_B T. Note that equipartition is a theorem for classical systems with quadratic energies. It fails for quantum systems at low temperature, which is why the heat capacity of solids drops at low T. Read: Schroeder, the section on equipartition in chapter 1.
Entropic forces. If the entropy depends on a position x, a system at temperature T feels an effective force F = T dS/dx. It points toward higher entropy and is proportional to T. The textbook example is an ideal polymer chain (Section 3.1 below). Read: P. Nelson, Biological Physics (the chapters on entropic forces and on polymer elasticity); Schroeder for the general free-energy argument.
Gauss's law and the Poisson equation. For gravity, the flux of the field g through any closed surface is -4 pi G times the mass inside. In differential form this is the Poisson equation, laplacian(Phi) = 4 pi G rho, where Phi is the gravitational potential and rho the mass density. This is the same mathematics as electrostatics with a sign change, because masses attract. Read: D. J. Griffiths, Introduction to Electrodynamics, chapter 2 (electrostatics: Gauss's law, divergence theorem, Poisson equation).
Black-hole thermodynamics and the Unruh effect. These are quantum-gravity results that the paper leans on. They are not in the reader-profile background, so Section 3 introduces them from scratch. Read: L. Susskind and J. Lindesay, An Introduction to Black Holes, Information and the String Theory Revolution: The Holographic Universe (short, aimed at advanced undergraduates); J. B. Hartle, Gravity: An Introduction to Einstein's General Relativity (for the general-relativity part).
General relativity, very briefly. In Einstein's theory gravity is the curvature of spacetime. Clocks run slower lower in a gravitational well, so light climbing out loses energy (gravitational redshift). The Einstein equations relate curvature, a matrix-like object called a tensor, to the energy and momentum of matter. You need only the idea for this primer, not the tensor calculus. Read: Hartle, the early chapters on gravity as geometry and on the Schwarzschild geometry.
3. The textbook view
3.1 Entropic force in a polymer (real, measured physics)
Model a polymer as a chain of n links of length b that point in random directions (a "freely jointed chain"). Every arrangement has the same energy. If the two ends are held a distance x apart, the number of arrangements falls as x grows. For x much smaller than n b, the entropy is approximately
S(x) = S_0 - (3 k_B x^2) / (2 n b^2)
so the entropic force is
F = T dS/dx = -(3 k_B T / (n b^2)) x
This is Hooke's law. The spring constant comes entirely from entropy and grows with temperature [memory: high; standard ideal-chain result]. Rubber really does get stiffer when heated, which is the experimental signature. Verlinde's Section 2 describes exactly this example: "An entropic force is recognized by the facts that it points in the direction of increasing entropy, and, secondly, that it is proportional to the temperature" [read: p.5]. He also notes that such a force "can be conservative, at least when the temperature is kept constant" [read: p.5]. That caveat matters later.
Symbols: S entropy, S_0 entropy at x = 0, k_B Boltzmann's constant, T temperature, n number of links, b link length, x end-to-end distance, F force.
3.2 The Unruh temperature
In 1976 W. G. Unruh showed that, in quantum field theory, an observer with constant acceleration a through empty space detects thermal radiation at temperature
k_B T = hbar a / (2 pi c)
where hbar = 1.054571817e-34 J s is the reduced Planck constant and c = 2.998e8 m/s is the speed of light [memory: high]. For a = 9.8 m/s^2, T = 4.0e-20 K [calc]. This is far too small to measure directly, and the Unruh effect has not been observed directly [memory: high; the arbiter notes this was not re-checked against recent claims]. Verlinde uses this formula as eq. (3.8), but says it should be read the other way round: as "the temperature T that is required to cause an acceleration equal to a" [read: p.8].
3.3 Black-hole entropy, Hawking temperature and the holographic principle
A non-rotating black hole of mass M has a horizon at the Schwarzschild radius R_s = 2GM/c^2, where G = 6.674e-11 m^3 kg^-1 s^-2 is Newton's constant. Bekenstein (1972) argued, and Hawking (1974-75) confirmed, that a black hole has entropy proportional to its horizon area A [memory: high]:
S_BH = k_B c^3 A / (4 G hbar)
and temperature
T_H = hbar c^3 / (8 pi G M k_B).
The combination G hbar / c^3 = l_P^2 is the square of the Planck length (l_P = 1.6e-35 m). So S_BH is k_B times one quarter of the area measured in Planck-length squares.
A useful check, done in example.py Part E: Hawking's temperature equals the Unruh formula with a = GM/R_s^2, the Newtonian surface gravity at the horizon. For one solar mass both give 6.17e-8 K [calc]. This coincidence is one of the clues that inspired thermodynamic views of gravity.
Bekenstein's thought experiment [memory: high; summarised in the paper, read: p.6]: lower a particle of mass m on a string toward a black hole. When it is within about one Compton wavelength (hbar/(mc)) of the horizon, count it as absorbed. The horizon area grows by an amount that corresponds to about one bit of entropy. Verlinde's starting postulate copies this step away from black holes.
The holographic principle ('t Hooft 1993, Susskind 1995) [memory: high]: the maximum information that can be stored in a region scales with the area of its boundary, not with its volume, at roughly one bit per Planck area. In the AdS/CFT correspondence (Maldacena 1997) this becomes precise. AdS/CFT (anti-de Sitter / conformal field theory) is a mathematical equivalence in string theory: a gravity theory in a negatively curved space ("anti-de Sitter") is exactly equivalent to an ordinary quantum theory without gravity living on its boundary. In that setting the extra spatial direction and gravity "emerge" from the boundary theory. This is established mathematics for that negatively curved setting. It has not been shown for our universe [memory: high; arbiter claim 5].
The Bekenstein bound [memory: high]: an object of energy E inside a sphere of radius R can hold at most S <= 2 pi k_B R E / (hbar c). A black hole saturates it. The paper writes the bound as "an entropy larger than ER" [read: p.27]. That is shorthand in "natural units", where hbar = c = k_B = 1, and it also drops the 2 pi. Taken literally, the shorthand would be violated by a factor 2 pi even by a black hole at its own horizon, so this primer uses the SI form with the 2 pi, as the reviewers did [deep; memory: high].
3.4 Newtonian gravity
Newton's law of gravitation and Gauss's law:
F = G M m / r^2, g = -grad(Phi), laplacian(Phi) = 4 pi G rho, closed-surface integral of grad(Phi) . dA = 4 pi G M_enclosed.
Phi is the gravitational potential (J/kg), g the gravitational acceleration, rho the mass density. Here G is a measured constant, known only to about 2 parts in 10^5 [memory: high].
3.5 Jacobson 1995: Einstein's equations as an equation of state
T. Jacobson took the relation between heat and entropy, delta Q = T dS, with T the Unruh temperature and S proportional to area. He assumed it holds for every small local "horizon" through every point of spacetime. From this he derived Einstein's field equations [web] https://arxiv.org/abs/gr-qc/9504004. His reading is that the Einstein equations may be like the equation of state of a gas: a large-scale law over unknown microscopic constituents. This is the respectable core of "thermodynamic gravity". Verlinde cites it as ref. [7] and adapts it [read: p.20, p.28]. T. Padmanabhan developed related ideas [read: ref. 14, p.29].
4. Where Verlinde departs
Verlinde does not change any equation of Newton or Einstein. He changes what they mean, and he moves a few quantities from "output" to "input". Side by side:
| Step | Textbook | Verlinde 2010 |
|---|---|---|
| Nature of gravity | Fundamental interaction (Newton: force; GR: curvature) | An entropic force like polymer elasticity: F Delta x = T Delta S (3.7) [read: p.7] |
| Entropy near a surface | Bekenstein: one bit when a particle is a Compton wavelength from a black-hole horizon | Postulate for any screen, anywhere: Delta S = 2 pi k_B (mc/hbar) Delta x (3.6) [read: p.7]. "The reason for putting in the factor of 2 pi will become apparent soon." It "is picked precisely in such a way that one recovers the second law of Newton" [read: p.7-8] |
| Temperature | Unruh: an accelerating observer sees T | The same formula (3.8), read as "the temperature required to cause an acceleration" [read: p.8]. Then "forget about the Unruh law (3.8), since we don't need it" [read: p.8], but the same form is used again for T in (4.17) and (5.28) [deep] |
| Information count | Holographic principle: a maximum bit count proportional to area, for horizons | Every closed screen carries N = A c^3/(G hbar) bits (3.10). "One can simply regard this equation as the definition of G" [read: p.8] |
| Energy on the screen | Equipartition holds for free classical systems | E = (1/2) N k_B T on the screen (3.11), and E = Mc^2 (3.12) [read: p.8-9]. "Perhaps the least obvious assumption is equipartition, which in general holds only for free systems" [read: p.10]. His defence, on the same page: "When the lost bits are randomly chosen among all bits, one expects the energy change associated with Delta S still to be proportional to the energy per unit area E/A. This fact could therefore be true even when equipartition is not strictly obeyed" [read: page image p.10]. It is a plausibility argument ("one expects", "could"); no distribution function or calculation is given [deep] |
| Newton's potential Phi | Solves Poisson's equation | A "coarse-graining" variable: it "keeps track of the depletion of the entropy per bit" (3.16) [read: p.11]. Screens are put on surfaces of constant Phi [read: p.12] |
| Einstein equations | Postulated (or derived from a least-action principle) | A "sketch" of a Jacobson-type argument applied to time-like screens through the Komar mass [read: p.20] |
| Space itself | A background arena (Newton) or a dynamical geometry (GR) | Emergent from information on screens, as in AdS/CFT [read: p.6, p.12] |
| Near a black-hole horizon (Section 6.3) | First law of black-hole thermodynamics, T_H dS_BH = c^2 dM: a consistency relation | The same relation read as F_gravity = T_H dS_BH/dx (6.40), called "perhaps the clearest argument for the fact that gravity is an entropic force"; the screen is then moved off the horizon [read: p.25-26] |
The author's own disclosure, which every reader should keep beside the derivation [read: p.9]:
"These equations do not just come out by accident. It had to work, partly for dimensional reasons, and also because the laws of Newton have been ingredients in the steps that lead to black hole thermodynamics and the holographic principle. In a sense we have reversed these arguments. But the logic is clearly different, and sheds new light on the origin of gravity: it is an entropic force!"
Author's other caveats, verbatim: the arguments are "admittedly ... rather heuristic" [read: p.22]; hbar "just serves as an auxiliary variable that is needed for dimensional reasons. It can therefore be chosen at will" [read: p.10]; the role of hbar is "subtle and not yet fully understood" [read: p.26]; the screen entropy "appears to be very high, and violates the Bekenstein bound" [read: p.27]; screens at equipotentials are "in general not in equilibrium" [read: p.13]. On predictions, he writes: "we need a better understanding of the theory to turn this in to a prediction" [read: p.27].
The relativistic step, in plain words. In Section 5 the screens sit where clocks all run at the same rate (constant redshift). Verlinde adds a redshift factor to the temperature and repeats the bit-counting. The result is a known GR formula: the Komar mass, which is the relativistic version of Gauss's law. He gets it as M = (1/(4 pi G)) times the surface integral of e^phi grad(phi) . dA, eq. (5.34) [read: p.19; deep]. Here phi is the log of the clock-rate factor, and e^phi is how much slower a clock ticks there than at infinity. The reviewers confirmed the algebra and checked that it returns M for a black hole at every radius [deep; calc]. The step from there to the full Einstein equations is one paragraph. The matter side is "presumably" fixed by comparing both sides [read: p.20], and in the standard textbook account that combination is itself obtained by using Einstein's equations [deep; memory: high, Wald].
The author's "clearest argument": black-hole horizons (Section 6.3). This is the one place where the paper's identifications are not free choices. Go back to Bekenstein's thought experiment: a particle of mass m hangs on a string just outside a black hole. Pull it out a little and its energy changes by the work done against gravity. Drop it in and the hole's mass grows by that same energy. The first law of black-hole thermodynamics, T_H dS_BH = c^2 dM, then fixes how much the hole's entropy grows. Putting the two together, Verlinde writes [read: p.25]
F_gravity = T_H dS_BH/dx (6.40)
where dS_BH/dx is "the response of S_BH due to a change in the distance x of the particle to the horizon". He calls this "surely known, and probably just regarded as a consistency check", then takes it "one or two steps further": near the horizon "the equations presented in section 3 are exactly valid", with hbar the actual Planck constant [read: p.25-26]. The same thought experiment for a Rindler horizon (the horizon an accelerating observer has in flat space) is said to give F = ma [read: p.26].
What the QE deep read and example.py Part F show [calc by deep read; standard inputs, memory: high]: - Near the horizon, with l the proper (ruler) distance from it and r_s = 2GM/c^2, the entropy the hole would gain if the particle were dropped from l is Delta S_BH = 2 pi k_B (mc/hbar) l [1 - l^2/(8 r_s^2) + ...]. The leading term is exactly Verlinde's postulate (3.6), with the real hbar. The black-hole mass cancels, so this holds for a hole of any size. - There the temperature of the Hawking radiation seen by the observer holding the string equals the Unruh temperature (3.8) of that observer's acceleration (the ratio is (r/r_s)^2, which is 1 at the horizon). So T dS/dx = ma. The claim that Section 3 is "exactly valid" is correct to leading order in l/r_s. - In fact T_loc d(Delta S_BH)/dl = m a holds exactly at every radius r, where T_loc is the local (Tolman) temperature. This is not new physics. It is the first law plus the fact that a held particle's energy, seen from far away, is m c^2 sqrt(1 - r_s/r). - Caution: dS_BH/dx is a "what-if" derivative (how much entropy the hole would gain if the particle were dropped from x). It is not an entropy that sits in space while the particle hangs there. Away from the horizon the Section 3 forms (3.6) and (3.8) do not follow from (6.40). - The Bekenstein-bound excess of Section 5, Step 8 (a factor R/R_s) falls to exactly 1 at the horizon. So the regime where hbar, T and S are the standard ones is also the regime where the screen entropy is allowed [calc].
The "steps further" are assumptions, not derivations: the screen "can" be moved outward; the force there "can be nothing else then an entropic effect"; the "correspondence rules ... must be such that F = T grad S translates in to the gravitational force" [read: p.26]. No calculation is shown beyond (6.40) [read: p.25-26]. The author concedes on p.26 that "we have no direct confirmation or proof that the same is true when we go away from the horizon", and that "one is not exactly at thermal equilibrium" there. This off-horizon step is exactly what Wang and Braunstein contest (evidence table below, claim 1b).
The string-theory support (Section 6.2), in plain words. In string theory there are open strings (with two loose ends, which can be stuck on a membrane called a D-brane) and closed strings (loops; one of their vibrations is the graviton, the carrier of gravity). A calculation in which open strings on a membrane fluctuate in a quantum loop gives exactly the same number as closed strings, that is gravity, travelling between membranes. A gravity-free theory, summed over its fluctuations, is equivalent to gravity [deep; memory: high that this "open/closed duality" is standard]. Verlinde reads this as gravity being emergent, identifies his screens with the membranes, and says it "supports the interpretation of gravity as an entropic force" [read: p.23-24]. A duality says two descriptions give the same answers. It does not say which one is fundamental, or that the force is entropic, and the paper gives no calculation for that step [deep]. He also suggests that the entropic mechanism "should be applicable" where AdS/CFT is used in condensed-matter physics, where gravity is only an effective description [read: p.23]. No one in the record has pursued that as a test.
5. Worked example: Verlinde's chain at Earth's surface
Run: .venv/bin/python review/Verlinde-Erik/example.py (all checks pass).
Take a spherical screen at Earth's surface. Inputs: M = 5.972e24 kg, R = 6.371e6 m, test mass m = 1 kg, CODATA constants (G, hbar, c, k_B as above).
Step 1. Count the bits (eq. 3.10). Area A = 4 pi R^2 = 5.101e14 m^2. N = A c^3/(G hbar) = 5.101e14 x (2.998e8)^3 / (6.674e-11 x 1.055e-34) = 1.95e84 bits [calc].
Step 2. Share Earth's rest energy over the bits (eqs. 3.11, 3.12). E = Mc^2 = 5.37e41 J. Equipartition E = (1/2) N k_B T gives T = 2E/(N k_B) = 3.98e-20 K [calc]. Each bit holds (1/2) k_B T = 2.7e-43 J.
Step 3. Compare with Unruh. The Unruh formula with a = g = GM/R^2 = 9.820 m/s^2 gives T = hbar g/(2 pi k_B c) = 3.98e-20 K. That is the same number, to every digit [calc]. This is not a coincidence or a test. Insert N into Step 2 and simplify, and you get T = hbar G M/(2 pi k_B c R^2) = hbar g/(2 pi k_B c) identically. The definition of G in (3.10) makes the two agree.
Step 4. Entropy gradient for the 1 kg test mass (eq. 3.6). dS/dx = 2 pi k_B m c/hbar = 2.47e20 J/K per metre, or 1.8e43 k_B per metre [calc].
Step 5. Entropic force (eq. 3.7). F = T dS/dx = 3.98e-20 K x 2.47e20 J/(K m) = 9.820 N. Newton's law gives G M m/R^2 = 9.820 N. Exact agreement [calc].
Step 6. Look at what made it work (symbolic, example.py Part B). Write the chain in symbols:
T = 2 M c^2 / (N k_B) = 2 M c^2 G hbar / (4 pi R^2 c^3 k_B) = G M hbar / (2 pi k_B c R^2) F = T x 2 pi k_B m c / hbar = G M m / R^2.
Three things to notice: - hbar cancels. Replace hbar by any multiple lambda x hbar and F is unchanged; only T changes, by lambda [calc]. The author says the same [read: p.10]. So the quantum constant is a placeholder. The temperature is not a measurable prediction, because it can be rescaled at will. - G cancels against its own definition. G enters only through the bit count N = A c^3/(G hbar), which the paper calls the definition of G [read: p.8]. The calculation therefore cannot predict the value of G or test Newton's law. What it does reproduce is the shape: 1/R^2 because bits scale with area, and F proportional to M and m because energy and entropy add. - The 2 pi was chosen. It sits in (3.6) so that the Unruh 2 pi cancels and F = ma comes out [read: p.8].
Step 7. Move the test mass off the screen (Verlinde eq. 4.22; example.py Part C). Verlinde's general rule is that each bit's entropy shifts by k_B delta Phi/(2c^2), where delta Phi is the change in potential on the screen as the particle moves [deep: eq. 4.22]. For a particle at distance d > R from a spherical screen of radius R, the total entropy change per metre is
dS/dx = (2 pi k_B m c/hbar) x (R/d)^2
[calc; agrees with deep]. The step that does the work is a fact from electrostatics: the average of 1/|r - r_m| over a sphere equals 1/d when the point r_m lies outside it (the mean-value property of harmonic functions). Numerically:
| d/R | entropy rate / (3.6) value | T dS/dx (N) | G M m/d^2 (N) |
|---|---|---|---|
| 1.01 | 0.9803 | 9.6265 | 9.6265 |
| 1.10 | 0.8264 | 8.1157 | 8.1157 |
| 1.50 | 0.4444 | 4.3644 | 4.3644 |
| 2.00 | 0.2500 | 2.4550 | 2.4550 |
Newton's inverse square comes out for every d, and the answer does not depend on the screen radius R. The R^2 in dS/dx cancels the 1/R^2 in T. Verlinde presents this screen independence as support for his coarse-graining picture [read: p.16]. He states it already on p.10: if the screen is moved in to R0 < R, "the number of bits on the screen is multiplied by a factor (R0/R)^2, while the temperature is divided by the same factor. Effectively, this means that only hbar is multiplied by that factor, and since it drops out, the resulting force will stay the same" [read: page image p.10]. (Read literally, the algebra needs hbar divided by that factor, not multiplied; the conclusion that F is unchanged stands [calc by deep read].) Mathematically it is Gauss's law at work [deep].
A side result from the same calculation: if the screen were a flat plane instead of a closed sphere, the same rule would give only half of the 2 pi in (3.6). The derivative of the plane integral is -2 pi, whereas the closed sphere gives -4 pi as d -> R [calc, example.py; first found by the deep read]. So the postulate (3.6) holds only for the whole closed screen, which the paper does not discuss.
Step 8. The Bekenstein bound (paper p.27; example.py Part D). If the screen's entropy is given the black-hole value S = k_B c^3 A/(4 G hbar) (the paper's 6.41), it equals 6.74e60 J/K. The Bekenstein bound for Earth's energy inside radius R is 2 pi k_B R M c^2/(hbar c) = 9.38e51 J/K. The ratio is
S/S_bound = R/R_s = 7.18e8, with R_s = 2GM/c^2 = 8.87 mm for Earth [calc].
The paper says the entropy "appears to be very high, and violates the Bekenstein bound" [read: p.27]; it states the bound in natural units without the 2 pi (Section 3.3 above), and this example uses the SI form. The numbers show the excess is almost a billion at Earth's surface, and that it shrinks to 1 only at a black-hole horizon, which is where the author's Section 6.3 argument works with the real hbar (Section 4 above). The author's suggested ways out are rescaling hbar or non-equilibrium [read: p.27], and they are not worked out. So the screen "bits" cannot be literal thermal degrees of freedom with the real Planck constant away from horizons, which the author partly concedes ("the role of hbar is subtle", p.26).
What the example teaches. Every number in Verlinde's chain is correct, and the force comes out exactly right. It comes out right because the constants were fixed so that it would. The calculation is a consistent re-encoding of Newton's law in the language of bits, temperature and entropy. That is worth something: it shows that Newtonian gravity can be written as F = T dS/dx with an area-law bit count. But it is not an independent derivation, and it gives no new number to measure. Steps 7 and 8 show where the picture is rich (the inverse square and screen independence fall out neatly) and where it is strained (the closed-screen requirement and the Bekenstein bound).
6. Evidence table
Verdicts are the arbiter's [arbiter.md sections 5 and 10]. "Tested?" means a neutral experiment that distinguishes the claim from standard physics.
Terms used in the table (all [memory: high] as definitions): - GRANIT: an experiment at the Institut Laue-Langevin in Grenoble that studies ultra-cold neutrons (neutrons slow enough to bounce on a mirror) sitting in discrete quantum energy levels in Earth's gravity, just as an electron sits in levels in an atom. - EG: Emergent Gravity, Verlinde's 2016 model (claim 5b), not the 2010 paper. - Dark matter, Lambda-CDM: galaxies rotate too fast for their visible mass. The standard cosmological model, Lambda-CDM (Lambda for the cosmological constant or dark energy, CDM for "cold dark matter"), explains this with unseen matter. - MOND: Modified Newtonian Dynamics (Milgrom 1983), a rival to dark matter that changes Newton's law at very small accelerations, around 1e-10 m/s^2. EG makes MOND-like predictions for galaxies. - Tully-Fisher relation (baryonic): an observed law that a spiral galaxy's ordinary ("baryonic") mass, stars plus gas, is proportional to the fourth power of its outer rotation speed. - Radial acceleration relation: the observed one-to-one link, point by point in galaxies, between the acceleration actually measured and the acceleration the visible mass alone would produce by Newton's law. - Weak (galaxy-galaxy) lensing: the mass of foreground galaxies slightly bends the light of background galaxies; averaging the tiny distortions over thousands of galaxies measures how much mass (seen or not) surrounds them. - Mass-to-light ratio: how many kilograms of stars go with each watt of starlight; it must be assumed or estimated to turn light into baryonic mass. - Effective field theory: a theory trusted only up to some energy, written without knowing the deeper physics; "graviton effective field theory" is ordinary quantum mechanics applied to small ripples of Einstein's gravity.
| Claim | Tested? | Result | Replicated? | Verdict |
|---|---|---|---|---|
| 1. Gravity is an entropic force, F = T dS/dx | Not directly. Indirect arguments from ultra-cold neutron bound states in Earth's field (the GRANIT-type experiments; Nesvizhevsky 2002 [memory: high]) and the neutron phase-shift experiment of Colella-Overhauser-Werner 1975 [memory: high]. Kobakhidze argues these "disprove" entropic gravity [web] https://arxiv.org/abs/1009.5414. Chaichian, Oksanen and Tureanu reply that they need not, though spontaneous decays of excited states would need extra ingredients [web] https://arxiv.org/abs/1104.4650 | A contested theoretical reading of existing data, not a controlled test. Theoretical objections: a force T grad S is conservative only if grad T and grad S are parallel (Visser [web] https://arxiv.org/abs/1108.5240); the first law fails on non-horizon screens except with spherical symmetry (Wang and Braunstein [web] https://www.nature.com/articles/s41467-018-05433-9). The inventor's 2026 note calls it an "adiabatic reaction force" that "acts without increasing the entropy" and keeps quantum coherence [web] https://www.worldscientific.com/doi/10.1142/S0217751X26470020 (Investigator's reading). This does not replace the 2010 picture: the 2010 paper already says total entropy "will remain constant" for an infinite heat bath and "in first approximation stays the same" microcanonically [read: page image p.5], and imposes constant entropy under virtual displacement, eq. (5.38) [read: p.21]. What 2026 adds is a coherence argument and the new name [arbiter section 10 B]. The Strings 2011 talk already had a chapter titled "Adiabatic reaction forces" (title only, content not checked) [web via Investigator] | No | Strong form (a literal thermal force with noise and decoherence): Never properly tested, in theoretical difficulty and contested. Weak form (gravity's equations have a thermodynamic structure): Plausible, untested |
| 1b. Section 6.3: near a horizon, F_gravity = T_H dS_BH/dx (6.40), the Section 3 formulas hold with the real hbar, and the force stays entropic when the screen is moved outward | The horizon part is a recalculation of standard black-hole thermodynamics (Section 4 above; example.py Part F). No experiment on the off-horizon step | Near-horizon identity and Section 3 forms with the real hbar: correct, to leading order in l/r_s [calc by deep read]. Off-horizon step: assumed, not derived; the author says "we have no direct confirmation or proof" there (p.26). Wang and Braunstein find the first law fails on non-horizon screens except with spherical symmetry, which covers the Schwarzschild example [web] https://www.nature.com/articles/s41467-018-05433-9 | n/a | Identity (6.40) and Section 3 forms near a horizon, including the Rindler case: Established (standard black-hole thermodynamics). Causal reading "gravity is entropic there": Not testable as stated. Off-horizon extension: Never properly tested (contested by calculation, not dismissed) |
| 2. Inertia is entropic: (3.6) + Unruh T gives F = ma | No | Reproduces F = ma by construction (2 pi chosen, p.8) | n/a | Not testable as stated (a calibration, not a derivation) |
| 3. Newton's law and Poisson's equation from bits + equipartition | Only by reproducing Newton, which is built in | Algebra correct (Section 5 above); G defined by the bit count; Poisson reached by "requiring" Gauss's law on equipotentials plus a "bit of mass pushed across" argument (p.14) | n/a | Algebra: Established. As a derivation or explanation: Not testable as stated. General mass distributions: Never properly tested (Visser, Wang-Braunstein objections are calculations, not experiments) |
| 4. Relativistic version: Komar mass, Einstein equations | No | (5.30), (5.34) correct; Schwarzschild check returns M [deep; calc]. Einstein step a "sketch" with the matter side assumed (p.20) | n/a | Plausible, untested (Jacobson 1995 is the sounder version) |
| 5a. Space and gravity are emergent; redshift comes from entropy gradients (2010) | No | The paper says both readings are "equivalent in the relativistic setting" (p.19), so there is no measurable difference | n/a | Not testable as stated. AdS/CFT emergence: Established, in AdS only [memory: high] |
| 5b. Successor: "Emergent Gravity and the Dark Universe" (2016, a different model: area-plus-volume entropy) [web] https://arxiv.org/abs/1611.02269 | Yes, by several groups | For: Brouwer et al. 2017, weak lensing of 33,613 isolated galaxies, "good agreement" with no free parameters, "only a first step" [web] https://arxiv.org/abs/1612.03034. Brouwer et al. 2021 (Verlinde a co-author, an interested party): radial acceleration relation "agrees well" with EG and MOND [web] https://arxiv.org/abs/2106.11677. Against: the same 2021 paper finds a difference of at least 6 sigma between early- and late-type galaxies that galaxy-independent modified gravity "would be unable to explain" without extra circumgalactic gas, and Lambda-CDM also fits. Lelli, McGaugh and Schombert 2017 (MOND proponents, a rival theory): consistent only with stellar mass-to-light ratios "in tension with other astronomical estimates" [web] https://arxiv.org/abs/1702.04355. Pardo (JCAP 2020): for 452 isolated dwarfs, maximum velocities "severely underpredicted" above about 100 km/s and overpredicted below it [web] https://arxiv.org/abs/1706.00785. For, from the same Pardo work as the Investigator recorded it: EG reproduces the baryonic Tully-Fisher relation with no free parameters and fits most massive spirals [web via Investigator, sites.md]. Nieuwenhuizen 2017: galaxy cluster Abell 1689 needs extra (dark) matter for the whole family of dark-matter-free modified gravity theories [web] https://arxiv.org/abs/1610.01543 | Partly (lensing by the same Leiden group twice) | Split, both sides kept: Tested, not supported for isolated dwarfs (Pardo), the mass-to-light ratios Lelli et al. require, and the 6 sigma early/late-type difference. The lensing and Tully-Fisher agreement: Never properly tested as a neutral, controlled test (a first step; Verlinde co-authored the 2021 paper; Lambda-CDM fits too). Not a test of the 2010 paper |
| 6. Gravitational force fluctuations | 2010: no number given (p.27). Later quantitative "geontropic" model: Verlinde and Zurek [web] https://arxiv.org/abs/1902.08207. Experiment GQuEST designed [web] https://arxiv.org/abs/2404.07524 | No result found. Carney et al. say graviton effective field theory predicts length fluctuations of order 1e-35 m, so a large signal would mean that theory breaks down [web] https://arxiv.org/abs/2409.03894. A constraint from the Fermilab Holometer experiment on the model's parameter is quoted second-hand (in a search summary used by the contrarian); the arbiter could not confirm the figure from the GQuEST abstract, so it is unverified | No | 2010 form: Not testable as stated. Later form: Never properly tested (an experiment is being built; not dismissed) |
Record. The record does not go silent. The sequence runs: Dutch press announcement (de Volkskrant, 12 Dec 2009; not read, blocked), arXiv (Jan 2010), JHEP (2011), many replies and critiques in 2010-2011, the Spinoza Prize (2011), the 2016 model, independent astrophysical tests, the 2019-2025 fluctuation programme and a 2026 restatement by the author [web via Investigator; arbiter section 7]. Nothing was suppressed or dismissed without testing that the review could document. One gap stays open: the 2010 "prediction" (fluctuations) was never given a number in that paper, and whether the 2019 geontropic model is the same claim has not been checked. The early press and blog reception (Volkskrant, NYT 2010, Woit's blog) was not read. The only record of A. Strominger's reported remark, that reactions ranged from "can't be right" to "right and we already knew it", is the quote on Wikipedia [web via Investigator]. The Holometer limit on the later fluctuation model is in the record only as an unverified second-hand figure [arbiter section 3].
Other material kept in the record. J. Mäkelä (arXiv:1001.3808, Jan 2010) says the equations Verlinde postulates are consequences of Mäkelä's own earlier microscopic model of spacetime [web] https://arxiv.org/abs/1001.3808. This is a priority claim by the earlier model's author and was not evaluated. The paper itself says "it is an entropic force! That is the main statement, which is new and has not been made before" [read: p.9]. T. Padmanabhan's "Equipartition of energy in the horizon degrees of freedom and the emergence of gravity", arXiv:0912.3165, submitted 16 Dec 2009 (three weeks before Verlinde's posting), reinterprets S = E/2T as equipartition of horizon degrees of freedom [web] https://arxiv.org/abs/0912.3165 (abstract checked by the arbiter). Verlinde cites Padmanabhan only via arXiv:0911.5004. Nobody has compared the two papers, so no conclusion about priority is drawn; it is a lead for the next Investigator run. Further leads, unread beyond the Investigator's notes: M. Vonk (2012) reports that applying the idea to the universe gives dark-matter and dark-energy amounts "surprisingly close" to the measured fractions (his characterization, before the 2016 model); Tower Wang, "Modified entropic gravity revisited" (arXiv:1211.5722); Yoon's comments on the 2016 model (2019); Visser's own remark that a thermodynamic interpretation of general relativity is "plausible", and his v2 section on decoherence [web via Investigator; arbiter section 10 E]. Other entropic or thermodynamic gravity proposals: Padmanabhan 2010; Bianconi 2025, "Gravity from entropy"; Parker and Jeynes; and 2010 follow-ups by Cai-Cao-Ohta, Easson-Frampton-Smoot, Smolin and others [web via Investigator].
7. What a learner should take away
Solid. - Entropic forces are real: rubber elasticity, osmosis and colloid depletion forces. F = T dS/dx is standard statistical mechanics. - Black holes have entropy proportional to area and a temperature. The Unruh, Hawking and Bekenstein results fit together (Part E of the example). - Jacobson's 1995 result that Einstein's equations follow from delta Q = T dS on local horizons is a respected, if still interpretive, result. - Verlinde's own "clearest argument" (Section 6.3) is right where it is standard: near a black-hole horizon, F = T_H dS_BH/dx holds and his Section 3 formulas come out with the real hbar (example.py Part F). This is the strongest part of the paper's case, and it is a consistency relation, not proof that entropy is the cause. - Every algebraic step in Verlinde's chain is correct (Section 5), apart from a stray k_B in printed eq. (4.17) and loose signs in (4.25) and (5.27)/(5.30), where the magnitudes are right [deep].
Wrong or overstated, and why it is instructive. - "Practically from first principles" [read: p.9] is not accurate. G is defined by the bit count, the 2 pi is chosen, hbar can be rescaled, and the Unruh form is used after being called unnecessary. Section 5 shows this concretely: when a constant is fixed by the answer, agreeing with the answer is not evidence. Learning to count which inputs were tuned is the most transferable lesson here. The author himself says the arguments are "reversed" (p.9). - The polymer analogy works cleanly at constant temperature [read: p.5]. Verlinde's screen temperature varies from point to point for non-spherical sources. The curl of T grad S is grad T x grad S, so the force need not be conservative. That is the root of Visser's objection. - The Bekenstein-bound excess (a factor R/R_s, about 7e8 at Earth's surface) shows the area-law bits cannot be literal thermal degrees of freedom far from horizons, at least not with the real hbar. Read with Section 6.3, the lesson is sharper: the picture works with standard values exactly at horizons and needs extra assumptions everywhere else. Carrying a result from where it is derived to where it is only assumed is a common and instructive step to watch for.
Genuinely open. - Is gravity, at bottom, a statistical phenomenon over unknown microscopic degrees of freedom? Jacobson, Padmanabhan, AdS/CFT and Verlinde all point that way, and none has a microscopic model for our universe. - Is the entropic force conservative for several bodies with the paper's T and S? The arbiter names this calculation as decisive, and it has not been done (Visser's work bears on it). - Does an entropic gravity cause decoherence or excited-state decays in neutron bound states? The two published camps disagree. The 2026 "adiabatic" wording, which sharpens a constant-entropy element already in the 2010 paper (p.5), bears on the question. - Can the Section 6.3 argument be carried off the horizon in a form that survives Wang and Braunstein, for example with the "rescaled hbar" the author suggests (p.27)? The paper does not address it. - Do "geontropic" fluctuations exist? GQuEST could answer this. - Does the 2016 dark-gravity model survive independent galaxy tests with mass-to-light ratios fixed independently? The 6 sigma early/late-type difference is the sharpest test.
8. Check yourself
- A rubber band is an entropic spring. If you heat it at fixed length, does its tension go up or down, and why?
- In Section 5, Step 3, the equipartition temperature and the Unruh temperature agree to every digit. Why is this agreement not evidence for Verlinde's picture?
- Suppose someone doubles hbar everywhere in Verlinde's Section 3 chain. What happens to N, to T and to F?
- For a spherical screen of radius R and a test mass at distance d > R, Verlinde's rule gives dS/dx proportional to (R/d)^2. Show that T dS/dx is independent of R.
- Compute the Bekenstein-bound excess S/S_bound for a screen at the Sun's surface (M = 1.989e30 kg, R = 6.96e8 m).
9. Further reading
The inventor's own work - E. Verlinde, "On the Origin of Gravity and the Laws of Newton", arXiv:1001.0785; JHEP 04 (2011) 029. The project document. - E. Verlinde, "Emergent Gravity and the Dark Universe", arXiv:1611.02269; SciPost Phys. 2, 016 (2017). The 2016 successor model. - E. Verlinde and K. Zurek, arXiv:1902.08207 (and 1911.02018, 2208.01059). Spacetime fluctuations in interferometers. - E. Verlinde, "Why does gravity know about microscopic entropy?", IJMPA 41 (2026) 2647002. The 2026 restatement as an adiabatic reaction force [web] https://www.worldscientific.com/doi/10.1142/S0217751X26470020. - Strings 2011 talk, "The Hidden Phase Space of Our Universe" (slides at the IPMU mirror; not read by this review).
Mainstream background - D. V. Schroeder, An Introduction to Thermal Physics. Entropy, temperature, equipartition. - P. Nelson, Biological Physics. Entropic forces and polymer elasticity. - D. J. Griffiths, Introduction to Electrodynamics, chapter 2. Gauss's law and the Poisson equation (the mathematics of Section 5, Step 7). - J. B. Hartle, Gravity: An Introduction to Einstein's General Relativity. Redshift, the Schwarzschild geometry, black holes. - L. Susskind and J. Lindesay, An Introduction to Black Holes, Information and the String Theory Revolution. Black-hole entropy and holography. - T. Jacobson, "Thermodynamics of Spacetime: The Einstein Equation of State", PRL 75, 1260 (1995) [web] https://arxiv.org/abs/gr-qc/9504004. - T. Padmanabhan, "Thermodynamical Aspects of Gravity: New insights", Rep. Prog. Phys. 73, 046901 (2010); arXiv:0911.5004.
Critiques and tests (each states its own view) - M. Visser, JHEP 10 (2011) 140, arXiv:1108.5240 (conservative-force constraints). - Z.-W. Wang and S. L. Braunstein, Nat. Commun. 9, 2977 (2018) (first law on non-horizon screens). - A. Kobakhidze, PRD 83, 021502 (2011), arXiv:1009.5414; M. Chaichian, M. Oksanen and A. Tureanu, PLB 702, 419 (2011), arXiv:1104.4650 (the neutron debate). - M. Brouwer et al. 2017, arXiv:1612.03034, and 2021, arXiv:2106.11677; F. Lelli et al. 2017, arXiv:1702.04355; K. Pardo, arXiv:1706.00785; T. Nieuwenhuizen, arXiv:1610.01543 (tests of the 2016 model). - S. Vermeulen et al., GQuEST design, arXiv:2404.07524; D. Carney et al., arXiv:2409.03894. - Plain-language: M. Vonk, "De zwaartekracht als entropische kracht", quantumuniverse.nl (2012, Dutch), a polymer-analogy explainer by an Amsterdam string theorist, which also reports the dark-sector estimate above [web via Investigator] https://www.quantumuniverse.nl/de-zwaartekracht-als-entropische-kracht. - T. Padmanabhan, "Equipartition of energy in the horizon degrees of freedom and the emergence of gravity", arXiv:0912.3165 (Dec 2009) [web] https://arxiv.org/abs/0912.3165.
Answers
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Up. The restoring force is F = -(3 k_B T/(n b^2)) x, which is proportional to T. At higher temperature the thermal jiggling drives the chain toward coiled states harder. This is the experimental fingerprint of an entropic force, and Verlinde names it ("proportional to the temperature", p.5). In Verlinde's picture there is no separate knob to turn: the screen "temperature" is fixed by the gravitating mass itself (T proportional to M/R^2), so the rubber-band test of heating at fixed geometry has no direct analogue.
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Substitute N = A c^3/(G hbar) into T = 2Mc^2/(N k_B). You get T = hbar G M/(2 pi k_B c R^2) = hbar g/(2 pi k_B c), which is exactly the Unruh form with a = g. The agreement is an algebraic identity built in by defining G through the bit count. Any set of numbers would agree.
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N = A c^3/(G hbar) halves. T = 2Mc^2/(N k_B) doubles. dS/dx = 2 pi k_B m c/hbar halves. F = T dS/dx is unchanged. This is why the paper says hbar "can be chosen at will" (p.10), and why the temperature is not a firm prediction.
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T = hbar G M/(2 pi k_B c R^2) and dS/dx = (2 pi k_B m c/hbar)(R/d)^2. Their product is (hbar G M/(2 pi k_B c R^2)) x (2 pi k_B m c R^2/(hbar d^2)) = G M m/d^2. The R^2 cancels, so the force is the same for any screen inside the test mass's orbit. This is Gauss's law in disguise.
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R_s = 2GM/c^2 = 2 x 6.674e-11 x 1.989e30/(2.998e8)^2 = 2.95e3 m. S/S_bound = R/R_s = 6.96e8/2.95e3 = 2.36e5 [calc]. That is smaller than Earth's 7.2e8 because the Sun is more compact relative to its Schwarzschild radius, but still far above 1.