A working library of theoretical physics

The question bank

A shared set of stable question IDs, with space for assumptions, calculations, checks, and revised questions.

For a physicist entering another fieldSources checked 12 September 2026Editable working edition
80 questions · 16 chaptersChoose one question, make its assumptions explicit, and keep a record of what the answer changes.

These are entry points for an investigation. Calibration reproduces established results. A Diagnostic tests a specified model or inference. An Extension proposes bounded further work; it is not a promise of novelty or success. Read the linked chapter before treating a question as self-contained.

Notes are saved only in this browser, on this page. They are not written into the HTML or synchronized. Export a notebook to keep a durable copy or move between browsers. Imports preserve existing notes. Progress labels are your working record, not validation of a scientific result.

QG-1 · Quantum gravityCalibration

Which gravitational phases are physically joint?

Do: Derive the determinant criterion above and compute each mass's reduced-state eigenvalues as functions of $\Phi$. Produce an entropy-versus-phase plot.

Check: Entropy vanishes at $\Phi=0,2\pi$ and is maximal at $\Phi=\pi$. Changing any local row or column phase leaves it unchanged.

Meaning: Establishes the precise witness that a proposed weak-field experiment must preserve. It is a known two-qubit result, not a new theory of gravity.

Investigation notes and progress

QG-2 · Quantum gravityCalibration

When is a curvature correction small?

Do: For a background curvature radius $L$, estimate the ratio of $c_1R^2$ to the Einstein term using $R\sim L^{-2}$. Repeat after including a large dimensionless $c_1$.

Check: The ratio scales as $c_1/(M_{\rm P}L)^2$, up to geometric factors. Identify the actual breakdown scale rather than assuming it is always $M_{\rm P}$.

Meaning: Turns “low energy” into a condition on an observable regime and its coefficients.

Investigation notes and progress

QG-3 · Quantum gravityDiagnostic

Which correction is robust against unknown local interactions?

Do: In Donoghue's low-momentum scattering amplitude, separate polynomial terms from logarithms and other nonanalytic terms. Fourier-transform representative terms at nonzero separation.

Check: Contact terms and long-range tails must be distinguished; compare amplitudes or explicitly defined observables before comparing coordinate-dependent potentials.

Meaning: Produce a table of universal predictions and coefficients requiring measurement. This is a literature-guided calculation with established benchmarks.

Investigation notes and progress

QG-4 · Quantum gravityDiagnostic

How much decoherence destroys the phase witness?

Do: Apply independent dephasing channels to the two-path state. Calculate the negative eigenvalues, if any, of its partial transpose, obtained by transposing only one subsystem's indices.

Check: Recover the pure-state result at zero noise and a separable mixture at complete dephasing. Separate state entanglement from the sensitivity of a particular witness.

Meaning: Gives a quantitative noise budget within the model, not an apparatus design or a detection claim.

Investigation notes and progress

QG-5 · Quantum gravityExtension

Does a proposed classical mediator actually satisfy its stated restrictions?

Do: Choose one published classical-channel model. Write its allowed operations and noise explicitly, then test the QG-1 preparation under that dynamics.

Check: Account for any hidden shared quantum resource, direct nonlocal interaction, or measurement feedback. Reproduce its published result first.

Meaning: A defensible output is an assumption-dependent distinction between model classes. Novelty requires checking the specific mediator literature; the general witness argument is established.

Investigation notes and progress

BH-1 · Black holes and informationCalibration

Why do independent Hawking-like pairs fail to purify radiation?

Do: Construct one, two, and three Bell pairs. Trace their partners and compute radiation entropy. Compare with arbitrary pure states on the same total qubits.

Check: Entropy is additive for independent pairs; a pure total state has equal entropies on complementary factors.

Meaning: Isolates the offending independence assumption in a solvable model. The Bell-pair construction approximates only part of the Hawking argument.

Investigation notes and progress

BH-2 · Black holes and informationCalibration

Which assumptions produce a Page curve?

Do: Reproduce the figure from complex Gaussian vectors normalized to unit length. Then constrain the total excitation number and repeat.

Check: Verify normalization, equality of complementary entropies, and zero endpoint entropy. State the change of ensemble explicitly.

Meaning: Shows how conservation laws alter a random-state benchmark. Random states are not a dynamical derivation.

Investigation notes and progress

BH-3 · Black holes and informationDiagnostic

Does the entropy curve identify the radiation state?

Do: Construct different pure states with identical bipartite Schmidt coefficients, the nonnegative weights in a paired basis decomposition. Compare their local correlation functions.

Check: Entropies agree while a chosen observable differs. Report that observable and the measurement basis.

Meaning: Produces an explicit limit on what an island entropy calculation alone establishes about decoding or local measurements.

Investigation notes and progress

BH-4 · Black holes and informationDiagnostic

Where does the island saddle become competitive?

Do: Choose one two-dimensional evaporating model from the island review. Reproduce its no-island and island generalized entropies, including its matter state and regulator prescription.

Check: Verify the extremization before taking the minimum; track the domain of the semiclassical approximation.

Meaning: A successful output is a model-specific transition with assumptions, not an unqualified solution for every black hole.

Investigation notes and progress

BH-5 · Black holes and informationExtension

How robust is the entropy transition to an imperfect radiation collector?

Do: In that same model, first replace complete collection by a specified erasure channel in a finite-dimensional analogue. Vary collection efficiency and compute entropy and recoverable correlations separately.

Check: Recover full collection and total loss limits. Do not transplant the qubit channel into a gravitational bath without deriving the correspondence.

Meaning: Identifies an operationally precise modification worth comparing with existing partial-bath calculations; novelty remains to be checked.

Investigation notes and progress

DE-1 · Vacuum energy and cosmic accelerationCalibration

Which components dilute, and which accelerate expansion?

Do: Derive $\rho(a)$ for matter, radiation, and constant $w$. Plot their densities after choosing an explicitly illustrative normalization.

Check: Recover powers $-3$, $-4$, and $0$. Test acceleration using the total $\rho+3p$, rather than the sign of one component's pressure.

Meaning: Provides an exact baseline within homogeneous general relativity. The chosen normalization is not a fit to observations.

Investigation notes and progress

DE-2 · Vacuum energy and cosmic accelerationCalibration

Can a canonical scalar cross the vacuum equation of state?

Do: Use $w+1=2K/(K+V)$ and positive energy to establish the restriction. Integrate a simple smooth potential and plot $w(t)$.

Check: Monitor energy conservation and compare the slow-roll limit with kinetic domination.

Meaning: Rules out an entire simple mechanism for a specified behavior; it does not establish that observations require that behavior.

Investigation notes and progress

DE-3 · Vacuum energy and cosmic accelerationDiagnostic

Does a proposed cancellation survive adding one heavy field?

Do: In a selected vacuum-energy proposal, integrate out a massive scalar and follow both its threshold correction and the adjustable constant term.

Check: Distinguish cancellation fixed by an identity or symmetry from a parameter chosen again after matching. Check renormalization-scale independence.

Meaning: Produce a stability audit with explicit assumptions. This is more decisive than comparing an arbitrary cutoff estimate with cosmological data.

Investigation notes and progress

DE-4 · Vacuum energy and cosmic accelerationDiagnostic

What does a two-parameter dark-energy fit actually assume?

Do: Derive $\rho(a)$ for $w(a)=w_0+w_a(1-a)$ and map it into distances for a flat homogeneous model.

Check: Recover $\rho/\rho_0=a^{-3(1+w_0+w_a)}e^{3w_a(a-1)}$. Reproduce a published likelihood only with its covariance and other priors included.

Meaning: Separates a convenient interpolation of data from a physical scalar-field theory.

Investigation notes and progress

DE-5 · Vacuum energy and cosmic accelerationExtension

Which additional observable breaks an expansion-history degeneracy?

Do: Construct two explicitly specified models with similar $H(a)$ over an observed interval. Compare their linear matter-growth equations and a lensing prediction.

Check: Match background parameters first and state which perturbation equations change. Test stability before fitting.

Meaning: The output is a discriminating observable in a restricted model pair. Check existing growth-versus-geometry tests before claiming novelty.

Investigation notes and progress

DM-1 · Dark matterCalibration

What follows from a flat rotation curve?

Do: Derive the density above and compare with a centrally concentrated luminous mass whose large-radius speed falls as $r^{-1/2}$.

Check: Keep units explicit and identify the spherical and equilibrium assumptions. A halo extending to infinity has infinite mass, so introduce a finite outer range.

Meaning: Clarifies the difference between a robust kinematic discrepancy and a unique microscopic interpretation.

Investigation notes and progress

DM-2 · Dark matterCalibration

How gradual is freeze-out?

Do: Integrate the abundance equation using an explicit equilibrium density and compare with the post-freeze-out solution above. Vary the annihilation strength.

Check: Test the early equilibrium and late constant-yield limits; tighten numerical tolerances near departure from equilibrium.

Meaning: Produces a relic-abundance mechanism you can explain quantitatively. It assumes the thermal and expansion history.

Investigation notes and progress

DM-3 · Dark matterDiagnostic

Can two production histories yield the same abundance?

Do: Tune one freeze-out and one simple decay-driven freeze-in model to the same final density. Compare the momentum distribution and a scattering observable.

Check: Verify that the freeze-in species never equilibrates and that both parameter choices satisfy their approximations.

Meaning: Shows why matching abundance is insufficient and identifies information needed to break the degeneracy.

Investigation notes and progress

DM-4 · Dark matterDiagnostic

What does a nuclear-recoil search constrain?

Do: Derive the maximum elastic recoil energy $E_R^{\max}=2\mu_{\chi N}^2v^2/m_N$, with reduced mass $\mu_{\chi N}$ and nuclear mass $m_N$. Compare light and heavy particles.

Check: Fold a specified speed distribution, threshold, and efficiency into a rate before interpreting an event count.

Meaning: Separates particle physics, halo assumptions, and detector sensitivity. A high-energy event need not be compatible with every familiar dark-matter model.

Investigation notes and progress

DM-5 · Dark matterExtension

Which halo uncertainty can a second target remove?

Do: Choose two nuclear targets and one interaction. Ask whether a cross-target rate ratio or common minimum-speed interval reduces sensitivity to the unknown speed distribution.

Check: Include nuclear response and threshold differences. Reproduce one existing halo-independent construction before modifying it.

Meaning: A bounded inference problem with established predecessors; a failure to remove the degeneracy is still an informative result.

Investigation notes and progress

IN-1 · The origin of cosmic structureCalibration

Can you derive freezing without a horizon-crossing slogan?

Do: Differentiate the mode solution and verify its equation. Plot the physical amplitude as a function of $|k\eta|$.

Check: Recover the short-wavelength vacuum normalization and long-wavelength constant amplitude. Keep the test-field and exact-de-Sitter assumptions visible.

Meaning: Turns an often-used verbal mechanism into a controlled calculation.

Investigation notes and progress

IN-2 · The origin of cosmic structureCalibration

Does the same scalar amplitude fix the inflationary scale?

Do: Hold $\mathcal P_\zeta$ fixed while varying $H$ and $\epsilon$ within slow roll. In the same canonical setup use the tensor ratio $r\simeq16\epsilon$.

Check: Verify that many pairs give the same scalar amplitude but different tensor power. The tensor relation inherits the model assumptions.

Meaning: Identifies what a second observable adds and what an upper limit leaves degenerate.

Investigation notes and progress

IN-3 · The origin of cosmic structureDiagnostic

What does a third-point correlation test that the power spectrum cannot?

Do: Follow the squeezed limit, with one wavelength much longer than the others, in Maldacena's single-field relation. Explain its connection to a long mode acting as a rescaling.

Check: List the attractor, initial-state, and single-clock assumptions; an attractor erases dependence on an independent background velocity.

Meaning: A failure can reject that class of models, not automatically all inflation. [16]

Investigation notes and progress

IN-4 · The origin of cosmic structureDiagnostic

How much does reheating move an inferred potential?

Do: Choose one inflationary potential and two constant effective reheating equations of state. Track the same observed mode back to its exit time.

Check: Conserve energy in each phase and require a hot radiation era compatible with light-element production.

Meaning: Produces an uncertainty band tied to an unknown history, instead of a falsely unique reconstructed potential.

Investigation notes and progress

IN-5 · The origin of cosmic structureExtension

Which feature survives imperfect knowledge of the initial state?

Do: In the test-field model, mix positive and negative frequency solutions with explicitly normalized coefficients over a finite band. Track changes in two-point and selected higher correlations after adding a specified interaction.

Check: Bound the excitation energy so the test-field approximation survives, and recover the vacuum limit.

Meaning: A finite, testable robustness question; compare existing excited-initial-state studies before interpreting novelty.

Investigation notes and progress

BA-1 · Why matter survivedCalibration

When does an asymmetry survive after its source stops?

Do: Derive both solutions above and replace constant washout by a pulse with the same integrated strength.

Check: The post-source survival depends on the washout integral. Washout overlapping production need not have the same effect as washout after it.

Meaning: Produces a precise source-versus-survival distinction using an exactly solvable model.

Investigation notes and progress

BA-2 · Why matter survivedCalibration

Why does equilibrium obstruct the usual mechanism?

Do: Write forward and inverse reaction terms in a simple decay-plus-inverse-decay network. Derive the equilibrium cancellation with the required equilibrium distributions.

Check: Include every process needed at the chosen perturbative order and avoid counting an on-shell intermediate process twice.

Meaning: Identifies why a decay-rate asymmetry alone is not a consistent cosmological source.

Investigation notes and progress

BA-3 · Why matter survivedDiagnostic

Which charge is actually protected?

Do: List changes in $B$ and $L$ under a chosen set of reactions. Find linear combinations left unchanged by all fast reactions.

Check: Electroweak sphaleron processes preserve $B-L$ in the Standard Model. Adding lepton-number violation can remove that protection.

Meaning: A null-space calculation determines which initial or generated excess can survive a specified reaction network.

Investigation notes and progress

BA-4 · Why matter survivedDiagnostic

Does a low-energy CP phase fix the sign of leptogenesis?

Do: In a seesaw model with more than one heavy neutrino, count independent high-energy parameters and compare them with the light mass matrix.

Check: Construct distinct high-energy choices with the same low-energy data before claiming an inference of the cosmological sign.

Meaning: Exposes the extra assumptions required to connect laboratory CP violation with the origin of matter.

Investigation notes and progress

BA-5 · Why matter survivedExtension

When does the one-number washout description fail?

Do: Replace $Y_\Delta$ by a two-flavor vector and $W$ by a positive relaxation matrix. Rotate its weakly washed-out direction relative to the source and solve.

Check: Recover the one-flavor limit and verify that any apparent protection corresponds to a slow mode of the network.

Meaning: A tractable diagnostic for flavor effects, with established leptogenesis predecessors. A research extension must specify a new physical rate hierarchy.

Investigation notes and progress

NU-1 · Neutrino mass and identityCalibration

What information disappears from an oscillation probability?

Do: Derive the two-flavor probability from amplitudes. Shift both squared masses by the same constant and change the sign of their difference.

Check: The vacuum two-flavor probability is invariant under both changes. Verify zero mixing, zero baseline, and probability conservation.

Meaning: Identifies precisely which mass information requires a different experiment.

Investigation notes and progress

NU-2 · Neutrino mass and identityCalibration

When does the seesaw approximation become accurate?

Do: Compare the exact matrix eigenvalues and mixing angle with the large-$M$ expansion over a range of $m_D/M$.

Check: Track signed eigenvalues separately from positive physical masses. Recover a Dirac pair as the Majorana term tends to zero.

Meaning: Quantifies the regime of a familiar mechanism and prevents interpreting an approximation as a universal mass relation.

Investigation notes and progress

NU-3 · Neutrino mass and identityDiagnostic

Can a Majorana signal cancel even when every mass is nonzero?

Do: Treat the terms in $m_{\beta\beta}$ as complex vectors with fixed lengths. Derive the allowed minimum and maximum as their phases vary.

Check: The maximum is the sum of lengths; the minimum is zero or the largest length minus the other two, whichever is greater.

Meaning: Gives an exact cancellation test before inserting oscillation uncertainties or nuclear physics.

Investigation notes and progress

NU-4 · Neutrino mass and identityDiagnostic

How can matter imitate a CP asymmetry?

Do: Add a constant electron-density potential to a two-flavor Hamiltonian and compare neutrino and antineutrino probabilities.

Check: Reverse the matter-potential sign for antiparticles and recover equality in vacuum. Two flavors have no intrinsic oscillation CP phase.

Meaning: Demonstrates an environmental asymmetry that must be separated from intrinsic CP violation in realistic analyses.

Investigation notes and progress

NU-5 · Neutrino mass and identityExtension

Which extra observable narrows a degenerate mass mechanism?

Do: Choose a two-heavy-neutrino model and fix a compatible light mass matrix. Vary the remaining high-energy freedom and compute one specified heavy-light mixing or lepton-number-violating observable.

Check: Preserve the fitted low-energy matrix throughout; verify perturbativity and the validity of the heavy-mass expansion.

Meaning: Maps what one additional measurement could determine. Existing seesaw reconstruction literature is the novelty baseline.

Investigation notes and progress

HI-1 · The electroweak scale and flavorCalibration

What exactly fixes the symmetry-breaking scale?

Do: Minimize the scalar potential and expand around each stationary point. Identify stable minima, fluctuation masses, and the symmetric limit.

Check: Keep $\lambda>0$ for stability and distinguish the negative quadratic coefficient at the origin from a negative physical mass squared at a minimum.

Meaning: Separates the mechanism of symmetry breaking from the unexplained input scale.

Investigation notes and progress

HI-2 · The electroweak scale and flavorCalibration

Does a heavy particle decouple from every observable equally?

Do: Derive the threshold formula above and the leading $h^6$ coefficient from the same expansion.

Check: The scalar-mass shift grows with $M^2$ at fixed coupling, while higher-dimension terms carry inverse powers of $M$. Recover complete decoupling at zero portal coupling.

Meaning: Explains how effective-theory decoupling and mass sensitivity can coexist.

Investigation notes and progress

HI-3 · The electroweak scale and flavorDiagnostic

Which proposed symmetry actually protects the small scalar mass?

Do: Choose one explicit symmetry model and list the interactions that break its protection. Determine the first allowed mass correction.

Check: The correction must vanish in the exact protecting-symmetry limit. Include symmetry-breaking interactions already required by the model.

Meaning: Produces a model-specific stability test, not a qualitative declaration that a symmetry solves the hierarchy.

Investigation notes and progress

HI-4 · The electroweak scale and flavorDiagnostic

Which flavor predictions are independent of basis choices?

Do: Construct two small complex Yukawa matrices, whose entries couple the Higgs to fermions. Diagonalize them by unitary transformations and identify masses and relative left-handed rotations.

Check: Rotate both interaction bases and verify that singular values and observable mixing remain invariant. Zeros in a matrix need not be physical predictions.

Meaning: Establishes the correct objects for assessing a proposed flavor pattern before adding more parameters.

Investigation notes and progress

HI-5 · The electroweak scale and flavorExtension

Does a claimed low-tuning region survive a change of matching scale?

Do: In the two-scalar model, match at nearby scales and evolve parameters consistently. Compare a physical low-energy prediction and the chosen sensitivity measure.

Check: Physical predictions agree to the retained order; residual differences quantify omitted terms. Report the independent-parameter convention behind the sensitivity measure.

Meaning: A reproducible robustness study. Novelty requires a particular model or inference issue beyond the textbook threshold calculation.

Investigation notes and progress

CP-1 · Strong CP and the axionCalibration

Why is a quark mass phase part of the strong angle?

Do: For one massive quark, track a chiral field rotation through its mass term and the anomalous quantum measure. Identify the invariant angle in a declared sign convention.

Check: Repeating a field redefinition cannot change an observable. A total derivative must be treated with its boundary and topological information.

Meaning: Establishes which parameter needs explaining; setting the written gluonic coefficient to zero alone is insufficient.

Investigation notes and progress

CP-2 · Strong CP and the axionCalibration

How far does a small explicit breaking shift the axion minimum?

Do: Derive the shift above and compare with numerical minimization as $\varepsilon$ and $k$ vary.

Check: Recover zero shift at $\delta=0$ on the stable small-breaking branch; determine when the perturbative minimum ceases to describe the global minimum.

Meaning: A controlled robustness test with an exact numerical comparison.

Investigation notes and progress

CP-3 · Strong CP and the axionDiagnostic

Does cosmological damping guarantee relaxation before today?

Do: Solve $\ddot a+3H\dot a+\partial V/\partial a=0$ with an explicitly chosen expansion history and temperature-dependent $\chi(T)$.

Check: Recover a nearly frozen field when $H\gg m_a$ and oscillations when $H\ll m_a$. State the initial angle and velocity.

Meaning: Connects minimization to a dynamical history and to possible dark-matter energy, within the chosen potential.

Investigation notes and progress

CP-4 · Strong CP and the axionDiagnostic

What does an electric-dipole null result exclude?

Do: Write a linear response $d_n=c_\theta\bar\theta+\sum_jc_jg_j$ with hadronic coefficients and additional CP couplings $g_j$. Compare one-source and multi-source constraints.

Check: Propagate coefficient uncertainty and exhibit cancellations if several sources are allowed.

Meaning: Separates an experimental bound from the assumptions behind a strong-angle inference.

Investigation notes and progress

CP-5 · Strong CP and the axionExtension

Which symmetry-breaking operators threaten a particular axion construction?

Do: Choose one explicit field content and symmetry assignment. Enumerate its lowest allowed breaking operators and map them to harmonics of the angular potential.

Check: Include radiatively generated terms and calculate their minimum shifts using CP-2. Verify the assumed suppression scale.

Meaning: Produces a finite operator audit. Its novelty depends on the construction; the quality problem itself is established.

Investigation notes and progress

YM-1 · Confinement and the mass gapCalibration

Can local flux fluctuations produce a linear static potential?

Do: Derive the plaquette product identity and exact loop expectation above. Compare loops of equal area but different perimeter.

Check: Specify open boundaries and the absence of global flux constraints. Recover $\langle W\rangle\to1$ at fixed lattice area as $\beta\to\infty$.

Meaning: A complete mechanism in a solvable model, with a clear boundary on transfer to four dimensions.

Investigation notes and progress

YM-2 · Confinement and the mass gapCalibration

How does a correlator reveal a mass without fitting too early?

Do: Generate a two-exponential correlator $C(t)=A_0e^{-m_0t}+A_1e^{-m_1t}$ and compute $m_{\rm eff}(t)=a_t^{-1}\ln[C(t)/C(t+a_t)]$.

Check: Recover $m_0$ only when excited-state contamination is small. Include the backward exponential if modeling periodic Euclidean time.

Meaning: Exposes a basic extraction bias before interpreting lattice plateaus as a gap.

Investigation notes and progress

YM-3 · Confinement and the mass gapDiagnostic

Which limit is required to claim a continuum gap?

Do: Draw a sequence of regulated theories with fixed physical volume and decreasing spacing, followed by increasing volume. Track dimensionless masses and physical correlation lengths.

Check: A nonzero mass in lattice units need not represent the desired continuum limit. State how the scale is set and which errors are controlled.

Meaning: Produces a precise distinction between numerical evidence and a constructive existence theorem.

Investigation notes and progress

YM-4 · Confinement and the mass gapDiagnostic

What changes when a flux tube can break?

Do: Use a two-state Hamiltonian mixing a linearly rising string energy with a nearly constant two-meson threshold. Diagonalize as a function of source separation.

Check: Recover a true crossing at zero mixing and an avoided crossing otherwise. Analyze the overlap of a string-like trial operator with the ground state.

Meaning: Explains why a poor operator basis can hide string breaking even when it occurs in the spectrum.

Investigation notes and progress

YM-5 · Confinement and the mass gapExtension

Which confinement diagnostic survives a controlled model deformation?

Do: Choose one finite lattice gauge model and add an explicitly specified dynamical matter field. Compare loop behavior, static-source energies, and a gauge-invariant correlation length.

Check: Benchmark the pure-gauge and decoupled-matter limits before extrapolating. Keep boundary and volume effects visible.

Meaning: Can separate diagnostics that coincide in a toy limit. Novelty needs a particular deformation; it is not a plan to prove the Clay problem by small-system numerics.

Investigation notes and progress

QM-1 · Quantum measurement and classical recordsCalibration

What disappears under a partial trace?

Do: Derive the reduced matrix, visibility, and eigenvalues in the independent-record model. Plot entropy and visibility against $N$.

Check: Recover a pure reduced state at $\theta=0$ and a diagonal reduced state for orthogonal environment records. Global purity remains one.

Meaning: Establishes decoherence precisely without presupposing a particular interpretation of outcomes.

Investigation notes and progress

QM-2 · Quantum measurement and classical recordsCalibration

Can local measurements distinguish entanglement from ignorance?

Do: Compare the two-qubit Bell state with the equally weighted mixture of $|00\rangle$ and $|11\rangle$. Compute single-qubit states and the joint correlation $\langle X\otimes X\rangle$.

Check: Both local states equal the identity divided by two, while the correlation is one for the Bell state and zero for the mixture. $X$ flips $0$ and $1$.

Meaning: An exact example of why local diagonality does not identify the global physical state.

Investigation notes and progress

QM-3 · Quantum measurement and classical recordsDiagnostic

Which states become stable records for a given interaction?

Do: Compare a system coupled to an environment through $Z$ with one coupled through $X$, where $Z$ distinguishes $0$ and $1$ and $X$ exchanges them.

Check: Identify which eigenstates are left undisturbed by each coupling. Add a noncommuting system Hamiltonian and track the competition.

Meaning: Explains a preferred record basis dynamically rather than declaring one in advance.

Investigation notes and progress

QM-4 · Quantum measurement and classical recordsDiagnostic

Which collapse effect is distinguishable from ordinary noise?

Do: Choose one published collapse model and one explicit environmental-noise model. Compare their predicted dependence on mass, separation, and interrogation time.

Check: Fix nuisance parameters using independent information. Agreement at one point does not establish agreement across a controlled scan.

Meaning: Produces a testable model comparison. This is a dynamics question, not a generic experiment deciding all interpretations.

Investigation notes and progress

QM-5 · Quantum measurement and classical recordsExtension

How much environmental access is needed to restore interference?

Do: In the independent-record model, reverse the interaction on only $k$ environment qubits. Compute the remaining visibility and compare with the best allowed joint measurement on the accessible part.

Check: Recover full reversal at $k=N$ and ordinary reduced visibility at $k=0$. State which operations and records are available.

Meaning: A tractable access-dependent question. The simple model is established; a worthwhile extension needs a specified correlated environment or operational restriction.

Investigation notes and progress

TH-1 · Thermalization and the arrow of timeCalibration

Which information survives time averaging?

Do: Derive the diagonal-ensemble expression from the finite-time integral of each phase. Repeat with one exact energy degeneracy.

Check: Equal-energy coherences survive; distinct energies require long averaging compared with their inverse splitting.

Meaning: Identifies both the approximation and the memory left after dephasing.

Investigation notes and progress

TH-2 · Thermalization and the arrow of timeCalibration

Can local entropy rise without global entropy production?

Do: Evolve a small chain with the Hamiltonian above. Calculate a one-spin reduced state and its entropy alongside global purity and energy.

Check: Global purity and energy remain constant within numerical error. Report local entropy decreases and recurrences rather than removing them.

Meaning: Reconciles unitary evolution with local mixedness in a fully specified finite model.

Investigation notes and progress

TH-3 · Thermalization and the arrow of timeDiagnostic

Does breaking integrability make the chosen observable thermal?

Do: Compare $g_z=0$ with a generic nonzero value at matched energy density. Plot diagonal matrix elements of a local observable against energy, resolving symmetries.

Check: Use several sizes and the same energy window. Smoothness alone is not enough if the initial energy distribution is broad.

Meaning: Produces a scoped eigenstate-thermalization diagnostic, not a universal law.

Investigation notes and progress

TH-4 · Thermalization and the arrow of timeDiagnostic

What happens if the apparently thermalizing state is reversed?

Do: Evolve a product state forward, then reverse the evolution exactly; repeat with a small controlled Hamiltonian error.

Check: Exact reversal returns the initial state. Quantify how errors affect a local observable and global overlap differently.

Meaning: Separates fundamental reversibility, special preparation, and practical irreversibility.

Investigation notes and progress

TH-5 · Thermalization and the arrow of timeExtension

Which observable forgets the initial state last?

Do: In one chain family, compare local magnetization, a two-point correlation, and a subsystem entropy after matched-energy quenches. A quench is a specified sudden parameter change.

Check: Define a relaxation tolerance and time window before inspecting results. Test sizes and initial states to distinguish slow dynamics from finite-size recurrences.

Meaning: A useful model-specific hierarchy of memory; novelty requires comparison with known conserved and nearly conserved modes.

Investigation notes and progress

TU-1 · Turbulence and anomalous dissipationCalibration

Can dissipation survive a coefficient tending to zero?

Do: Verify the shock solution and evaluate the dissipation integral analytically and numerically for several viscosities.

Check: Increase spatial resolution as the width decreases and include boundary energy flux. The integral tends to $2U^3/3$ without inventing a forcing term.

Meaning: A complete controlled example of a singular dissipation limit.

Investigation notes and progress

TU-2 · Turbulence and anomalous dissipationCalibration

What assumptions go into the minus-five-thirds spectrum?

Do: Derive the spectrum from units and its normalization. Then allow an outer length or a fluctuating local transfer rate as an extra input.

Check: Distinguish dimensional consistency from a uniqueness theorem. Define the scale interval in which forcing and viscosity are both negligible in the balance.

Meaning: Reveals exactly what the scaling argument explains and leaves undetermined.

Investigation notes and progress

TU-3 · Turbulence and anomalous dissipationDiagnostic

Can a measured structure function test the energy flux?

Do: In a homogeneous, isotropic, statistically stationary three-dimensional dataset, compare the longitudinal third-order velocity increment with the inertial-range prediction $\langle(\delta u_L)^3\rangle=-4\varepsilon r/5$. Here $\delta u_L=[\mathbf u(\mathbf x+\mathbf r)-\mathbf u(\mathbf x)]\cdot\hat{\mathbf r}$ is the velocity difference projected along the separation.

Check: Account for finite-viscosity, forcing, anisotropy, and finite-sampling corrections before declaring a violation.

Meaning: Tests a constrained flux relation rather than merely fitting a spectral slope. Its assumptions and limiting range are essential. [35]

Investigation notes and progress

TU-4 · Turbulence and anomalous dissipationDiagnostic

Which rare events dominate high moments?

Do: For a specified velocity dataset or synthetic model, compare $\langle|\delta u|^p\rangle$ for several orders $p$, including sensitivity to removing a small extreme tail.

Check: Use independent samples and convergence checks. A high-order moment with no stable estimate is not a measured exponent.

Meaning: Quantifies intermittency and distinguishes statistical uncertainty from failure of simple scaling.

Investigation notes and progress

TU-5 · Turbulence and anomalous dissipationExtension

Which coarse-graining scale reveals a stable energy flux?

Do: Filter one resolved velocity field at several lengths and derive the sub-filter transfer from the filtered equation. Compare it with the dissipation estimate.

Check: The filter definition and boundaries must be explicit; verify the resolved-plus-unresolved energy balance and vary the filter shape.

Meaning: A bounded robustness study of scale transfer. Existing coarse-graining theory is the starting benchmark, not a novelty claim.

Investigation notes and progress

SM-1 · Strange metals and electrical resistanceCalibration

Can an interacting clean metal have zero direct-current resistance?

Do: Derive current–momentum proportionality for a parabolic band and the conductivity above. Examine $\Gamma\to0$ at finite and then zero frequency.

Check: The clean real conductivity contains a zero-frequency delta contribution; the order and meaning of limits must be stated.

Meaning: Establishes a conservation-law obstruction to a naive collision-rate argument.

Investigation notes and progress

SM-2 · Strange metals and electrical resistanceCalibration

How uncertain is an inferred Planckian coefficient?

Do: Use the slope formula to propagate uncertainties in $A$, $n$, and $m$ into $\alpha$. Repeat with a temperature-dependent current weight.

Check: Keep SI units or a fully declared natural-unit convention throughout. Identify correlated inputs instead of treating every error independently.

Meaning: Separates an empirical slope from a model-dependent relaxation time.

Investigation notes and progress

SM-3 · Strange metals and electrical resistanceDiagnostic

Which step makes disorder essential in a solvable strange-metal model?

Do: Follow the cited random-interaction model through its conductivity calculation. Identify the term that relaxes current and compare with a spatially uniform coupling.

Check: Include the corrections required by charge conservation when relating self-energy to conductivity. Recover the stated clean-limit behavior.

Meaning: Determines necessity or sufficiency only within the specified model, not for every strange metal. [36]

Investigation notes and progress

SM-4 · Strange metals and electrical resistanceDiagnostic

Can one mechanism explain transport and thermodynamics together?

Do: For a single chosen parameter set, compare the predicted temperature dependence of resistivity, optical conductivity, and specific heat, the derivative of energy with temperature.

Check: Use one parameter set and one regime. Record which observable is fitted and which is then predicted.

Meaning: A mechanism becomes informative when agreement with one measurement constrains another; a separate fit for every curve weakens the test.

Investigation notes and progress

SM-5 · Strange metals and electrical resistanceExtension

Which disorder dependence separates two plausible mechanisms?

Do: Choose a conventional momentum-relaxation model and one critical-interaction model. Vary only a specified disorder parameter and compare residual resistance and temperature slope.

Check: Determine whether disorder also changes carrier density, pairing, or the critical point. Hold those fixed only when the model permits it.

Meaning: Produces an experimentally motivated comparison with explicit nuisance effects. Novelty depends on the selected pair and observable.

Investigation notes and progress

SC-1 · Unconventional superconductivityCalibration

What does repulsion actually do in the two-site problem?

Do: Derive the dimer spectrum and double occupancy using the derivative of $E_s$ with respect to $U$.

Check: The derivative gives total double occupancy over both sites. Recover the large-$U$ exchange and the noninteracting spectrum.

Meaning: Establishes superexchange with correct factors. It does not demonstrate superconductivity or a universal optimum interaction.

Investigation notes and progress

SC-2 · Unconventional superconductivityCalibration

When can a repulsive kernel favor a sign-changing gap?

Do: Diagonalize the two-patch kernel for varying $u/g$, then give patches unequal density-of-states weights.

Check: Recover the symmetric result and distinguish an attractive pairing eigenvalue from a measured critical temperature.

Meaning: Explains a mechanism for channel selection and identifies which symmetry information the toy model lacks.

Investigation notes and progress

SC-3 · Unconventional superconductivityDiagnostic

Does a small-cluster binding energy predict long-distance order?

Do: Compare a defined pair-binding energy with pair-correlation decay across a sequence of small clusters or ladders using the same Hamiltonian.

Check: Fix boundary conditions and particle-number conventions. Pair binding on one cluster is neither necessary nor sufficient evidence for a two-dimensional condensate.

Meaning: Locates the inferential gap between local energetics and a thermodynamic superconducting phase.

Investigation notes and progress

SC-4 · Unconventional superconductivityDiagnostic

Is phase stiffness a ceiling or the actual limiting scale?

Do: In a chosen two-dimensional model, compute or use benchmark values of temperature-dependent stiffness and pairing amplitude. Compare the stiffness transition criterion with the pairing scale.

Check: Use renormalized stiffness near the transition, not only its zero-temperature value. State dimensional and interaction assumptions.

Meaning: Determines the bottleneck in that regime; an upper bound alone cannot establish it. [38]

Investigation notes and progress

SC-5 · Unconventional superconductivityExtension

Which conclusion survives changing the microscopic reduction?

Do: Match a small multi-orbital cluster to a one-band model using low-energy levels. Compare one additional pair or spin observable not used in matching.

Check: Transform observables as well as the Hamiltonian and identify the energy window where discarded states remain separated.

Meaning: Tests transfer of a mechanism across a reduction. It is a bounded continuation of the original cuprate program, with novelty requiring a specific regime and comparison.

Investigation notes and progress

AQ-1 · Local quantum fields and operational accessCalibration

Can infinite-dimensional quantum mechanics still have ordinary subsystems?

Do: Derive the oscillator covariances and entropy. Compare a truncated oscillator calculation as the number-state cutoff increases.

Check: Recover zero coupling and the uncertainty bound $\nu\geq1/2$. Separate truncation errors from the exact infinite-dimensional type-I result.

Meaning: Prevents confusing infinitely many levels, strong entanglement, and type-III local structure.

Investigation notes and progress

AQ-2 · Local quantum fields and operational accessCalibration

Which entropy quantity survives comparing nearby states?

Do: For two full-rank finite Gaussian or qubit states, compute relative entropy before and after discarding a subsystem or applying dephasing.

Check: Verify nonnegativity and monotonicity; study what happens when the reference state loses support on part of the other state.

Meaning: Establishes a dependable distinguishability tool and the conditions under which it can diverge.

Investigation notes and progress

AQ-3 · Local quantum fields and operational accessDiagnostic

What changes when a boundary is given a finite buffer?

Do: On a massive free-field lattice, compare adjacent regions with regions separated by a fixed physical gap. Refine the spacing while keeping region and buffer sizes physical.

Check: Separate ultraviolet, volume, and mass effects. For mutual information, compute the entropy combination in a common regulator before extrapolating.

Meaning: Tests the value of separation for a specified information quantity. A numerical limit is evidence in this model, not a proof of the split property.

Investigation notes and progress

AQ-4 · Local quantum fields and operational accessDiagnostic

What is the operational cost of a local postselection?

Do: In a finite entangled-chain analogue, choose a local measurement outcome intended to prepare a distant target. Track conditional fidelity, success probability, and energy change together.

Check: Average over all local outcomes and verify no change in the distant reduced state. High conditional fidelity must not hide vanishing success.

Meaning: Makes the resource issue behind remote-preparation statements concrete without equating the chain with continuum QFT.

Investigation notes and progress

AQ-5 · Local quantum fields and operational accessExtension

Which continuum distinction remains after an energy budget is imposed?

Do: Specify one local discrimination or preparation task, two state families, a spatial buffer, and a bound on injected energy. Compare a free-field continuum prediction with convergent lattice approximations.

Check: Hold physical budgets fixed as the cutoff changes; inspect whether the claimed advantage requires energy or operator norms to diverge.

Meaning: A focused bridge between algebraic structure and operations. Its novelty must be checked against energy-constrained and split-inclusion literature before a research claim.

Investigation notes and progress