ASTR 420 Lecture 09: Dark Matter and the Growth of Structure

Cosmology ยท study notes

Learning objectives

Terms Developed in Context

These terms form the lecture's reasoning chain from observable through model to a bounded physical conclusion.

Density contrast

The fractional density departure delta=(rho-rhobar)/rhobar from the cosmic mean. In this lecture it supports the evidence-to-model chain for linear growth, transfer functions, and gravitational collapse.

Use and relationship: Read it together with Nonlinear collapse and Linear growth factor. The governing relation \(\\delta(a)=\\delta\\rho/\\bar\\rho,\\quad \\delta\\propto a\\;\\text{(matter era)}\) shows where the concept enters quantitatively; the student should state whether its value is measured, calibrated, adopted, or inferred.

Boundary: The result remains linear only until delta approaches unity; collapsed halos require nonlinear dynamics. This caveat prevents the term from being treated as a unique explanation or a context-free number.

Linear growth factor

The time-dependent multiplier describing perturbation growth while density contrasts remain much smaller than unity. In this lecture it supports the evidence-to-model chain for linear growth, transfer functions, and gravitational collapse.

Use and relationship: Read it together with Density contrast and Transfer function. The governing relation \(\\delta(a)=\\delta\\rho/\\bar\\rho,\\quad \\delta\\propto a\\;\\text{(matter era)}\) shows where the concept enters quantitatively; the student should state whether its value is measured, calibrated, adopted, or inferred.

Boundary: The result remains linear only until delta approaches unity; collapsed halos require nonlinear dynamics. This caveat prevents the term from being treated as a unique explanation or a context-free number.

Transfer function

The scale-dependent processing that maps primordial perturbations into the later matter distribution. In this lecture it supports the evidence-to-model chain for linear growth, transfer functions, and gravitational collapse.

Use and relationship: Read it together with Linear growth factor and Cold dark matter. The governing relation \(\\delta(a)=\\delta\\rho/\\bar\\rho,\\quad \\delta\\propto a\\;\\text{(matter era)}\) shows where the concept enters quantitatively; the student should state whether its value is measured, calibrated, adopted, or inferred.

Boundary: The result remains linear only until delta approaches unity; collapsed halos require nonlinear dynamics. This caveat prevents the term from being treated as a unique explanation or a context-free number.

Cold dark matter

A nonrelativistic, weakly interacting matter component that clusters gravitationally on cosmological scales. In this lecture it supports the evidence-to-model chain for linear growth, transfer functions, and gravitational collapse.

Use and relationship: Read it together with Transfer function and Nonlinear collapse. The governing relation \(\\delta(a)=\\delta\\rho/\\bar\\rho,\\quad \\delta\\propto a\\;\\text{(matter era)}\) shows where the concept enters quantitatively; the student should state whether its value is measured, calibrated, adopted, or inferred.

Boundary: The result remains linear only until delta approaches unity; collapsed halos require nonlinear dynamics. This caveat prevents the term from being treated as a unique explanation or a context-free number.

Nonlinear collapse

The regime in which density contrasts approach or exceed unity and linear perturbation theory fails. In this lecture it supports the evidence-to-model chain for linear growth, transfer functions, and gravitational collapse.

Use and relationship: Read it together with Cold dark matter and Density contrast. The governing relation \(\\delta(a)=\\delta\\rho/\\bar\\rho,\\quad \\delta\\propto a\\;\\text{(matter era)}\) shows where the concept enters quantitatively; the student should state whether its value is measured, calibrated, adopted, or inferred.

Boundary: The result remains linear only until delta approaches unity; collapsed halos require nonlinear dynamics. This caveat prevents the term from being treated as a unique explanation or a context-free number.

Lecture arc

The linear result is a controlled approximation only before collapse; nonlinear structure requires simulations and a specified power spectrum. Begin with the observational puzzle and ask students what is directly measured. Introduce linear growth, transfer functions, and gravitational collapse only after the data-model boundary is explicit.

The visual is a reasoning object: students should narrate what each line, region, or axis means before seeing the equation.

Derivation and interpretation

\(\\delta(a)=\\delta\\rho/\\bar\\rho,\\quad \\delta\\propto a\\;\\text{(matter era)}\)

Define the symbols, units, and assumptions. Explain why the relation is useful and where it fails. Relate the result to the paired lab's data record rather than treating the equation as a detached recipe.

nonlineardelta=1scale factor
linear growth, transfer functions, and gravitational collapse. The axes, labels, and geometry carry the physical inference rather than serving as decoration.

Worked example

Linear matter-era growth from z=1100 to today is a factor of 1+z = 1101; a 10^-5 seed becomes 0.01101 in the idealized model.

The result remains linear only until delta approaches unity; collapsed halos require nonlinear dynamics. Require students to estimate the answer, show units, and state whether the approximation is controlled, empirical, or merely illustrative.

Misconceptions and study guidance

The linear result is a controlled approximation only before collapse; nonlinear structure requires simulations and a specified power spectrum. Common traps include confusing redshift with a unique velocity, treating a model-dependent parameter as a direct measurement, and overlooking covariance. Study by reproducing the calculation, changing one assumption, and comparing the result with the exact OpenStax anchor listed in the reference log.

Preparation for the problem set: write a one-paragraph evidence chain from observation to conclusion and identify the weakest link.