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Equation 1 · Part 6 · Reading the Oldest Light: How a Temperature Map Becomes a Cosmology

fraction

θs=rs(z∗)DA(z∗).\theta_{\mathrm s} = \frac{r_{\mathrm s}(z_\ast)}{D_{\mathrm A}(z_\ast)}.
fraction

What this part means

Divide the expression above the line by the one below it.

Its job in the formula

The expression above the fraction bar is divided by the complete expression below it. The denominator must not be zero.

The passage around this formula

The consequence is a harmonic series in the sky. Modes that happened to be at maximum compression or maximum rarefaction at last scattering show the largest temperature contrast; modes caught at their zero crossing show the least. Because the phase depends on wavenumber times the sound horizon, the peaks fall at multiples of a fundamental scale. The physical length of that scale is the comoving sound horizon at last scattering, and the angle it subtends is a ratio of two lengths: θs=rs(z∗)DA(z∗)\theta_{\mathrm s} = \frac{r_{\mathrm s}(z_\ast)}{D_{\mathrm A}(z_\ast)}. The numerator is set by pre-recombination physics — the expansion rate and sound speed before decoupling, which depend on the baryon and radiation densities. The denominator is set by everything…

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Learn the underlying idea

A fraction a/b means a divided by b. The top number is the numerator; the bottom number is the denominator, and it cannot be zero.

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Sources cited in the article section

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