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Equation 4 · Part 2 · Comparing the Main Approaches to Precision Cosmology

Symbol a

w(a)=w0+wa(1−a)w(a) = w_0 + w_a (1 - a)
aa

What this part means

a is an argument of the function-like quantity on the left; its role is set by that function’s stated inputs.

Its job in the formula

a is an argument of the function-like quantity on the left; its role is set by that function’s stated inputs.

The passage around this formula

Evolving dark energy , in the w0-wa parametrization, keeps the sound horizon alone and instead lets dark energy’s equation of state change with cosmic time: w(a)=w0+wa(1−a)w(a) = w_0 + w_a (1 - a). where a is the cosmic scale factor (a = 1 today) and w = -1 recovers a plain cosmological constant. This is the family DESI’s DR2 BAO release put back on the table: fit jointly to DESI BAO, Planck CMB, and supernovae, a w0-wa model is preferred over flat LambdaCDM at up to several sigma, with the preferred trajectory suggesting dark energy was somewhat more negative than -1 in the past and is evolving toward less negative values now [ 3 , 4 ] .

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Learn the underlying idea

A variable is a named place for a value. Its letter is a local label: x can mean position in one formula and a data point in another.

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Sources cited in the article section

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