Relativity, Gravitation and Cosmology (Cheng)
July 2005 Corrections
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correction |
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121 |
line above Eq(7.19) |
Insert sidebar number ‘4’ to
read: “or
equivalently a critical energy density4 of” and add new sidebar: “ 4 In
the natural unit system of quantum field theory, this energy per unit volume
is approximately (2.5×10-3eV)4/(ħc)3,
where ħ is Planck’s
constant (over 2p) with ħc ≈ 2×10-5eV∙cm.” |
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184 |
subtitle: Possible resolution ... |
Change ‘L’ to ‘dark energy’ and add sidebar superscript ‘5’ in title to read: “Possible resolution through a
nonvanishing dark energy5”
and add the new sidebar: “ 5 Dark energy is
defined as the “negative equation-of-state energy”, w < 0 in Eq. (8.4). It gives rise to a gravitational repulsion
(cf. Sec 9.1.1). The simplest example of a dark energy is Einstein’s
cosmological constant, with w = -1.
NB: One should not confuse this with the energies of neutrinos, black holes,
etc., which are also ‘dark’, but are counted as parts of the “dark matter”
(cf. Sec 7.1.4), as the associated pressure is not negative.” |
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185 |
sidebar 6 (sidebar 5
before renumbering on p.184) |
Change sidebar to read: “ 6
A Hubble curve (as in Fig 9.7) is a
plot of the luminosity distance versus the redshift (measuring recession
velocity). A straight Hubble curve means a cosmic expansion that is coasting.
This can only happen in an empty universe (cf. Sec 7.1.3 and Fig 8.2). If the
expansion is accelerating, the expansion rate H must be smaller in the past. From Eq. (7.5): H∆r = z, we see that, for a given
redshift z, the distance ∆r to the light-emitting
supernova must be larger than that for an empty or decelerating universe.” |
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282 |
2nd line above Eq.
(A.21) |
Insert ‘is’ before ‘associated’
and replace ‘rX ≈ rc’ by ‘,
being comparable to the critical density rcc2 [cf. Eq. (7.19)],’ to read: “is associated with the dark energy. The observed dark energy, being comparable
to the critical density rcc2 [cf. Eq. (7.19)], then corresponds to…” |