Corrigenda to Inhomogeneous universes in observational coordinates (vol 13, pg 253, 1996)

Roy Maartens; Neil P. Humphreys; David R. Matravers; William R. Stoeger

doi:10.1088/0264-9381/13/6/030

Corrigenda to Inhomogeneous universes in observational coordinates (vol 13, pg 253, 1996)

Roy Maartens, Neil P. Humphreys, David R. Matravers, William R. Stoeger

Institute of Cosmology & Gravitation

Research output: Contribution to journal › Article › peer-review

Abstract

Four corrections should be made to this paper:

1. The right-hand side of equation (20) should be -½mN*AB/C³.

2. The equation before (23) should read v2 + 2uv = 1 -mN*/C.

3. The factor M in equations (42) and (43) should be replaced by N'.

4. Point (iii) at the end of section 3 implicitly assumes Ȧ (w₀, y) = Ḃ(w₀,y). It should
be replaced by:
(iii) A past null-cone integral for F.y/ may be obtained from equations (24) and (27):

F(y) = 1/2I ∫[(Cv² + C)'/Cv] Idy

where

I(y) = Cv exp (1/2 m ∫ N'/Cv dy)

Original language	English
Pages (from-to)	1689-1689
Journal	Classical and Quantum Gravity
Volume	13
Issue number	6
DOIs	https://doi.org/10.1088/0264-9381/13/6/030
Publication status	Published - Jun 1996

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title = "Corrigenda to Inhomogeneous universes in observational coordinates (vol 13, pg 253, 1996)",

abstract = "Four corrections should be made to this paper: 1. The right-hand side of equation (20) should be -½mN*AB/C3. 2. The equation before (23) should read v2 + 2uv = 1 -mN*/C. 3. The factor M in equations (42) and (43) should be replaced by N'. 4. Point (iii) at the end of section 3 implicitly assumes Ȧ (w0, y) = Ḃ(w0,y). It shouldbe replaced by:(iii) A past null-cone integral for F.y/ may be obtained from equations (24) and (27):F(y) = 1/2I ∫[(Cv2 + C)'/Cv] IdywhereI(y) = Cv exp (1/2 m ∫ N'/Cv dy)",

author = "Roy Maartens and Humphreys, {Neil P.} and Matravers, {David R.} and Stoeger, {William R.}",

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T1 - Corrigenda to Inhomogeneous universes in observational coordinates (vol 13, pg 253, 1996)

AU - Maartens, Roy

AU - Humphreys, Neil P.

AU - Matravers, David R.

AU - Stoeger, William R.

PY - 1996/6

Y1 - 1996/6

N2 - Four corrections should be made to this paper: 1. The right-hand side of equation (20) should be -½mN*AB/C3. 2. The equation before (23) should read v2 + 2uv = 1 -mN*/C. 3. The factor M in equations (42) and (43) should be replaced by N'. 4. Point (iii) at the end of section 3 implicitly assumes Ȧ (w0, y) = Ḃ(w0,y). It shouldbe replaced by:(iii) A past null-cone integral for F.y/ may be obtained from equations (24) and (27):F(y) = 1/2I ∫[(Cv2 + C)'/Cv] IdywhereI(y) = Cv exp (1/2 m ∫ N'/Cv dy)

AB - Four corrections should be made to this paper: 1. The right-hand side of equation (20) should be -½mN*AB/C3. 2. The equation before (23) should read v2 + 2uv = 1 -mN*/C. 3. The factor M in equations (42) and (43) should be replaced by N'. 4. Point (iii) at the end of section 3 implicitly assumes Ȧ (w0, y) = Ḃ(w0,y). It shouldbe replaced by:(iii) A past null-cone integral for F.y/ may be obtained from equations (24) and (27):F(y) = 1/2I ∫[(Cv2 + C)'/Cv] IdywhereI(y) = Cv exp (1/2 m ∫ N'/Cv dy)

U2 - 10.1088/0264-9381/13/6/030

DO - 10.1088/0264-9381/13/6/030

M3 - Article

SN - 0264-9381

VL - 13

SP - 1689

EP - 1689

JO - Classical and Quantum Gravity

JF - Classical and Quantum Gravity

IS - 6

ER -

Corrigenda to Inhomogeneous universes in observational coordinates (vol 13, pg 253, 1996)

Abstract

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