2013
DOI: 10.1007/s10714-013-1556-3
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Recent developments concerning generic spacelike singularities

Abstract: This is a review of recent progress concerning generic spacelike singularities in general relativity. For brevity the main focus is on singularities in vacuum spacetimes, although the connection with, and the role of, matter for generic singularity formation is also commented on. The paper describes recent developments in two areas and show how these are connected within the context of the conformally Hubble-normalized state space approach. The first area is oscillatory singularities in spatially homogeneous c… Show more

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Cited by 27 publications
(46 citation statements)
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“…(iii) The present dynamical systems formulation can be adapted so that it can be used in more general contexts such as anisotropic, spatially homogeneous cosmology and even for models without any symmetries at all, as shown for perfect fluids in, e.g., Refs. [13] and [14]. Such an extension of the present paper would make it possible to address the issue of initial conditions for inflation in a generic context.…”
Section: Introductionmentioning
confidence: 89%
“…(iii) The present dynamical systems formulation can be adapted so that it can be used in more general contexts such as anisotropic, spatially homogeneous cosmology and even for models without any symmetries at all, as shown for perfect fluids in, e.g., Refs. [13] and [14]. Such an extension of the present paper would make it possible to address the issue of initial conditions for inflation in a generic context.…”
Section: Introductionmentioning
confidence: 89%
“…Ω, β ± are continuous in τ , though not differentiable at the transition times. For details see, e.g., [1,2,22,[25][26][27][28].…”
Section: Classical Solutionsmentioning
confidence: 99%
“…As basic perturbation variables for the ΛCDM model we choose (u 1 , u 2 ) = (HB c , −φ c ), where we have scaled B c with H to obtain a dimensionless quantity, as discussed in [21] and [23]. We now specialize the governing equations (16) to the ΛCDM model, using equations (17) and (18). After expanding the ∂ N derivatives and replacing ∂ N by we obtain…”
Section: -Velocity Components According To the Relationmentioning
confidence: 99%
“…On the other hand a typical model undergoes a more complicated evolution described by BKL oscillations and possible so-called spike oscillations on approach to the singularity (see e.g. Uggla (2013) [18]). Nevertheless, the Hubble-normalized anisotropy scalars Σ 2 and C 2 remain bounded during this process, a result that we will use later in this section.…”
Section: Measures Of Anisotropy: the Shear And Weyl Tensorsmentioning
confidence: 99%