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1
Introduction
2
Outline
3
The cosmological constant
4
Einstein equations
5
Main result
6
Motivation
7
Setting
8
Theorem
9
Proof by contradiction
10
Proof by intuition
11
Proof of causal theory
12
Proof of strong causality
13
Applications to inflationary theory
14
The inflationary era
15
Freemans second equation
16
Future work
17
C0 conformal extension
18
Freeman equations
19
Future directions
Description:
Explore a lecture on the cosmological constant's role as an initial condition in Milne-like spacetimes. Delve into Eric Ling's presentation from the Workshop on "Non-regular Spacetime Geometry" at the Erwin Schrödinger International Institute. Examine the generalization of previous findings to spacetimes with similar geometrical properties to Milne-like spacetimes, without assuming spatial isotropy or homogeneity. Investigate the implications for inflationary scenarios and the early universe's "quasi de Sitter" expansion. Follow the detailed proof structure, including contradiction and intuition approaches, as well as causal theory and strong causality proofs. Gain insights into applications to inflationary theory, the inflationary era, and Freeman's second equation. Consider future research directions, including C0 conformal extension and Freeman equations.

Remarks on the Cosmological Constant as an Initial Condition for Milne-like Spacetimes

Erwin Schrödinger International Institute for Mathematics and Physics (ESI)
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