New #cosmology paper: https://arxiv.org/pdf/1609.01310.pdf

Using a dynamical systems approach to provide a unifying framework for the AdS, Minkowski, and de Sitter universes. #physics #mathematics #science

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# Tag: Physics

## New Cosmology Paper

## Talk today at Perimeter

## The Possible Initial States of The Universe

## 2016 Real-Time Election Predictions

## Protected: Physics, Data, and The 2016 US Elections

## Attempts at a General Einstein Equation for an Arbitrary FLRW Cosmology

## New paper published on cosmological singularities

New #cosmology paper: https://arxiv.org/pdf/1609.01310.pdf

Using a dynamical systems approach to provide a unifying framework for the AdS, Minkowski, and de Sitter universes. #physics #mathematics #science

I have a talk today at Perimeter Institute: here are the slides.

I basically showed that even a stochastic multiverse must be generated by precise initial conditions!

Most people when talking about cosmology typically talk about the universe in one context, that is, as a particular solution to the Einstein field equations. Part of my research in mathematical cosmology is to try to determine whether the present-day universe which we observe to be very close to spatially flat and homogeneous, and very close to isotropic could have emerged from a more general geometric state.

What is often not discussed adequately is the fact that not only has our universe emerged from special initial conditions, but the fact that these special initial conditions also must include the geometry of the early universe, and the type of matter in the early universe. Below, I have attached a simulation that shows how the early universe can evolve to different possible states depending on the type of physical matter parametrized by an equation of state parameter . In particular, some examples are:

- : Vacuum energy
- : Radiation
- : Stiff Fluid

**Note: Click the image below to access the simulation!**

In these simulations, we present phase plots of solutions to the Einstein field equations for spatially homogeneous and isotropic flat, hyperbolic, and closed universe geometries. The different points are:

- dS: de Sitter universe – Inflationary epoch
- M: Milne universe
- F: spatially flat FLRW universe – our present-day universe
- E: Einstein static universe

Note how by changing the value of , the dynamics lead to different possible future states. Dynamical systems people will recognize the problem at hand requires one to determine for which values of is F a saddle or stable node.

Further to my original post on using physics to predict the outcome of the 2016 US Presidential elections, I have now written a cloud-based app using the powerful Wolfram Cloud to pull the most recent polling data on the web from The HuffPost Pollster, which “tracks thousands of public polls to give you the latest data on elections, political opinions and more”. This app works in real-time and applies my PDE-solver / machine learning based algorithm to predict the probability of a candidate winning a state assuming the election is held tomorrow.

The app can be accessed by clicking the image below: (Note: If you obtain some type of server error, it means Wolfram’s server is busy, a refresh usually works. Also, results are only computed for states for which there exists reliable polling data. )

I tried to derive a general Einstein field equation for an arbitrary FLRW cosmology. That is, one that can handle any of the possible spatial curvatures: hyperbolic, spherical, or flat. Deriving the equation was easy, solving it was not! It ends up being a nonlinear, second-order ODE, with singularities at a=0, which turns out to be the Big Bang singularity, which obviously is of physical significance. Anyways, here’s a log of my notebook, showing the attempts. More to follow!

My new paper has now been published in Annalen der Physik, which is a great honour, because 100 years ago, Einstein’s General Theory of Relativity was also published in the same journal.

This paper describes a method by which one is able to determine whether a given spatially flat cosmological model produces finite-time singularities, and also gives some examples of interesting cosmological model configurations.

The paper can be accessed by clicking the image below:

The preprint can be accessed here on the arXiv.