Skip to content

Code for simulating inflation, including Lagrangians with non-canonical kinetic energy.

License

Notifications You must be signed in to change notification settings

maxitg/InflationSimulator

Folders and files

NameName
Last commit message
Last commit date

Latest commit

 

History

29 Commits
 
 
 
 
 
 
 
 
 
 
 
 
 
 

Repository files navigation

Inflation Simulator

Code for simulating inflation, including multiple field Lagrangians with non-canonical kinetic energy.

Overview

To demonstrate some functionality of the package, let's consider a two-field potential with a saddle point:

image

image

We can obtain equations of motion for this potential by using InflationEquationsOfMotion:

image

Here n[t] stands for the number of e-foldings. We can use these equations to produce an evolution of the fields and the number of e-foldings over time, starting for example with initial conditions a[0] = 5, a'[0] = 0, b[0] = 0.2, b'[0] = 0 using InflationEvolution:

image

We get InterpolatingFunctions and some extra information such as the total number of e-foldings. If we plot evolution of the fields over time, we can see that the fields reach the saddle point, and "slow-roll" through it for some time:

image

Let's plot that against the potential to see the trajectory of the fields:

image

We can check if this particular model is consistent with experimental constraints. One way to do that is to evaluate the ratio of tensor-to-scalar power spectra, and the scalar spectral index, assuming horizon exit for the scale we see today occured 60 e-foldings before the end of inflation:

image

Let's check if that's in experimental range:

image

What if we change the initial value of b? Let's plot the scalar spectral index against it:

image

It appears we can get experimentally allowed values near b[0] = 0.05. Let's try it:

image

It is consistent! So, we have found an inflation model (albeit with a non-physical potential) that is consistent with experimental constraints on scalar spectral index and tensor-to-scalar ratio.

Build

  1. Open the project in Wolfram Workbench using File -> Open Projects from File System..., and selecting root repository directory.
  2. Open Window -> Show View -> Application Tools.
  3. Select InflationSimulator as a project.
  4. Click Build to build documentation.
  5. Click Deploy Application, and select a directory to put a temporary deployed package.
  6. Make sure all files selected, click Next. Make sure documentation is selected, click Finish. A new directory InflationSimulator will be created in a directory specified.
  7. Open Mathematica, and evaluate PacletManager`PackPaclet["path_to_newly_created_InflationSimulator_directory"]. The output will be the path to the compiled paclet.

Install

Evaluate PacletManager`PacletInstall["path_to_paclet"], where path_to_paclet is the path to the .paclet file, which can either be downloaded from releases page, or build using the steps above.

About

Code for simulating inflation, including Lagrangians with non-canonical kinetic energy.

Topics

Resources

License

Stars

Watchers

Forks

Packages

No packages published