Programs and Data Files Related to Various Publications

Programs and data for the plots in "Infrared Effects and the Unruh State", arXiv:2210.16397

Programs and data for the plots in "Horizons and correlation functions in 2D Schwarzschild-de Sitter Spacetime", JHEP 01 (2022) 192

Programs written by Silvia Pla Garcia for the plots in "Pair production due to an electric field in 1 + 1 dimensions and the validity of the semiclassical approximation", Physical Review D103, 105003 (2021).

Instructions to reproduce the plots

MATLAB files used to reproduce the plots for massive scalar fields

MATLAB files used to reproduce the plots for massive spin 1/2 fields

Programs written by Shohreh Gholizadeh Siahmazgi for some of the plots in "Method to compute the stress-energy tensor for a quantized scalar field when a black hole forms from the collapse of a null shell", Physical Review D102 125035 (2020)

Mathematica notebook for the plots in Figure 3

Mathematica notebook for the plot in Figure 4

Programs for plots generated by Richard Dudley for "Correlations between a Hawking particle and its partner in a 1+1D Bose-Einstein condensate analog black hole ", Physical Review D102, 105005 (2020).

Instructions to reproduce the plots

Files used to reproduce the plots

Program written by Taylor Ordines for some plots in "Semiclassical predictions regarding a preinflationary era and its effects on the power spectrum", Physical Review D102, 063528 (2020)

Programs for plots generated by Richard Dudley for "Particle production in the interiors of acoustic black holes", Physical Review D100, 105021 (2019)

Programs and data for plots in "Late time approach to Hawking radiation: Terms beyond leading order", Physical Review D100, 061703(R) (2019).

Program to compute the plots in Fig. 1. The data files for the plots are named N12D.dat, N22D.dat, and N32D.dat.

Program to compute the data for the plot in Fig. 2. The data file for the plot is named N3b4D.dat.

Programs and Data for "Black hole remnants may exist if Starobinsky inflation occurred", Physical Review D98, 125011 (2018)

Programs for plots generated by Richard Dudley for "Correlation patterns from massive phonons in 1 + 1 dimensional acoustic black holes: A toy model", Physical Review D98, 124011 (2018)

Instructions to reproduce the plots

Files used to reproduce the plots

Programs and Data for "Decay of the de Sitter vacuum", Physical Review D97, 065016 (2018)

Programs and Data for "Future singularities if the universe underwent Starobinsky inflation in the past", Physical Review D95, 044012 (2017)

Programs and Data for "Breakdown of the semiclassical approximation during the early stages of preheating", Physical Review D92, 083522 (2015)

Programs and Data for "Instability of global de Sitter space to particle creation", Physical Review D89, 104038 (2014)

Programs and Data for "On the instability of 'eternal' de Sitter space", Physical Review D89, 104039 (2014)

Mathematic Programs Written by Jason Bates to Compute the Noise Kernel in Schwarzschild spacetime and de Sitter spacetime

Approximations to the Stress-Energy Tensor for Scalar Fields in Static Black Hole Spacetimes

Some of the work referenced on this page was supported in part by the National Science Foundation under grant numbers PHY-1912584, PHY-1505875, PHY-1308325, PHY-0856050, PHY-0556292, PHY-0070981, PHY-9800971, PHY-9512686, PHY-0601550, and PHY-0801368.  Any opinions, findings and conclusions or recomendations expressed in this material are those of the author(s) and do not necessarily reflect the views of the National Science Foundation (NSF).