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2 votes
0 answers
54 views

Cosmological numerical computations

I am unsure where to ask this question, whether here or in the Mathematica stackexchange, but either way, I was wondering what are some recommendations for cosmological computations specifically using ...
0 votes
0 answers
18 views

Computing matter power spectrum using FFT

I have a 3-dimensional density field from a big N-body simulation, and I would like to compute the matter power spectrum $P(k)$ to see how it compares with the one observed by Planck etc. I know that ...
Frogfire's user avatar
  • 157
2 votes
0 answers
70 views

Initial condition of the millenium simulation

I would like to know the initial conditions used for the millenium simulation. More specifically, I would like to know the amplitude of the initial power spectrum $\mathcal{A}$. I have found the ...
konstle's user avatar
  • 758
1 vote
0 answers
49 views

Numerical evolution of Einstein-Boltzmann equations for cold dark matter

I'm trying to numerically evolve the Einstein-Boltzmann equations for cold dark matter perturbations using Runge-Kutta method of the fourth order. There are 5 standard equations: \begin{align} \dot{\...
hidenori's user avatar
1 vote
1 answer
94 views

Solve the perturbed Boltzmann Einstein equations in cosmology using RK4 method

I'm trying to learn to numerically solve the perturbed Boltzmann-Einstein equations in cosmology using the RK4 method. These are the equations: \begin{align} \dot{\Theta}_{r,0}+k\Theta_{r,1}&=-\...
hidenori's user avatar
1 vote
1 answer
52 views

Supernovae apparent magnitude in a simplified LCDM model

I want to generate some fake apparent magnitude of supernovae Ia at different redshift using the LCDM model and the fiducial absolute magnitude of supernovae Ia (-19.35) and I want to compare it with ...
Alucard's user avatar
  • 299
1 vote
0 answers
145 views

Smoothing a density field in Python [closed]

I want to smooth a density field. It's represented as a contour plot. The data were given from a 3d array. A smoothed field should be periodic but what I take does not have periodicity. The code I use ...
Manos Bougioukoglou's user avatar
0 votes
1 answer
55 views

Astropy Package - Defining new dark energy parametrization

I was looking through astropy, and I wonder is it possible to define a new dark energy parametrization instead of using the pre-defined ones..? I couldn't see the reference but maybe I missed it. ...
seVenVo1d's user avatar
  • 3,122
3 votes
1 answer
157 views

Cosmology context - MCMC code : Recomputation of covariance matrix after each point accepted

I am working on a MCMC code (basically with Metropolis-Hastings) and I would like to understand different important points. We always mention the covariance matrix which is used in the computation of ...
user avatar
0 votes
1 answer
163 views

Numerical solution to the equation of curvature perturbation

Numerical solution to Mukhanov-Sasaki equation In the above link, an equation is given which is the evolution equation of curvature perturbation as a function of $N$ (number of e-folds). In order to ...
CosmoTM's user avatar
  • 21
0 votes
1 answer
693 views

How do I convert a .FITS into a numpy array (or a file that can be used in Python)? [closed]

I'm trying to train an AI algorithm to determine photometric redshifts of galaxies, and to do so I have a .FITS file which contains the training data. I need to convert this .FITS file into a format ...
Lara's user avatar
  • 11
0 votes
1 answer
123 views

Numerical solution to background equations of cosmology

I am trying to solve the background equations of cosmology numerically using Runge-Kutta Dormand prince method with simplified assumption $8\pi G=1$ and $c=1$. The equations are $$ \ddot a = -\frac{1}{...
Dori's user avatar
  • 31
1 vote
0 answers
82 views

Numerical code Friedmann equations [closed]

I have to write a numerical code to solve the ‘Ω-form’ of the Friedmann equation: H(t)^2/H_0^2 = Ωmat/a^3 + Ωrad/a^4 + Ωk/a^2 + Ωx/a^3(1+w) ...
Pien's user avatar
  • 11
0 votes
0 answers
43 views

Numerically solving the equation of motion for inflation in cosmology

So I want to solve the equation of inflation involving a scalar field numerically using python libraries such as odient or scipy. The equation is: $$\def\phi{\varphi} \phi''(t)+3H\phi'(t)+V'(\phi(t))=...
user14491798's user avatar
2 votes
0 answers
41 views

Why is the boundary of friends-of-friends (FOF) halo corresponding to iso-density contour?

The friends-of-friends algorithm (hereafter FOF) is commonly used to find halos in cosmological simulations. (For more information, please refer to here and here) I found that some literature argues ...
Wang Yun's user avatar
  • 529

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