Paramo

"Vine a Comala porque me dijeron que acá vivía mi padre, un tal Pedro Páramo."

What it does

Paramo stands for: PArticles and RAdiation MOnitor. In a few words: this code solves que Fokker-Planck equation and calculates synchrotron and inverse Compton emission.

Prerequisites

• Fortran (either GNU or Intel)
• HDF5

How to run it

Customize Makefile

The Makefile has a sereies of variables that allow to compile to our convenience.

• COMPILER: 0 for GCC and 1 for Intel compilers
• DEBUGGING: Compile in debugging or optimized mode
• USEHDF5: Compile with HDF5 libraries and save data in that format. NOTE: Not all problems are

Compile and run

• Clone the repository
• Create parameters file
• make
• Run executable

Example

A fast way to run Paramo can be done by downloading/copy the file runGRB190114C.py from the snippets. Running this file will:

• Create the parameters file
• Compile Paramo for an afterglow simulation
• Run the executable

Note: The code can be run from another directory. This can be done by specifying in runGRB190114C.py its full address, as well Paramo's.

References

These are the most referenced works on which I based all the modeling of afterglows

• [PVP14] Pannanen, Vurm, Poutanen, 2014, A&A, 564, A77
• [PM09] Petropoulou, Mastichiadis, 2009, A&A, 507, 599
• [RM92] Rees & Meszaros, 1992, MNRAS, 258, 41P
• [DM09] Dermer & Menon, 2009, "High Energy Radiation from Black Holes: Gamma Rays, Cosmic Rays, and Neutrinos", Princeton Series in Astrophysics
• [SPN98] Sari, Piran, Narayan, 1998, ApJ, 497, L17
• [PK00] Panaitescu & Kumar, 2000, ApJ, 543, 66
• [CL00] Chavalier & Li, 2000, ApJ, 536, 195
• [CD99] Chiang & Dermer, 1999, ApJ, 512, 699