Gyoto
Gyoto.h
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1/*
2 Copyright 2011-2016, 2018-2019 Thibaut Paumard, Frédéric Vincent,
3 Éric Gourgoulhon
4
5 This file is part of Gyoto.
6
7 Gyoto is free software: you can redistribute it and/or modify
8 it under the terms of the GNU General Public License as published by
9 the Free Software Foundation, either version 3 of the License, or
10 (at your option) any later version.
11
12 Gyoto is distributed in the hope that it will be useful,
13 but WITHOUT ANY WARRANTY; without even the implied warranty of
14 MERCHANTABILITY or FITNESS FOR A PARTICULAR PURPOSE. See the
15 GNU General Public License for more details.
16
17 You should have received a copy of the GNU General Public License
18 along with Gyoto. If not, see <http://www.gnu.org/licenses/>.
19 */
20
34#include<GyotoUtils.h>
35#include<GyotoError.h>
36#include<GyotoSmartPointer.h>
37#include<GyotoWorldline.h>
38#include<GyotoPhoton.h>
39
40#include<GyotoMetric.h>
41#include<GyotoKerrBL.h>
42#include<GyotoKerrKS.h>
43#include<GyotoChernSimons.h>
45
46#include<GyotoAstrobj.h>
47#include<GyotoThinDisk.h>
50#include<GyotoPatternDisk.h>
53#include<GyotoDisk3D.h>
54#include<GyotoFixedStar.h>
55#include<GyotoInflateStar.h>
56#include<GyotoStar.h>
59
Astronomical objects (light emitters)
Chern-Simons 1st order perturbation to KerrBL metric.
Slender torus subject to simple time-periodic deformations.
Geometrically thin disk read from FITS file.
A geometrically thick, optically thin disk.
A geometrically thin, optically thick disk, evolving dynamically.
Equatorial hot spot.
Error handling.
Fixed (i.e. non-moving) star.
Mass-less, spherical object following a timelike geodesic.
KerrBL metric.
KerrKS metric.
Base class for metric description.
A geometrically thin, optically thick disk.
A geometrically thin, optically thick disk.
A PatternDisk object with possibility to compute a black body spectrum when PatternDiskBB::emission_ ...
A single light ray.
Spherically-symmetric parametrized metric of Rezzolla&Zhidenko 2014 See the paper: PRD,...
Reference-counting pointers.
Mass-less, spherical object following a timelike geodesic.
Geometrically thin disks and rings.
GYOTO utilities.
Timelike or null geodesics.