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>
48 #include<GyotoPageThorneDisk.h>
49 #include<GyotoDirectionalDisk.h>
50 #include<GyotoPatternDisk.h>
51 #include<GyotoPatternDiskBB.h>
52 #include<GyotoDynamicalDisk.h>
53 #include<GyotoDisk3D.h>
54 #include<GyotoFixedStar.h>
55 #include<GyotoInflateStar.h>
56 #include<GyotoStar.h>
57 #include<GyotoDeformedTorus.h>
59 
Geometrically thin disk read from FITS file.
Mass-less, spherical object following a timelike geodesic.
A geometrically thin, optically thick disk.
A geometrically thin, optically thick disk, evolving dynamically.
Astronomical objects (light emitters)
Mass-less, spherical object following a timelike geodesic.
Reference-counting pointers.
Equatorial hot spot.
Slender torus subject to simple time-periodic deformations.
Chern-Simons 1st order perturbation to KerrBL metric.
KerrKS metric.
Timelike or null geodesics.
Base class for metric description.
A geometrically thick, optically thin disk.
KerrBL metric.
A geometrically thin, optically thick disk.
Geometrically thin disks and rings.
A PatternDisk object with possibility to compute a black body spectrum when PatternDiskBB::emission_ ...
GYOTO utilities.
Spherically-symmetric parametrized metric of Rezzolla&Zhidenko 2014 See the paper: PRD...
Error handling.
A single light ray.
Fixed (i.e. non-moving) star.