Planetary Orbital Evolution due to Tides
Orbital evolution of two objects experiencing tides
IOColumns.h
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7 #ifndef __IO_COLUMNS_H
8 #define __IO_COLUMNS_H
9 
10 #include <vector>
11 #include <string>
12 
14 namespace InCol {
17  enum InputColumns {
21  WINDK=0,
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44 
45 #ifdef TWO_QS
46  LGQ,
47  LGQ_INERTIAL,
48 #else
49  LGQ,
52 #endif
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68  TEND,
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99  };
100 };
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103 namespace OutCol {
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170  LORB,//< The orbital angular momentum
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223  };
224 };
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227 const std::vector<std::string> &output_column_names();
228 
229 #endif
The number of real values quantities.
Definition: IOColumns.h:86
The number of different output quantities supported.
Definition: IOColumns.h:222
Age in Myr when disk dissipates.
Definition: IOColumns.h:62
powerlaw index of Q* dependence.
Definition: IOColumns.h:50
Wind saturation frequency in rad/day.
Definition: IOColumns.h:25
Second derivative of the moment of inertia of the entire star.
Definition: IOColumns.h:158
The orbital periapsis in the reference frame of the stellar radiative zone in radians.
Definition: IOColumns.h:186
Spin period of the stellar surface in days.
Definition: IOColumns.h:208
The evolution mode for the step that starts at this age.
Definition: IOColumns.h:217
Age derivative of the convective moment of inertia in .
Definition: IOColumns.h:130
Second derivative of the moment of ivertia of the radiative zone.
Definition: IOColumns.h:155
Orbital period in days at which the planet forms.
Definition: IOColumns.h:64
Age derivative of the stellar radius in .
Definition: IOColumns.h:141
The name of the file to write the evolution to.
Definition: IOColumns.h:83
Angular velocity of the stellar surface in rad/day.
Definition: IOColumns.h:202
Age derivative of the moment of inertia of the entire star in .
Definition: IOColumns.h:138
The orbital frequency in rad/day.
Definition: IOColumns.h:168
The number of real valued output quantities.
Definition: IOColumns.h:214
Second derivative of the core-envelope boundary.
Definition: IOColumns.h:161
The maximum age to stop the evolution at in Gyr.
Definition: IOColumns.h:68
The orbital period days.
Definition: IOColumns.h:169
Eccentricity at which the planet forms.
Definition: IOColumns.h:65
Angular momentum of the radiative zone of the star in (low mass stars only)
Definition: IOColumns.h:196
Second derivative of the moment of ivertia of the convective zone.
Definition: IOColumns.h:152
SEMIMAJOR
The derivative w.r.t. the semimajor axis in AU.
The angle between the stellar core spin and orbital angular momentum in radians.
Definition: IOColumns.h:178
The angle between the stellar surface spin and orbital angular momentum in radians.
Definition: IOColumns.h:174
Radius of the planet in Jupiter radii.
Definition: IOColumns.h:55
Inclination with which the planet forms.
Definition: IOColumns.h:66
Spin period of the stellar core in days (low mass stars only).
Definition: IOColumns.h:211
Should the evolution start with the stellar surface spinning synchronously with the orbit...
Definition: IOColumns.h:90
Lg(Q*) at tidal frequency of 1 day.
Definition: IOColumns.h:49
Angular velocity of the stellar core in rad/day (low mass stars only).
Definition: IOColumns.h:206
Isolates the tags for the output columns.
Definition: IOColumns.h:103
Isolates the tags for the input columns.
Definition: IOColumns.h:14
Semimajor axis at which the planet forms in AU.
Definition: IOColumns.h:63
Age derivative of the mass of the radiative core in .
Definition: IOColumns.h:149
Angular momentum of the entire star in .
Definition: IOColumns.h:200
Stellar surface spin while disk is present in rad/day.
Definition: IOColumns.h:57
Wind saturation period in days for low mass stars.
Definition: IOColumns.h:36
Age derivative of the radiative moment of inertia in .
Definition: IOColumns.h:134
Angular momentum of the convective zone of the star in (low mass stars only)
Definition: IOColumns.h:191
Radius of the star in .
Definition: IOColumns.h:119
The wind strength for high mass stars.
Definition: IOColumns.h:24
InputColumns
Tags for the quantities required to fully specify the system to evolve.
Definition: IOColumns.h:17
A column which is not needed to calculate the evolution.
Definition: IOColumns.h:95
Stellar surface rotation period in days while disk is present.
Definition: IOColumns.h:60
The maximum timestep to take.
Definition: IOColumns.h:78
Wind strength in .
Definition: IOColumns.h:21
ECCENTRICITY
The derivative w.r.t. the eccentricity.
Moment of inertia of the radiative zone of the star (low mass stars only) in .
Definition: IOColumns.h:114
A list of ages guaranteed to be included in the tabulated orbit.
Definition: IOColumns.h:93
AGE
The derivative w.r.t. age, excluding the dependence through the body&#39;s radius and the moments of iner...
The minimum age to start evolution at in Gyr.
Definition: IOColumns.h:67
Moment of inertia of the convective zone of the star (low mass stars only) in .
Definition: IOColumns.h:110
Wind saturation frequency in rad/day for low mass stars.
Definition: IOColumns.h:28
The saturation state of the wind.
Definition: IOColumns.h:219
Wind saturation frequency in rad/day for high mass stars.
Definition: IOColumns.h:31
The number of different input quantities supported.
Definition: IOColumns.h:98
Wind saturation period in days for high mass stars.
Definition: IOColumns.h:39
Wind saturation period in days.
Definition: IOColumns.h:33
Lg(Q*) outside the inertial mode range.
Definition: IOColumns.h:51
Initial rotation of the radiative core in rad/day if the evolution starts after the core has formed...
Definition: IOColumns.h:72
Luminosity of the star in .
Definition: IOColumns.h:120
Radius of the stellar core in (low mass stars only).
Definition: IOColumns.h:123
OutputColumns
Tags for the possible columns to output.
Definition: IOColumns.h:105
The orbital periapsis in the reference frame of the stellar convective zone in radians.
Definition: IOColumns.h:182
The index of the last quantity requiring no orbital evolution.
Definition: IOColumns.h:164
Mass of the star in .
Definition: IOColumns.h:53
The number of significant figures require of the evolution.
Definition: IOColumns.h:81
Age when planet appears in Gyr.
Definition: IOColumns.h:56
Surface rotation of the star in rad/day if the evolution starts after the disk has dissipated...
Definition: IOColumns.h:76
Mass of the stellar core in (low mass stars only).
Definition: IOColumns.h:126
Mass of the planet in Jupiter masses.
Definition: IOColumns.h:54
The wind strength for low mass stars.
Definition: IOColumns.h:23
Core-envelope coupling timescale in Myr, ignore for high mass stars.
Definition: IOColumns.h:43
const std::vector< std::string > & output_column_names()
Define the names of the output columns.
Definition: IOColumns.cpp:3
Total moment of inertia of the star in .
Definition: IOColumns.h:117