#include <Windaccretion.h>
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| typedef std::map< std::string, size_t > | _PrintMap |
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| | WindaccretionDisabled (_UNUSED IO *_io=nullptr, bool reg=true) |
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| std::string | name () override |
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| WindaccretionDisabled * | instance () override |
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| int | evolve (_UNUSED Binstar *binstar) override |
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| bool | is_process_ongoing () const override |
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| Windaccretion * | Instance (_UNUSED IO *_io) override |
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| virtual double | DA (_UNUSED Binstar *b, _UNUSED int procID) |
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| virtual double | DE (_UNUSED Binstar *b, _UNUSED int procID) |
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| virtual double | NS_DBmag_accretion (_UNUSED Binstar *b, _UNUSED Star *s, _UNUSED double DM) const |
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| virtual double | NS_DOmegaRem_accretion (_UNUSED Binstar *b, _UNUSED Star *s, _UNUSED double DM) const |
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| virtual int | special_evolve (_UNUSED Binstar *binstar) |
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| double | get (const size_t &id) |
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| double | get_var (const size_t &starID, const size_t &propID) |
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| std::string & | get_msg () |
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| void | restore () |
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| int | modify_SemimajorDV_by_a_factor (double factor) |
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| int | modify_EccentricityDV_by_a_factor (double factor) |
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| bool | is_mass_transfer_happening () |
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| void | set_event (double code) |
| | Events handling. More...
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| double | get_event () |
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| void | reset_event () |
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| void | special_evolution_alarm_switch_on () |
| | Three methods to handle the private member special_evolution_alarm. More...
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| void | special_evolution_alarm_switch_off () |
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| bool | is_special_evolution_alarm_on () const |
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| virtual double | estimate_accreted_mass (_UNUSED double DM, _UNUSED Star *donor, _UNUSED Star *accretor, _UNUSED Binstar *binstar) const |
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◆ _PrintMap
◆ WindaccretionDisabled()
| WindaccretionDisabled::WindaccretionDisabled |
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_UNUSED IO * |
_io = nullptr, |
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bool |
reg = true |
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) |
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inline |
◆ accrete_mass()
| virtual int MaccretionProcess::accrete_mass |
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_UNUSED Binstar * |
binstar | ) |
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inlineprotectedvirtualinherited |
Function in which the mass accretion is handled. This function should take care of changing all the single stellar evolution properties (not only the mass) The change of binary parameters such as Semimajor axis and Eccentricity are instead changed inside evolve using the methods DA and DE.
- Parameters
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| binstar | Pointer to the binary star |
- Returns
- EXIT SUCCESS
◆ DA()
◆ DE()
◆ estimate_accreted_mass()
Public interface to allow the user to get information without actually evolving the systems. NOTICE: to be self-consistent the protected and private methods (such DA and DE should use these methods) when changing the properties of stars and binaries. This function should be an interface for the user to return the amount of mass accreted on the accretor given the binary, the donor and the available amount of mass DM. NOTICE: internally the accrete mass should use this method to be self-consistent
- Parameters
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| DM | amount of mass available to be accreted in Msun. |
| donor | Pointer to the Star that is donating the mass |
| accretor | Pointer to the star that is receiving the mass |
| binstar | Pointer to the binary system hosting the donor and the accretore |
- Returns
- the amount of accreted mass
Reimplemented in WindaccretionHurley.
◆ evolve()
◆ get()
| double Process::get |
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const size_t & |
id | ) |
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inlineinherited |
◆ get_event()
| double Process::get_event |
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inlineinherited |
◆ get_msg()
| std::string & Process::get_msg |
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inlineinherited |
◆ get_var()
| double Process::get_var |
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const size_t & |
starID, |
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const size_t & |
propID |
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) |
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inlineinherited |
◆ GetStaticMap()
| static std::map< std::string, Windaccretion * > & Windaccretion::GetStaticMap |
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inlinestaticprotectedinherited |
◆ GetUsed()
| static std::vector< int > & Windaccretion::GetUsed |
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inlinestaticprotectedinherited |
◆ handle_NS_massaccretion()
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protectedvirtualinherited |
It is a wrapper of all the necessray function calls to set the DV of NS properties after mass accretion
- Parameters
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| s | Pointer to the ns star |
| dM | Mass accreted in Msun |
◆ instance()
◆ Instance()
◆ is_mass_transfer_happening()
| bool Process::is_mass_transfer_happening |
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| ) |
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inlineinherited |
Check if this process is changing the mass
- Returns
- false if the DV regarding the Mass of both stars is currently set to 0, true otherwise
◆ is_process_ongoing()
| bool WindaccretionDisabled::is_process_ongoing |
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| ) |
const |
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inlineoverridevirtual |
Check if the current process is ongoing
- Returns
- true if the process is ongoing, false otherwise
Reimplemented from Windaccretion.
◆ is_special_evolution_alarm_on()
| bool Process::is_special_evolution_alarm_on |
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| ) |
const |
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inlineinherited |
◆ modify_EccentricityDV_by_a_factor()
| int Process::modify_EccentricityDV_by_a_factor |
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double |
factor | ) |
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inlineinherited |
Correct the VB cell containing the Eccentricity variation
- Parameters
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| factor | correction factor the new DE will be DE*factor. |
- Returns
- EXIT_SUCCESS
◆ modify_SemimajorDV_by_a_factor()
| int Process::modify_SemimajorDV_by_a_factor |
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double |
factor | ) |
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inlineinherited |
Correct the VB cell containing the Semimajor variation
- Parameters
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| factor | correction factor the new DA will be DA*factor. |
- Returns
- EXIT_SUCCESS
◆ name()
| std::string WindaccretionDisabled::name |
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| ) |
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inlineoverridevirtual |
◆ NS_DBmag_accretion()
This function estimate the increment or decrement of NS Bmag due do the accretion of material
- Parameters
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| s | Pointer to the star that is accreting |
| dM | Mass accreted in Msun |
- Returns
- THe difference in Bmag after accretion
Checks
◆ NS_DOmegaRem_accretion()
This function estimate the increment or decrement of NS angular velocity OmegaRem due do the accretion of material
- Parameters
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| s | Pointer to the star that is accreting |
| dM | Mass accreted in Msun |
- Returns
- THe difference in OmegaRem after accretion
Checks
◆ Register()
| void Process::Register |
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Process * |
_p, |
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size_t * |
id, |
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const std::string & |
_name |
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) |
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inlineprotectedinherited |
◆ Register_specific()
| static void Windaccretion::Register_specific |
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Windaccretion * |
ptr | ) |
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inlinestaticprotectedinherited |
◆ reset_event()
| void Process::reset_event |
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inlineinherited |
◆ restore()
| void Process::restore |
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inlineinherited |
◆ set()
| void Process::set |
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const size_t & |
id, |
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const double & |
value |
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) |
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inlineprotectedinherited |
◆ set_event()
| void Process::set_event |
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double |
code | ) |
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inlineinherited |
◆ set_msg()
| void Process::set_msg |
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const std::string & |
str | ) |
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inlineprotectedinherited |
◆ set_V_to_0()
| void Process::set_V_to_0 |
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inlineprotectedinherited |
◆ set_var()
| void Process::set_var |
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const size_t & |
starID, |
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const size_t & |
propID, |
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const double & |
value |
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) |
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inlineprotectedinherited |
◆ special_evolution_alarm_switch_off()
| void Process::special_evolution_alarm_switch_off |
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inlineinherited |
◆ special_evolution_alarm_switch_on()
| void Process::special_evolution_alarm_switch_on |
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inlineinherited |
Three methods to handle the private member special_evolution_alarm.
◆ special_evolve()
◆ _uniform_real
| std::uniform_real_distribution<double> Process::_uniform_real |
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protectedinherited |
◆ _windaccretion
Initialisation of the static (fake) instance NB: take care of the order of initialisation. The processes will be evolved exactly in the same order in which they are initialised here
◆ _windaccretiondisabled
◆ accretor
| Star* Process::accretor = nullptr |
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protectedinherited |
◆ all
| std::vector< Process * > Process::all |
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staticinherited |
◆ alphaw
| double Windaccretion::alphaw |
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protectedinherited |
Bondi-Hoyle accretion parameter (Eq. 6, Hurley+02)
◆ betaw
| double Windaccretion::betaw |
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protectedinherited |
Wind escape velocity parameter (Eq. 9, Hurley+02)
◆ donor
| Star* Process::donor = nullptr |
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protectedinherited |
◆ event_code
| double Process::event_code =-1 |
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privateinherited |
◆ ID
◆ message
| std::string Process::message |
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privateinherited |
◆ muw
| double Windaccretion::muw |
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protectedinherited |
Angular momentum transfer efficiency (Eq. 11, Hurley+02)
◆ NO_WINDACCRETION
| constexpr int Windaccretion::NO_WINDACCRETION = 0 |
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staticconstexprinherited |
◆ orb_change
◆ PrintMap
◆ size
Instruction for adding new property PROC 1- Add the size_t PROC::ID 2- Initialise the static (fake) instance PROC PROC::_proc. NB: take care of the order of initialisation. The processes will be evolved exactly in the same order in which they are initialised here Define: @size: total number of instances of Process and derived classes (both fake and real). @all: vector containing all the (pointers) to the processes. @PrintMap: map containing the pair (process_name, process_id) for output purpose. Note all and PrintMap are filled during the instantiation of the fake Processes (see below)
◆ special_evolution_alarm
| bool Process::special_evolution_alarm =false |
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privateinherited |
Member used to check if a special evolution is required
◆ svlog
◆ VB
| std::vector<double> Process::VB |
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privateinherited |
values of the properties of the binary system (e.g. processes change eccentricity, semimajor...)
◆ VS
| std::vector<std::vector<double> > Process::VS |
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privateinherited |
variations of the single star parameters due to binary stellar evolution processes (e.g. mass, radius...)
The documentation for this class was generated from the following files: