SEVN: Hurley_mod_rl Class Reference

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#include <Orbit.h>

Inheritance diagram for Hurley_mod_rl:

Public Member Functions
	Hurley_mod_rl (bool reg=true)

Hurley_mod_rl *	instance () override

std::string	name () override

void	init (_UNUSED Binstar *b) override

double	DA (_UNUSED Binstar *b, _UNUSED int procID) override

double	DE (_UNUSED Binstar *b, _UNUSED int procID) override

double	DAngMomSpin (_UNUSED Binstar *b, _UNUSED int procID, _UNUSED int starID) override

void	set_options (IO *_io) override

virtual void	set_options (_UNUSED IO *_io)

int	speciale_evolve (_UNUSED Binstar *b) override
	Mass transfer. More...

double	get_DM (int ID)

double	DM (_UNUSED Binstar *b, _UNUSED int procID, _UNUSED int starID) override

bool	is_swallowed (int starID)

bool	is_process_ongoing () override
	Other function that return useful information. More...

bool	is_colliding ()

Static Public Member Functions
static Orbital_change_RL *	Instance (const std::string &name)

Public Attributes
bool	novae =false

bool	super_eddington =false

Static Public Attributes
static Hurley_mod_rl	_Hurley_mod_rl

static Hurley_rl	_Hurley_rl

Protected Member Functions
void	set_orbital (_UNUSED Binstar *b) override

void	init_common_variable (Star donor_star, Star accretor_star, Binstar *b)

bool	check_doubleRLO (Binstar *b)
	AUX. More...

bool	check_collision_at_periastron (Star donor, Star accretor, Binstar *b)

int	outcome_double_RLO (_UNUSED Binstar *b) override

int	outcome_collision (_UNUSED Binstar *b) override

int	outcome_collision (Star donor, Star accretor, _UNUSED Binstar *b) override

virtual int	outcome_collision (_UNUSED Star donor, _UNUSED Star accretor, _UNUSED Binstar *b)

void	RLO (_UNUSED Binstar *b)

virtual void	RLO (_UNUSED Star donor, _UNUSED Star accretor, _UNUSED Binstar *b)

double	dynamic_dmdt (_UNUSED Star s, _UNUSED Binstar b) override
	Mass transfer. More...

double	nuclear_dmdt (_UNUSED Star s, _UNUSED Binstar b) override

double	thermal_dmdt (_UNUSED Star s, _UNUSED Binstar b) override

int	dynamic_swallowing (_UNUSED Binstar *b) override

double	thermal_nuclear_accreted_mass (_UNUSED double DM_donor, _UNUSED Star donor, _UNUSED Star accretor, _UNUSED Binstar *b) override

double	fRL_radius (_UNUSED Star star, _UNUSED Binstar b) override

Star *	get_donor ()

Star *	get_accretor ()

double	get_rldonor ()

void	set_DA (double DA)

void	set_DE (double DE)

double	get_mt_value () const override

double	get_mt_tshold () const override

void	Register (Orbital_change_RL *ptr, const std::string &_name)

virtual double	correct_accreted_mass (double DM_accreted, _UNUSED double DM_donor, _UNUSED Star donor, _UNUSED Star accretor, _UNUSED Binstar *b)

int	set_DM (double DM, int starID)

int	reset_DM ()

int	set_swallowed (int starID)

int	reset_swallowed (int starID)

int	reset_swallowed ()

void	set_mix ()

void	unset_mix ()

bool	get_mix ()

void	set_comenv ()

void	unset_comenv ()

bool	get_comenv ()

void	set_is_RLO_happening ()

void	unset_is_RLO_happening ()

void	set_is_colliding ()

void	unset_is_colliding ()

virtual double	estimate_q (Star donor, Star accretor)
	q stuff More...

virtual double	Hfrac (Star *s)

virtual double	dMdt_eddington (Star donor, Star accretor, Binstar *b)

bool	is_giant_like (int star_type_bse)

virtual double	kelvin_helmotz_tscale (Star *s)
	time scales More...

virtual double	dynamic_tscale (Star *s)

virtual int	check_compact_accretor (int donor_type_bse, int accretor_type_bse)
	Checks. More...

Protected Attributes
Star *	donor

Star *	accretor

int	star_type1 = utilities::NULL_INT

int	star_type2 = utilities::NULL_INT

double	frl1 = utilities::NULL_DOUBLE

double	rl1 = utilities::NULL_DOUBLE

bool	is_RL_in_core = false

double	mt_value = utilities::NULL_DOUBLE

double	mt_tshold = utilities::NULL_DOUBLE

double	f_MT = utilities::NULL_DOUBLE
	Accretion efficency. More...

double	dmdt_edd = utilities::NULL_DOUBLE

double	dt = utilities::NULL_DOUBLE
	Times. More...

double	tkh1 = utilities::NULL_DOUBLE

double	tdyn1 = utilities::NULL_DOUBLE

double	taum = utilities::NULL_DOUBLE

double	tkh2 = utilities::NULL_DOUBLE

double	_DA = 0

double	_DE = 0

double	_DLspin [2] ={0.,0.}

MTstability *	mt_stability

SevnLogging	svlog

Static Private Member Functions
static std::map< std::string, Orbital_change_RL * > &	GetStaticMap ()

static std::vector< int > &	GetUsed ()

Private Attributes
double	_DM [2] ={0,0}

bool	_is_swallowed [2] ={false, false}

bool	mix = false

bool	comenv = false

bool	_is_RLO_happening =false

bool	_is_colliding =false

Constructor & Destructor Documentation

◆ Hurley_mod_rl()

Hurley_mod_rl::Hurley_mod_rl ( bool reg = true )

inline

Member Function Documentation

◆ check_collision_at_periastron()

bool Hurley_rl::check_collision_at_periastron	(	Star *	donor,
		Star *	accretor,
		Binstar *	b
	)

protectedinherited

Check if both stars are colliding at the periastron. The outcome of this two events can be a Mix or a CE.

Parameters

b	Pointer to the binary

Returns: true if one of two conditions is fulfilled

◆ check_compact_accretor()

virtual int Orbital_change_RL::check_compact_accretor	(	int	donor_type_bse,
		int	accretor_type_bse
	)

inlineprotectedvirtualinherited

Checks.

Check that for compact remnants (WD,NS,BH) the accretor is as compact or more compact with respect to the donor.

Parameters

donor_type_bse	BSE type of the donor
accretor_type_bse	BSE type of the accretor

Returns: EXIT_SUCCESS or throw an error

Exceptions

sevnstd::rl_error

◆ check_doubleRLO()

bool Hurley_rl::check_doubleRLO ( Binstar * b )

protectedinherited

AUX.

Aux.

Check if both stars are filling the RL The outcome of this two events can be a Mix or a CE.

Parameters

b	Pointer to the binary

Returns: true if one of two conditions is fulfilled

◆ correct_accreted_mass()

virtual double Orbital_change_RL::correct_accreted_mass	(	double	DM_accreted,
		_UNUSED double	DM_donor,
		_UNUSED Star *	donor,
		_UNUSED Star *	accretor,
		_UNUSED Binstar *	b
	)

inlineprotectedvirtualinherited

General function to be called to correct the accreted mass for whatever reason. In this general version it just returns the same amount of DM_accreted in input. The idea is that specialised version of this process could need to add special correction without change the rest of the process.

Parameters

DM_accreted	mass accreted by the accretor (before this correction) in Msun
DM_donor	mass donated by the donor in Msun
donor	Pointer to the star that is overflowing the RocheLobe
accretor	Pointer to the star that is accreting mass
b	Pointer to the binary

Reimplemented in Hurley_rl_propeller.

◆ DA()

double Hurley_rl::DA	(	_UNUSED Binstar *	b,
		_UNUSED int	procID
	)

overridevirtualinherited

Reimplemented from Orbital_change.

◆ DAngMomSpin()

double Hurley_rl::DAngMomSpin	(	_UNUSED Binstar *	b,
		_UNUSED int	procID,
		_UNUSED int	starID
	)

overridevirtualinherited

Reimplemented from Orbital_change.

◆ DE()

double Hurley_rl::DE	(	_UNUSED Binstar *	b,
		_UNUSED int	procID
	)

overridevirtualinherited

Variation of Eccentricity. In BSE derived from Hurley+20, the eccentricity is set to 0 at onset of RLO. In order to take this into account we set the DE to a large negative value so that e<0 and in the subsequent checks it is forced to 0.

Parameters

b	Pointer to binary
procID	ID of process calling DE.

Returns

Reimplemented from Orbital_change.

◆ DM()

double Orbital_change_RL::DM	(	_UNUSED Binstar *	b,
		_UNUSED int	procID,
		_UNUSED int	starID
	)

inlineoverridevirtualinherited

Reimplemented from Orbital_change.

◆ dMdt_eddington()

double Orbital_change_RL::dMdt_eddington	(	Star *	donor,
		Star *	accretor,
		Binstar *	b
	)

protectedvirtualinherited

Estimate the rate of mass transfer considering the Eddington limit

Parameters

donor	Star that is donating mass through the RLO
accretor	Star that is accreting mass

Returns

◆ dynamic_dmdt()

double Hurley_rl::dynamic_dmdt	(	_UNUSED Star *	s,
		_UNUSED Binstar *	b
	)

overrideprotectedvirtualinherited

Mass transfer.

Rate of dynamic mass transfer from Eq. 62 in Hurley+2002

Parameters

s	pointer to the Star that is losing mass
b	pointer to the binary

Returns: dm/dt

Reimplemented from Orbital_change_RL.

◆ dynamic_swallowing()

int Hurley_rl::dynamic_swallowing ( _UNUSED Binstar * b )

overrideprotectedvirtualinherited

Function that handle the situation in which the mass transfer is dynamic unstable but the stars are not mixing or doing a ce. Note in that case we use the current stellar properties (after single and binary evolution) not the properties at time 0.

Parameters

b	Pointer to the binary

Returns: EXIT_SUCCESS;

Reimplemented from Orbital_change_RL.

Reimplemented in Hurley_rl_bse.

◆ dynamic_tscale()

double Orbital_change_RL::dynamic_tscale ( Star * s )

protectedvirtualinherited

Dynamic time scale (Eq. 63, Hurley+2002) Directly taken from SEVN1

Parameters

s	Pointer to star

Returns: Dynamic time scale in yr

◆ estimate_q()

double Orbital_change_RL::estimate_q	(	Star *	donor,
		Star *	accretor
	)

protectedvirtualinherited

q stuff

Simply estimate the mass fraction of the donor over the accretor

Parameters

donor	Star that is donating mass through the RLO
accretor	Star that is accreting mass

Returns: mass_fraction

◆ fRL_radius()

double Hurley_rl::fRL_radius	(	_UNUSED Star *	star,
		_UNUSED Binstar *	b
	)

overrideprotectedvirtualinherited

Roche Lobe radius normalised over the star radius

Parameters

star	pointer to the star for which we are estimateting fRL
b	pointer to the binary

Returns: R_rl/R_star

Reimplemented from Orbital_change_RL.

◆ get_accretor()

Star * Hurley_rl::get_accretor ( )

inlineprotectedinherited

◆ get_comenv()

bool Orbital_change_RL::get_comenv ( )

inlineprotectedinherited

◆ get_DM()

double Orbital_change_RL::get_DM ( int ID )

inlineinherited

◆ get_donor()

Star * Hurley_rl::get_donor ( )

inlineprotectedinherited

Returns

◆ get_mix()

bool Orbital_change_RL::get_mix ( )

inlineprotectedinherited

◆ get_mt_tshold()

double Hurley_rl::get_mt_tshold ( ) const

inlineoverrideprotectedvirtualinherited

Reimplemented from Orbital_change_RL.

◆ get_mt_value()

double Hurley_rl::get_mt_value ( ) const

inlineoverrideprotectedvirtualinherited

Reimplemented from Orbital_change_RL.

◆ get_rldonor()

double Hurley_rl::get_rldonor ( )

inlineprotectedinherited

◆ GetStaticMap()

static std::map< std::string, Orbital_change_RL * > & Orbital_change_RL::GetStaticMap ( )

inlinestaticprivateinherited

◆ GetUsed()

static std::vector< int > & Orbital_change_RL::GetUsed ( )

inlinestaticprivateinherited

◆ Hfrac()

double Orbital_change_RL::Hfrac ( Star * s )

protectedvirtualinherited

Estimate the H fraction based on the functional form .... (found in SEVN1)

Parameters

s	Pointer to the star

Returns

◆ init()

void Hurley_rl::init ( _UNUSED Binstar * b )

overridevirtualinherited

Init function to be called at the beginning of the Process::evolve

Parameters

b	Pointer to the binary

NOW check for Mix or Common envelope due to both stars filling the Roche Lobe

NOW analyse the RLO

Now SET the binary mix or comenv outcome

Reimplemented from Orbital_change_RL.

◆ init_common_variable()

void Hurley_rl::init_common_variable	(	Star *	donor_star,
		Star *	accretor_star,
		Binstar *	b
	)

protectedinherited

Set the common variable used by DM, DE, DA assuming a given donor and accretor star

Parameters

donor_star	Pointer to the star that is filling the RL
accretor_star	Pointer to the star that is accreting mass
b	Pointer to the binary

mt stuff - NOTICE, the interpretation of these two values depend on the mt_stability option if the option is from the qcrit family, mt_value=q and mt_tshold=qcrit, if the option is from the zeta family, mt_value=zeta_adiabatic and mt_tshold=zeta_RL

Accretion efficency

Times

◆ instance()

Hurley_mod_rl * Hurley_mod_rl::instance ( )

inlineoverridevirtual

Reimplemented from Hurley_rl.

◆ Instance()

Orbital_change_RL * Orbital_change_RL::Instance ( const std::string & name )

staticinherited

◆ is_colliding()

bool Orbital_change_RL::is_colliding ( )

inlineinherited

◆ is_giant_like()

bool Orbital_change_RL::is_giant_like ( int star_type_bse )

inlineprotectedinherited

Check if the star can be considered giant or giant-like in the BSE type classification

Parameters

star_type_bse BSE star type

Returns: true if the type is between 2 and 9 (inclusive) but not 7, false otherwise

◆ is_process_ongoing()

bool Orbital_change_RL::is_process_ongoing ( )

inlineoverridevirtualinherited

Other function that return useful information.

Check if the process is really ongoing, i.e. it is really changing properties.

Returns

Reimplemented from Orbital_change.

Reimplemented in disabled_rl.

◆ is_swallowed()

bool Orbital_change_RL::is_swallowed ( int starID )

inlineinherited

◆ kelvin_helmotz_tscale()

double Orbital_change_RL::kelvin_helmotz_tscale ( Star * s )

protectedvirtualinherited

time scales

Time scales.

Kelvin-Helmholtz time scale from the modified classical expression (Eq. 61, Hurley+2002) Directly taken from SEVN1

Parameters

s	Pointer to star

Returns: Kelvin-Helmholtz time scale in yr

◆ name()

std::string Hurley_mod_rl::name ( )

inlineoverridevirtual

Reimplemented from Hurley_rl.

◆ nuclear_dmdt()

double Hurley_rl::nuclear_dmdt	(	_UNUSED Star *	s,
		_UNUSED Binstar *	b
	)

overrideprotectedvirtualinherited

Rate of dynamic mass transfer from Eq. 60 in Hurley+2002

Parameters

s	pointer to the Star that is losing mass
b	pointer to the binary

Returns: dm/dt

Reimplemented from Orbital_change_RL.

◆ outcome_collision() [1/3]

int Hurley_rl::outcome_collision ( _UNUSED Binstar * b )

overrideprotectedvirtualinherited

Set binary mix or common evelope to true depending on the stellar bse phases in case of collision at the pericenter. In that version the check is made in a symmetric way (both the donor and accretor have the same role)

Parameters

donor_star	Pointer to the star that is filling the RL
accretor_star	Pointer to the star that is accreting mass
b	Pointer to the binary

Returns: EXIT_SUCCESS

Reimplemented from Orbital_change_RL.

◆ outcome_collision() [2/3]

virtual int Orbital_change_RL::outcome_collision	(	_UNUSED Star *	donor,
		_UNUSED Star *	accretor,
		_UNUSED Binstar *	b
	)

inlineprotectedvirtualinherited

Set binary mix or common evelope to true depending on the stellar bse phases in case of collision at the pericenter

Parameters

b	Pointer to the binary

Returns: EXIT_SUCCESS

◆ outcome_collision() [3/3]

int Hurley_rl::outcome_collision	(	Star *	donor,
		Star *	accretor,
		_UNUSED Binstar *	b
	)

overrideprotectedinherited

Set binary mix or common evelope to true depending on the stellar bse phases in case of collision at the pericenter. In that version the check is made in a asymmetric way, the donor is the star filling the Roche Lobe.

Parameters

b	Pointer to the binary

Returns: EXIT_SUCCESS

◆ outcome_double_RLO()

int Hurley_rl::outcome_double_RLO ( _UNUSED Binstar * b )

overrideprotectedvirtualinherited

Set binary mix or common evelope to true depending on the stellar bse phases in case of both stars are overfilling the RL

Parameters

b	Pointer to the binary

Returns: EXIT_SUCCESS

Reimplemented from Orbital_change_RL.

◆ Register()

void Orbital_change_RL::Register	(	Orbital_change_RL *	ptr,
		const std::string &	_name
	)

inlineprotectedinherited

◆ reset_DM()

int Orbital_change_RL::reset_DM ( )

inlineprotectedinherited

◆ reset_swallowed() [1/2]

int Orbital_change_RL::reset_swallowed ( )

inlineprotectedinherited

◆ reset_swallowed() [2/2]

int Orbital_change_RL::reset_swallowed ( int starID )

inlineprotectedinherited

◆ RLO() [1/2]

void Hurley_rl::RLO ( _UNUSED Binstar * b )

protectedinherited

Actual RocheLobe Overflow process as reported in Hurely+2002 and BSE

Parameters

donor	Pointer to the star that is overflowing the RocheLobe
accretor	Pointer to the star that is accreting mass
b	Pointer to the binary

Note: : Sometime the code does not strictly follows what reported in Hurley2002 paper, this because BSE code has been updated. The current implementation is directly ported from SEVN1 with a modification made by MM on the fraction of the mass accreted that is now tuned by the parameter rlo_f_mass_accreted.

MM: UNSTABLE ACCRETION ON DYNAMICAL TIMESCALE: CALL COMMON ENVELOPE OR MERGE

Case for WDs

Assume the energy released by ignition of triple=alpha is enough to destroy the star(s)

STABLE MASS TRANSFER ON THERMAL TIME SCALE OR NUCLEAR (take the minimum) (Hurley+2002, Sec. 2.6.2 and Sec. 2.6.3)

◆ RLO() [2/2]

virtual void Orbital_change_RL::RLO	(	_UNUSED Star *	donor,
		_UNUSED Star *	accretor,
		_UNUSED Binstar *	b
	)

inlineprotectedvirtualinherited

Actual RocheLobe Overflow process

Parameters

donor	Pointer to the star that is overflowing the RocheLobe
accretor	Pointer to the star that is accreting mass
b	Pointer to the binary

◆ set_comenv()

void Orbital_change_RL::set_comenv ( )

inlineprotectedinherited

◆ set_DA()

void Hurley_rl::set_DA ( double DA )

inlineprotectedinherited

◆ set_DE()

void Hurley_rl::set_DE ( double DE )

inlineprotectedinherited

◆ set_DM()

int Orbital_change_RL::set_DM	(	double	DM,
		int	starID
	)

inlineprotectedinherited

◆ set_is_colliding()

void Orbital_change_RL::set_is_colliding ( )

inlineprotectedinherited

◆ set_is_RLO_happening()

void Orbital_change_RL::set_is_RLO_happening ( )

inlineprotectedinherited

◆ set_mix()

void Orbital_change_RL::set_mix ( )

inlineprotectedinherited

◆ set_options() [1/2]

virtual void Orbital_change::set_options ( _UNUSED IO * _io )

inlinevirtualinherited

◆ set_options() [2/2]

void Orbital_change_RL::set_options ( IO * _io )

inlineoverrideinherited

◆ set_orbital()

void Hurley_mod_rl::set_orbital ( _UNUSED Binstar * b )

overrideprotectedvirtual

Load current Mass transfer

First check if actual mass transfer is happening

Angmom lost from the system

Angmom from donor Orbit-spin coupling

Now estimate _DA as anew - a, where anew estimated from the updated AngMom

Reimplemented from Hurley_rl.

◆ set_swallowed()

int Orbital_change_RL::set_swallowed ( int starID )

inlineprotectedinherited

◆ speciale_evolve()

int Orbital_change_RL::speciale_evolve ( _UNUSED Binstar * b )

overridevirtualinherited

Mass transfer.

Reimplemented from Orbital_change.

◆ thermal_dmdt()

double Hurley_rl::thermal_dmdt	(	_UNUSED Star *	s,
		_UNUSED Binstar *	b
	)

overrideprotectedvirtualinherited

Rate of dynamic mass transfer from Eq. 58 and Eq.59 in Hurley+2002

Parameters

s	pointer to the Star that is losing mass
b	pointer to the binary

Returns: dm/dt

Note: the implementation is a bit different with respect to what is reported in Hurley+2002, but it comes directly from BSE

Reimplemented from Orbital_change_RL.

◆ thermal_nuclear_accreted_mass()

double Hurley_rl::thermal_nuclear_accreted_mass	(	_UNUSED double	DM_donor,
		_UNUSED Star *	donor,
		_UNUSED Star *	accretor,
		_UNUSED Binstar *	b
	)

overrideprotectedvirtualinherited

Handle the mass accreted on the companion on thermal or nuclear timescale It takes into account also special cases such as accretionon compact objects. The basic accreted mass is simply DM_accreted=fMT*DM_donor (fmt is the runtime parameter rlo_f_mass_accreted)

Parameters

DM_donor	Total amount of mass lost by the donor star [Msun]
donor	Pointer to the donor star
accretor	Pointer to the accretor star
b	Pointer to the binary

Returns: Final amount of mass accreted on the accretor

Mass accretion

Reimplemented from Orbital_change_RL.

Reimplemented in Hurley_rl_bse.

◆ unset_comenv()

void Orbital_change_RL::unset_comenv ( )

inlineprotectedinherited

◆ unset_is_colliding()

void Orbital_change_RL::unset_is_colliding ( )

inlineprotectedinherited

◆ unset_is_RLO_happening()

void Orbital_change_RL::unset_is_RLO_happening ( )

inlineprotectedinherited

◆ unset_mix()

void Orbital_change_RL::unset_mix ( )

inlineprotectedinherited

Member Data Documentation

◆ _DA

double Hurley_rl::_DA = 0

protectedinherited

◆ _DE

double Hurley_rl::_DE = 0

protectedinherited

◆ _DLspin

double Hurley_rl::_DLspin[2] ={0.,0.}

protectedinherited

◆ _DM

double Orbital_change_RL::_DM[2] ={0,0}

privateinherited

◆ _Hurley_mod_rl

Hurley_mod_rl Hurley_mod_rl::_Hurley_mod_rl

static

◆ _Hurley_rl

Hurley_rl Hurley_rl::_Hurley_rl

staticinherited

◆ _is_colliding

bool Orbital_change_RL::_is_colliding =false

privateinherited

◆ _is_RLO_happening

bool Orbital_change_RL::_is_RLO_happening =false

privateinherited

◆ _is_swallowed

bool Orbital_change_RL::_is_swallowed[2] ={false, false}

privateinherited

Array of bool corresponding to the ID of stars in binary. If true, the star has been swallowed through the RLO

◆ accretor

Star* Hurley_rl::accretor

protectedinherited

◆ comenv

bool Orbital_change_RL::comenv = false

privateinherited

◆ dmdt_edd

double Hurley_rl::dmdt_edd = utilities::NULL_DOUBLE

protectedinherited

◆ donor

Star* Hurley_rl::donor

protectedinherited

◆ dt

double Hurley_rl::dt = utilities::NULL_DOUBLE

protectedinherited

Times.

◆ f_MT

double Hurley_rl::f_MT = utilities::NULL_DOUBLE

protectedinherited

Accretion efficency.

◆ frl1

double Hurley_rl::frl1 = utilities::NULL_DOUBLE

protectedinherited

◆ is_RL_in_core

bool Hurley_rl::is_RL_in_core = false

protectedinherited

◆ mix

bool Orbital_change_RL::mix = false

privateinherited

◆ mt_stability

MTstability* Orbital_change_RL::mt_stability

protectedinherited

◆ mt_tshold

double Hurley_rl::mt_tshold = utilities::NULL_DOUBLE

protectedinherited

◆ mt_value

double Hurley_rl::mt_value = utilities::NULL_DOUBLE

protectedinherited

◆ novae

bool Orbital_change_RL::novae =false

inherited

◆ rl1

double Hurley_rl::rl1 = utilities::NULL_DOUBLE

protectedinherited

◆ star_type1

int Hurley_rl::star_type1 = utilities::NULL_INT

protectedinherited

◆ star_type2

int Hurley_rl::star_type2 = utilities::NULL_INT

protectedinherited

◆ super_eddington

bool Orbital_change_RL::super_eddington =false

inherited

◆ svlog

SevnLogging Orbital_change::svlog

protectedinherited

◆ taum

double Hurley_rl::taum = utilities::NULL_DOUBLE

protectedinherited

◆ tdyn1

double Hurley_rl::tdyn1 = utilities::NULL_DOUBLE

protectedinherited

◆ tkh1

double Hurley_rl::tkh1 = utilities::NULL_DOUBLE

protectedinherited

◆ tkh2

double Hurley_rl::tkh2 = utilities::NULL_DOUBLE

protectedinherited

The documentation for this class was generated from the following files:

/Users/giulianoiorio/Documents/sevn_public/src/binstar/Orbit.h
/Users/giulianoiorio/Documents/sevn_public/src/binstar/Orbit.cpp
/Users/giulianoiorio/Documents/sevn_public/include/static_main.h

Public Member Functions

Static Public Member Functions

Public Attributes

Static Public Attributes

Protected Member Functions

Protected Attributes

Static Private Member Functions

Private Attributes

Constructor & Destructor Documentation

◆ Hurley_mod_rl()

Member Function Documentation

◆ check_collision_at_periastron()

◆ check_compact_accretor()

◆ check_doubleRLO()

◆ correct_accreted_mass()

◆ DA()

◆ DAngMomSpin()

◆ DE()

◆ DM()

◆ dMdt_eddington()

◆ dynamic_dmdt()

◆ dynamic_swallowing()

◆ dynamic_tscale()

◆ estimate_q()

◆ fRL_radius()

◆ get_accretor()

◆ get_comenv()

◆ get_DM()

◆ get_donor()

◆ get_mix()

◆ get_mt_tshold()

◆ get_mt_value()

◆ get_rldonor()

◆ GetStaticMap()

◆ GetUsed()

◆ Hfrac()

◆ init()

◆ init_common_variable()

◆ instance()

◆ Instance()

◆ is_colliding()

◆ is_giant_like()

◆ is_process_ongoing()

◆ is_swallowed()

◆ kelvin_helmotz_tscale()

◆ name()

◆ nuclear_dmdt()

◆ outcome_collision() [1/3]

◆ outcome_collision() [2/3]

◆ outcome_collision() [3/3]

◆ outcome_double_RLO()

◆ Register()

◆ reset_DM()

◆ reset_swallowed() [1/2]

◆ reset_swallowed() [2/2]

◆ RLO() [1/2]

◆ RLO() [2/2]

◆ set_comenv()

◆ set_DA()

◆ set_DE()

◆ set_DM()

◆ set_is_colliding()

◆ set_is_RLO_happening()

◆ set_mix()

◆ set_options() [1/2]

◆ set_options() [2/2]

◆ set_orbital()

◆ set_swallowed()

◆ speciale_evolve()

◆ thermal_dmdt()

◆ thermal_nuclear_accreted_mass()

◆ unset_comenv()

◆ unset_is_colliding()

◆ unset_is_RLO_happening()

◆ unset_mix()

Member Data Documentation

◆ _DA

◆ _DE

◆ _DLspin

◆ _DM