Lorene::Eos_Fermi Class Reference
[Equations of state]

Degenerate ideal Fermi gas. More...

#include <eos.h>

Inheritance diagram for Lorene::Eos_Fermi:
Lorene::Eos

List of all members.

Public Member Functions

 Eos_Fermi (double mass)
 Standard constructor (sets g_s to 2).
 Eos_Fermi (double mass, int g_degen)
 Standard constructor.
 Eos_Fermi (const Eos_Fermi &)
 Copy constructor.
virtual ~Eos_Fermi ()
 Destructor.
void operator= (const Eos_Fermi &)
 Assignment to another Eos_Fermi.
virtual bool operator== (const Eos &) const
 Comparison operator (egality).
virtual bool operator!= (const Eos &) const
 Comparison operator (difference).
virtual int identify () const
 Returns a number to identify the sub-classe of Eos the object belongs to.
double get_m () const
 Returns the fermion mass in eV/c2.
int get_g_degen () const
 Returns the degeneracy factor.
virtual void sauve (FILE *) const
 Save in a file.
virtual double nbar_ent_p (double ent, const Param *par=0x0) const
 Computes the baryon density from the log-enthalpy.
virtual double ener_ent_p (double ent, const Param *par=0x0) const
 Computes the total energy density from the log-enthalpy.
virtual double press_ent_p (double ent, const Param *par=0x0) const
 Computes the pressure from the log-enthalpy.
virtual double der_nbar_ent_p (double ent, const Param *par=0x0) const
 Computes the logarithmic derivative $d\ln n/d\ln H$ from the log-enthalpy.
virtual double der_ener_ent_p (double ent, const Param *par=0x0) const
 Computes the logarithmic derivative $d\ln e/d\ln H$ from the log-enthalpy.
virtual double der_press_ent_p (double ent, const Param *par=0x0) const
 Computes the logarithmic derivative $d\ln p/d\ln H$ from the log-enthalpy.
const char * get_name () const
 Returns the EOS name.
void set_name (const char *name_i)
 Sets the EOS name.
virtual bool operator== (const Eos &) const =0
 Comparison operator (egality).
virtual bool operator!= (const Eos &) const =0
 Comparison operator (difference).
Cmp nbar_ent (const Cmp &ent, int nzet, int l_min=0, Param *par=0x0) const
 Computes the baryon density field from the log-enthalpy field and extra parameters.
Scalar nbar_ent (const Scalar &ent, int nzet, int l_min=0, Param *par=0x0) const
 Computes the baryon density field from the log-enthalpy field and extra parameters.
Cmp ener_ent (const Cmp &ent, int nzet, int l_min=0, Param *par=0x0) const
 Computes the total energy density from the log-enthalpy and extra parameters.
Scalar ener_ent (const Scalar &ent, int nzet, int l_min=0, Param *par=0x0) const
 Computes the total energy density from the log-enthalpy and extra parameters.
Cmp press_ent (const Cmp &ent, int nzet, int l_min=0, Param *par=0x0) const
 Computes the pressure from the log-enthalpy and extra parameters.
Scalar press_ent (const Scalar &ent, int nzet, int l_min=0, Param *par=0x0) const
 Computes the pressure from the log-enthalpy and extra parameters.
Cmp der_nbar_ent (const Cmp &ent, int nzet, int l_min=0, Param *par=0x0) const
 Computes the logarithmic derivative $d\ln n/d\ln H$ from the log-enthalpy and extra parameters.
Scalar der_nbar_ent (const Scalar &ent, int nzet, int l_min=0, Param *par=0x0) const
 Computes the logarithmic derivative $d\ln n/d\ln H$ from the log-enthalpy and extra parameters.
Cmp der_ener_ent (const Cmp &ent, int nzet, int l_min=0, Param *par=0x0) const
 Computes the logarithmic derivative $d\ln e/d\ln H$ from the log-enthalpy and extra parameters.
Scalar der_ener_ent (const Scalar &ent, int nzet, int l_min=0, Param *par=0x0) const
 Computes the logarithmic derivative $d\ln e/d\ln H$ from the log-enthalpy and extra parameters.
Cmp der_press_ent (const Cmp &ent, int nzet, int l_min=0, Param *par=0x0) const
 Computes the logarithmic derivative $d\ln p/d\ln H$ from the log-enthalpy and extra parameters.
Scalar der_press_ent (const Scalar &ent, int nzet, int l_min=0, Param *par=0x0) const
 Computes the logarithmic derivative $d\ln p/d\ln H$ from the log-enthalpy and extra parameters.

Static Public Member Functions

static Eoseos_from_file (FILE *)
 Construction of an EOS from a binary file.
static Eoseos_from_file (ifstream &)
 Construction of an EOS from a formatted file.

Protected Member Functions

 Eos_Fermi (FILE *)
 Constructor from a binary file (created by the function sauve(FILE*) ).
 Eos_Fermi (ifstream &)
 Constructor from a formatted file.
void set_auxiliary ()
 Computes the auxiliary quantities n_0 , ener_0.
virtual ostream & operator>> (ostream &) const
 Operator >>.
void calcule (const Cmp &thermo, int nzet, int l_min, double(Eos::*fait)(double, const Param *) const, Param *par, Cmp &resu) const
 General computational method for Cmp 's.
void calcule (const Scalar &thermo, int nzet, int l_min, double(Eos::*fait)(double, const Param *) const, Param *par, Scalar &resu) const
 General computational method for Scalar 's.

Protected Attributes

double m_0
 Individual particule mass $m_0$ [unit: eV/c2].
int g_s
 Degeneracy parameter.
double n_0
 Number density scale [unit: $n_{\rm nuc} := 0.1 \ {\rm fm}^{-3}$].
double ener_0
 Energy density scale [unit: $\rho_{\rm nuc} c^2$], where $\rho_{\rm nuc} := 1.66\ 10^{17} \ {\rm kg/m}^3$].
double p_0
 Pressure scale [unit: $\rho_{\rm nuc} c^2$], where $\rho_{\rm nuc} := 1.66\ 10^{17} \ {\rm kg/m}^3$].
char name [100]
 EOS name.

Friends

EosEos::eos_from_file (FILE *)
 The construction functions from a file.
EosEos::eos_from_file (ifstream &)
ostream & operator<< (ostream &, const Eos &)
 Display.

Detailed Description

Degenerate ideal Fermi gas.

This equation of state describes an ideal gas of relativistic fermions at zero temperature. It has two parameters : the fermion mass $m$ and the degeneracy $g_s$ of each momentum state (for electrons or neutrons : $g_s = 2$).

*** NB: This class is _under construction_ and not fully tested yet ! ***

()

Definition at line 2095 of file eos.h.


Constructor & Destructor Documentation

Lorene::Eos_Fermi::Eos_Fermi ( double  mass  ) 

Standard constructor (sets g_s to 2).

Parameters:
mass mass of each fermion in eV/c2

Definition at line 65 of file eos_fermi.C.

References set_auxiliary().

Lorene::Eos_Fermi::Eos_Fermi ( double  mass,
int  g_degen 
)

Standard constructor.

Parameters:
mass mass of each fermion in eV/c2
g_degen degeneracy factor (value for electrons or neutrons: 2)

Definition at line 76 of file eos_fermi.C.

References set_auxiliary().

Lorene::Eos_Fermi::Eos_Fermi ( const Eos_Fermi eosi  ) 

Copy constructor.

Definition at line 87 of file eos_fermi.C.

References set_auxiliary().

Lorene::Eos_Fermi::Eos_Fermi ( FILE *  fich  )  [protected]

Constructor from a binary file (created by the function sauve(FILE*) ).

This constructor is protected because any EOS construction from a binary file must be done via the function Eos::eos_from_file(FILE*) .

Definition at line 98 of file eos_fermi.C.

References Lorene::fread_be(), g_s, m_0, and set_auxiliary().

Lorene::Eos_Fermi::Eos_Fermi ( ifstream &  fich  )  [protected]

Constructor from a formatted file.

This constructor is protected because any EOS construction from a formatted file must be done via the function Eos::eos_from_file(ifstream&) .

Definition at line 111 of file eos_fermi.C.

References g_s, m_0, and set_auxiliary().

Lorene::Eos_Fermi::~Eos_Fermi (  )  [virtual]

Destructor.

Definition at line 126 of file eos_fermi.C.


Member Function Documentation

void Lorene::Eos::calcule ( const Scalar thermo,
int  nzet,
int  l_min,
double(Eos::*)(double, const Param *) const   fait,
Param par,
Scalar resu 
) const [protected, inherited]

General computational method for Scalar 's.

Parameters:
thermo [input] thermodynamical quantity (for instance the enthalpy field)from which the thermodynamical quantity resu is to be computed.
nzet [input] number of domains where resu is to be computed.
l_min [input] index of the innermost domain is which resu is to be computed [default value: 0]; resu is computed only in domains whose indices are in [l_min,l_min+nzet-1] . In the other domains, it is set to zero.
fait [input] pointer on the member function of class Eos which performs the pointwise calculation.
par possible extra parameters of the EOS
resu [output] result of the computation.

Definition at line 282 of file eos.C.

References Lorene::Param::add_int_mod(), Lorene::Scalar::annule(), Lorene::Valeur::c, Lorene::Valeur::coef_i(), Lorene::Tbl::get_etat(), Lorene::Scalar::get_etat(), Lorene::Tensor::get_mp(), Lorene::Mg3d::get_nzone(), Lorene::Scalar::get_spectral_va(), Lorene::Tbl::get_taille(), Lorene::Valeur::set_etat_c_qcq(), Lorene::Tbl::set_etat_qcq(), Lorene::Mtbl::set_etat_qcq(), Lorene::Scalar::set_etat_qcq(), Lorene::Tbl::set_etat_zero(), Lorene::Scalar::set_etat_zero(), Lorene::Scalar::set_spectral_va(), Lorene::Tbl::t, and Lorene::Mtbl::t.

void Lorene::Eos::calcule ( const Cmp thermo,
int  nzet,
int  l_min,
double(Eos::*)(double, const Param *) const   fait,
Param par,
Cmp resu 
) const [protected, inherited]

General computational method for Cmp 's.

Parameters:
thermo [input] thermodynamical quantity (for instance the enthalpy field)from which the thermodynamical quantity resu is to be computed.
nzet [input] number of domains where resu is to be computed.
l_min [input] index of the innermost domain is which resu is to be computed [default value: 0]; resu is computed only in domains whose indices are in [l_min,l_min+nzet-1] . In the other domains, it is set to zero.
fait [input] pointer on the member function of class Eos which performs the pointwise calculation.
par possible extra parameters of the EOS
resu [output] result of the computation.

Definition at line 210 of file eos.C.

References Lorene::Param::add_int_mod(), Lorene::Cmp::annule(), Lorene::Valeur::c, Lorene::Valeur::coef_i(), Lorene::Tbl::get_etat(), Lorene::Cmp::get_etat(), Lorene::Cmp::get_mp(), Lorene::Mg3d::get_nzone(), Lorene::Tbl::get_taille(), Lorene::Valeur::set_etat_c_qcq(), Lorene::Tbl::set_etat_qcq(), Lorene::Mtbl::set_etat_qcq(), Lorene::Cmp::set_etat_qcq(), Lorene::Tbl::set_etat_zero(), Lorene::Cmp::set_etat_zero(), Lorene::Tbl::t, Lorene::Mtbl::t, and Lorene::Cmp::va.

Scalar Lorene::Eos::der_ener_ent ( const Scalar ent,
int  nzet,
int  l_min = 0,
Param par = 0x0 
) const [inherited]

Computes the logarithmic derivative $d\ln e/d\ln H$ from the log-enthalpy and extra parameters.

Parameters:
ent [input, unit: $c^2$] log-enthalpy H defined by $H = c^2 \ln\left( {e+p \over m_B c^2 n} \right) $, where e is the (total) energy density, p the pressure, n the baryon density, and $m_B$ the baryon mass
nzet number of domains where the derivative dln(e)/dln(H) is to be computed.
l_min index of the innermost domain is which the coefficient dln(n)/dln(H) is to be computed [default value: 0]; the derivative dln(e)/dln(H) is computed only in domains whose indices are in [l_min,l_min+nzet-1] . In the other domains, it is set to zero.
par possible extra parameters of the EOS
Returns:
dln(e)/dln(H)

Definition at line 461 of file eos.C.

References Lorene::Eos::calcule(), Lorene::Eos::der_ener_ent_p(), and Lorene::Tensor::get_mp().

Cmp Lorene::Eos::der_ener_ent ( const Cmp ent,
int  nzet,
int  l_min = 0,
Param par = 0x0 
) const [inherited]

Computes the logarithmic derivative $d\ln e/d\ln H$ from the log-enthalpy and extra parameters.

Parameters:
ent [input, unit: $c^2$] log-enthalpy H defined by $H = c^2 \ln\left( {e+p \over m_B c^2 n} \right) $, where e is the (total) energy density, p the pressure, n the baryon density, and $m_B$ the baryon mass
nzet number of domains where the derivative dln(e)/dln(H) is to be computed.
l_min index of the innermost domain is which the coefficient dln(n)/dln(H) is to be computed [default value: 0]; the derivative dln(e)/dln(H) is computed only in domains whose indices are in [l_min,l_min+nzet-1] . In the other domains, it is set to zero.
par possible extra parameters of the EOS
Returns:
dln(e)/dln(H)

Definition at line 451 of file eos.C.

References Lorene::Eos::calcule(), Lorene::Eos::der_ener_ent_p(), and Lorene::Cmp::get_mp().

double Lorene::Eos_Fermi::der_ener_ent_p ( double  ent,
const Param par = 0x0 
) const [virtual]

Computes the logarithmic derivative $d\ln e/d\ln H$ from the log-enthalpy.

Parameters:
ent [input, unit: $c^2$] log-enthalpy H
par possible extra parameters of the EOS (not used here)
Returns:
dln(e)/dln(H)

Implements Lorene::Eos.

Definition at line 314 of file eos_fermi.C.

Scalar Lorene::Eos::der_nbar_ent ( const Scalar ent,
int  nzet,
int  l_min = 0,
Param par = 0x0 
) const [inherited]

Computes the logarithmic derivative $d\ln n/d\ln H$ from the log-enthalpy and extra parameters.

Parameters:
ent [input, unit: $c^2$] log-enthalpy H defined by $H = c^2 \ln\left( {e+p \over m_B c^2 n} \right) $, where e is the (total) energy density, p the pressure, n the baryon density, and $m_B$ the baryon mass
nzet number of domains where the derivative dln(n)/dln(H) is to be computed.
l_min index of the innermost domain is which the coefficient dln(n)/dln(H) is to be computed [default value: 0]; the derivative dln(n)/dln(H) is computed only in domains whose indices are in [l_min,l_min+nzet-1] . In the other domains, it is set to zero.
par possible extra parameters of the EOS
Returns:
dln(n)/dln(H)

Definition at line 438 of file eos.C.

References Lorene::Eos::calcule(), Lorene::Eos::der_nbar_ent_p(), and Lorene::Tensor::get_mp().

Cmp Lorene::Eos::der_nbar_ent ( const Cmp ent,
int  nzet,
int  l_min = 0,
Param par = 0x0 
) const [inherited]

Computes the logarithmic derivative $d\ln n/d\ln H$ from the log-enthalpy and extra parameters.

Parameters:
ent [input, unit: $c^2$] log-enthalpy H defined by $H = c^2 \ln\left( {e+p \over m_B c^2 n} \right) $, where e is the (total) energy density, p the pressure, n the baryon density, and $m_B$ the baryon mass
nzet number of domains where the derivative dln(n)/dln(H) is to be computed.
l_min index of the innermost domain is which the coefficient dln(n)/dln(H) is to be computed [default value: 0]; the derivative dln(n)/dln(H) is computed only in domains whose indices are in [l_min,l_min+nzet-1] . In the other domains, it is set to zero.
par possible extra parameters of the EOS
Returns:
dln(n)/dln(H)

Definition at line 428 of file eos.C.

References Lorene::Eos::calcule(), Lorene::Eos::der_nbar_ent_p(), and Lorene::Cmp::get_mp().

double Lorene::Eos_Fermi::der_nbar_ent_p ( double  ent,
const Param par = 0x0 
) const [virtual]

Computes the logarithmic derivative $d\ln n/d\ln H$ from the log-enthalpy.

Parameters:
ent [input, unit: $c^2$] log-enthalpy H
par possible extra parameters of the EOS (not used here)
Returns:
dln(n)/dln(H)

Implements Lorene::Eos.

Definition at line 304 of file eos_fermi.C.

Scalar Lorene::Eos::der_press_ent ( const Scalar ent,
int  nzet,
int  l_min = 0,
Param par = 0x0 
) const [inherited]

Computes the logarithmic derivative $d\ln p/d\ln H$ from the log-enthalpy and extra parameters.

Parameters:
ent [input, unit: $c^2$] log-enthalpy H defined by $H = c^2 \ln\left( {e+p \over m_B c^2 n} \right) $, where e is the (total) energy density, p the pressure, n the baryon density, and $m_B$ the baryon mass
nzet number of domains where the derivative dln(p)/dln(H) is to be computed.
par possible extra parameters of the EOS
l_min index of the innermost domain is which the coefficient dln(n)/dln(H) is to be computed [default value: 0]; the derivative dln(p)/dln(H) is computed only in domains whose indices are in [l_min,l_min+nzet-1] . In the other domains, it is set to zero.
Returns:
dln(p)/dln(H)

Definition at line 483 of file eos.C.

References Lorene::Eos::calcule(), Lorene::Eos::der_press_ent_p(), and Lorene::Tensor::get_mp().

Cmp Lorene::Eos::der_press_ent ( const Cmp ent,
int  nzet,
int  l_min = 0,
Param par = 0x0 
) const [inherited]

Computes the logarithmic derivative $d\ln p/d\ln H$ from the log-enthalpy and extra parameters.

Parameters:
ent [input, unit: $c^2$] log-enthalpy H defined by $H = c^2 \ln\left( {e+p \over m_B c^2 n} \right) $, where e is the (total) energy density, p the pressure, n the baryon density, and $m_B$ the baryon mass
nzet number of domains where the derivative dln(p)/dln(H) is to be computed.
par possible extra parameters of the EOS
l_min index of the innermost domain is which the coefficient dln(n)/dln(H) is to be computed [default value: 0]; the derivative dln(p)/dln(H) is computed only in domains whose indices are in [l_min,l_min+nzet-1] . In the other domains, it is set to zero.
Returns:
dln(p)/dln(H)

Definition at line 473 of file eos.C.

References Lorene::Eos::calcule(), Lorene::Eos::der_press_ent_p(), and Lorene::Cmp::get_mp().

double Lorene::Eos_Fermi::der_press_ent_p ( double  ent,
const Param par = 0x0 
) const [virtual]

Computes the logarithmic derivative $d\ln p/d\ln H$ from the log-enthalpy.

Parameters:
ent [input, unit: $c^2$] log-enthalpy H
par possible extra parameters of the EOS
Returns:
dln(p)/dln(H)

Implements Lorene::Eos.

Definition at line 324 of file eos_fermi.C.

Scalar Lorene::Eos::ener_ent ( const Scalar ent,
int  nzet,
int  l_min = 0,
Param par = 0x0 
) const [inherited]

Computes the total energy density from the log-enthalpy and extra parameters.

Parameters:
ent [input, unit: $c^2$] log-enthalpy H defined by $H = c^2 \ln\left( {e+p \over m_B c^2 n} \right) $, where e is the (total) energy density, p the pressure, n the baryon density, and $m_B$ the baryon mass
nzet number of domains where the energy density is to be computed.
l_min index of the innermost domain is which the energy density is to be computed [default value: 0]; the energy density is computed only in domains whose indices are in [l_min,l_min+nzet-1] . In the other domains, it is set to zero.
par possible extra parameters of the EOS
Returns:
energy density [unit: $\rho_{\rm nuc} c^2$], where $\rho_{\rm nuc} := 1.66\ 10^{17} \ {\rm kg/m}^3$

Definition at line 394 of file eos.C.

References Lorene::Eos::calcule(), Lorene::Eos::ener_ent_p(), and Lorene::Tensor::get_mp().

Cmp Lorene::Eos::ener_ent ( const Cmp ent,
int  nzet,
int  l_min = 0,
Param par = 0x0 
) const [inherited]

Computes the total energy density from the log-enthalpy and extra parameters.

Parameters:
ent [input, unit: $c^2$] log-enthalpy H defined by $H = c^2 \ln\left( {e+p \over m_B c^2 n} \right) $, where e is the (total) energy density, p the pressure, n the baryon density, and $m_B$ the baryon mass
nzet number of domains where the energy density is to be computed.
l_min index of the innermost domain is which the energy density is to be computed [default value: 0]; the energy density is computed only in domains whose indices are in [l_min,l_min+nzet-1] . In the other domains, it is set to zero.
par possible extra parameters of the EOS
Returns:
energy density [unit: $\rho_{\rm nuc} c^2$], where $\rho_{\rm nuc} := 1.66\ 10^{17} \ {\rm kg/m}^3$

Definition at line 384 of file eos.C.

References Lorene::Eos::calcule(), Lorene::Eos::ener_ent_p(), and Lorene::Cmp::get_mp().

double Lorene::Eos_Fermi::ener_ent_p ( double  ent,
const Param par = 0x0 
) const [virtual]

Computes the total energy density from the log-enthalpy.

Parameters:
ent [input, unit: $c^2$] log-enthalpy H
par possible extra parameters of the EOS (not used here)
Returns:
energy density e [unit: $\rho_{\rm nuc} c^2$], where $\rho_{\rm nuc} := 1.66\ 10^{17} \ {\rm kg/m}^3$

Implements Lorene::Eos.

Definition at line 267 of file eos_fermi.C.

References ener_0, Lorene::exp(), Lorene::log(), and Lorene::sqrt().

Eos * Lorene::Eos::eos_from_file ( ifstream &  fich  )  [static, inherited]

Construction of an EOS from a formatted file.

The fist line of the file must start by the EOS number, according to the following conventions:

  • 1 = relativistic polytropic EOS (class Eos_poly ).
  • 2 = Newtonian polytropic EOS (class Eos_poly_newt ).
  • 3 = Relativistic incompressible EOS (class Eos_incomp ).
  • 4 = Newtonian incompressible EOS (class Eos_incomp_newt ).
  • 5 = Strange matter (MIT Bag model)
  • 6 = Strange matter (MIT Bag model) with crust
  • 10 = SLy4 (Douchin & Haensel 2001)
  • 11 = FPS (Friedman-Pandharipande + Skyrme)
  • 12 = BPAL12 (Bombaci et al. 1995)
  • 13 = AkmalPR (Akmal, Pandharipande & Ravenhall 1998)
  • 14 = BBB2 (Baldo, Bombaci & Burgio 1997)
  • 15 = BalbN1H1 (Balberg 2000)
  • 16 = GlendNH3 (Glendenning 1985, case 3)
  • 17 = Compstar (Tabulated EOS for 2010 CompStar school)
  • 18 = magnetized (tabulated) equation of state
  • 19 = relativistic ideal Fermi gas at zero temperature (class Eos_Fermi)
  • 100 = Multi-domain EOS (class MEos )
  • 110 = Multi-polytropic EOS (class Eos_multi_poly )
  • 120 = Fitted SLy4 (Shibata 2004)
  • 121 = Fitted FPS (Shibata 2004)
  • 122 = Fitted AkmalPR (Taniguchi 2005)

The second line in the file should contain a name given by the user to the EOS. The following lines should contain the EOS parameters (one parameter per line), in the same order than in the class declaration.

Definition at line 317 of file eos_from_file.C.

Eos * Lorene::Eos::eos_from_file ( FILE *  fich  )  [static, inherited]

Construction of an EOS from a binary file.

The file must have been created by the function sauve(FILE*) .

Definition at line 180 of file eos_from_file.C.

References Lorene::fread_be().

int Lorene::Eos_Fermi::get_g_degen (  )  const

Returns the degeneracy factor.

Definition at line 169 of file eos_fermi.C.

References g_s.

double Lorene::Eos_Fermi::get_m (  )  const

Returns the fermion mass in eV/c2.

Definition at line 165 of file eos_fermi.C.

References m_0.

const char * Lorene::Eos::get_name (  )  const [inherited]

Returns the EOS name.

Definition at line 176 of file eos.C.

References Lorene::Eos::name.

int Lorene::Eos_Fermi::identify (  )  const [virtual]

Returns a number to identify the sub-classe of Eos the object belongs to.

Implements Lorene::Eos.

Definition at line 162 of file eos_from_file.C.

Scalar Lorene::Eos::nbar_ent ( const Scalar ent,
int  nzet,
int  l_min = 0,
Param par = 0x0 
) const [inherited]

Computes the baryon density field from the log-enthalpy field and extra parameters.

Parameters:
ent [input, unit: $c^2$] log-enthalpy H defined by $H = c^2 \ln\left( {e+p \over m_B c^2 n} \right) $, where e is the (total) energy density, p the pressure, n the baryon density, and $m_B$ the baryon mass
nzet number of domains where the baryon density is to be computed.
l_min index of the innermost domain is which the baryon density is to be computed [default value: 0]; the baryon density is computed only in domains whose indices are in [l_min,l_min+nzet-1] . In the other domains, it is set to zero.
par possible extra parameters of the EOS
Returns:
baryon density [unit: $n_{\rm nuc} := 0.1 \ {\rm fm}^{-3}$]

Definition at line 369 of file eos.C.

References Lorene::Eos::calcule(), Lorene::Tensor::get_mp(), and Lorene::Eos::nbar_ent_p().

Cmp Lorene::Eos::nbar_ent ( const Cmp ent,
int  nzet,
int  l_min = 0,
Param par = 0x0 
) const [inherited]

Computes the baryon density field from the log-enthalpy field and extra parameters.

Parameters:
ent [input, unit: $c^2$] log-enthalpy H defined by $H = c^2 \ln\left( {e+p \over m_B c^2 n} \right) $, where e is the (total) energy density, p the pressure, n the baryon density, and $m_B$ the baryon mass
nzet number of domains where the baryon density is to be computed.
l_min index of the innermost domain is which the baryon density is to be computed [default value: 0]; the baryon density is computed only in domains whose indices are in [l_min,l_min+nzet-1] . In the other domains, it is set to zero.
par possible extra parameters of the EOS
Returns:
baryon density [unit: $n_{\rm nuc} := 0.1 \ {\rm fm}^{-3}$]

Definition at line 359 of file eos.C.

References Lorene::Eos::calcule(), Lorene::Cmp::get_mp(), and Lorene::Eos::nbar_ent_p().

double Lorene::Eos_Fermi::nbar_ent_p ( double  ent,
const Param par = 0x0 
) const [virtual]

Computes the baryon density from the log-enthalpy.

Parameters:
ent [input, unit: $c^2$] log-enthalpy H
par possible extra parameters of the EOS (not used here)
Returns:
baryon density n [unit: $n_{\rm nuc} := 0.1 \ {\rm fm}^{-3}$]

Implements Lorene::Eos.

Definition at line 251 of file eos_fermi.C.

References Lorene::exp(), n_0, and Lorene::sqrt().

virtual bool Lorene::Eos::operator!= ( const Eos  )  const [pure virtual, inherited]

Comparison operator (difference).

bool Lorene::Eos_Fermi::operator!= ( const Eos eos_i  )  const [virtual]

Comparison operator (difference).

Definition at line 213 of file eos_fermi.C.

References operator==().

void Lorene::Eos_Fermi::operator= ( const Eos_Fermi eosi  ) 

Assignment to another Eos_Fermi.

Definition at line 135 of file eos_fermi.C.

References g_s, m_0, Lorene::Eos::name, set_auxiliary(), and Lorene::Eos::set_name().

virtual bool Lorene::Eos::operator== ( const Eos  )  const [pure virtual, inherited]

Comparison operator (egality).

bool Lorene::Eos_Fermi::operator== ( const Eos eos_i  )  const [virtual]

Comparison operator (egality).

Definition at line 180 of file eos_fermi.C.

References g_s, identify(), Lorene::Eos::identify(), and m_0.

ostream & Lorene::Eos_Fermi::operator>> ( ostream &  ost  )  const [protected, virtual]

Operator >>.

Implements Lorene::Eos.

Definition at line 233 of file eos_fermi.C.

References g_s, and m_0.

Scalar Lorene::Eos::press_ent ( const Scalar ent,
int  nzet,
int  l_min = 0,
Param par = 0x0 
) const [inherited]

Computes the pressure from the log-enthalpy and extra parameters.

Parameters:
ent [input, unit: $c^2$] log-enthalpy H defined by $H = c^2 \ln\left( {e+p \over m_B c^2 n} \right) $, where e is the (total) energy density, p the pressure, n the baryon density, and $m_B$ the baryon mass
nzet number of domains where the pressure is to be computed.
l_min index of the innermost domain is which the pressure is to be computed [default value: 0]; the pressure is computed only in domains whose indices are in [l_min,l_min+nzet-1] . In the other domains, it is set to zero.
par possible extra parameters of the EOS
Returns:
pressure [unit: $\rho_{\rm nuc} c^2$], where $\rho_{\rm nuc} := 1.66\ 10^{17} \ {\rm kg/m}^3$

Definition at line 416 of file eos.C.

References Lorene::Eos::calcule(), Lorene::Tensor::get_mp(), and Lorene::Eos::press_ent_p().

Cmp Lorene::Eos::press_ent ( const Cmp ent,
int  nzet,
int  l_min = 0,
Param par = 0x0 
) const [inherited]

Computes the pressure from the log-enthalpy and extra parameters.

Parameters:
ent [input, unit: $c^2$] log-enthalpy H defined by $H = c^2 \ln\left( {e+p \over m_B c^2 n} \right) $, where e is the (total) energy density, p the pressure, n the baryon density, and $m_B$ the baryon mass
nzet number of domains where the pressure is to be computed.
l_min index of the innermost domain is which the pressure is to be computed [default value: 0]; the pressure is computed only in domains whose indices are in [l_min,l_min+nzet-1] . In the other domains, it is set to zero.
par possible extra parameters of the EOS
Returns:
pressure [unit: $\rho_{\rm nuc} c^2$], where $\rho_{\rm nuc} := 1.66\ 10^{17} \ {\rm kg/m}^3$

Definition at line 406 of file eos.C.

References Lorene::Eos::calcule(), Lorene::Cmp::get_mp(), and Lorene::Eos::press_ent_p().

double Lorene::Eos_Fermi::press_ent_p ( double  ent,
const Param par = 0x0 
) const [virtual]

Computes the pressure from the log-enthalpy.

Parameters:
ent [input, unit: $c^2$] log-enthalpy H
par possible extra parameters of the EOS (not used here)
Returns:
pressure p [unit: $\rho_{\rm nuc} c^2$], where $\rho_{\rm nuc} := 1.66\ 10^{17} \ {\rm kg/m}^3$

Implements Lorene::Eos.

Definition at line 285 of file eos_fermi.C.

References Lorene::exp(), Lorene::log(), p_0, and Lorene::sqrt().

void Lorene::Eos_Fermi::sauve ( FILE *  fich  )  const [virtual]

Save in a file.

Reimplemented from Lorene::Eos.

Definition at line 224 of file eos_fermi.C.

References Lorene::fwrite_be(), g_s, and m_0.

void Lorene::Eos_Fermi::set_auxiliary (  )  [protected]

Computes the auxiliary quantities n_0 , ener_0.

Definition at line 151 of file eos_fermi.C.

References ener_0, g_s, m_0, n_0, and p_0.

void Lorene::Eos::set_name ( const char *  name_i  )  [inherited]

Sets the EOS name.

Definition at line 170 of file eos.C.

References Lorene::Eos::name.


Friends And Related Function Documentation

Eos* Eos::eos_from_file ( FILE *   )  [friend]

The construction functions from a file.

ostream& operator<< ( ostream &  ,
const Eos  
) [friend, inherited]

Display.


Member Data Documentation

double Lorene::Eos_Fermi::ener_0 [protected]

Energy density scale [unit: $\rho_{\rm nuc} c^2$], where $\rho_{\rm nuc} := 1.66\ 10^{17} \ {\rm kg/m}^3$].

Definition at line 2117 of file eos.h.

int Lorene::Eos_Fermi::g_s [protected]

Degeneracy parameter.

Definition at line 2108 of file eos.h.

double Lorene::Eos_Fermi::m_0 [protected]

Individual particule mass $m_0$ [unit: eV/c2].

Definition at line 2104 of file eos.h.

double Lorene::Eos_Fermi::n_0 [protected]

Number density scale [unit: $n_{\rm nuc} := 0.1 \ {\rm fm}^{-3}$].

Definition at line 2112 of file eos.h.

char Lorene::Eos::name[100] [protected, inherited]

EOS name.

Definition at line 199 of file eos.h.

double Lorene::Eos_Fermi::p_0 [protected]

Pressure scale [unit: $\rho_{\rm nuc} c^2$], where $\rho_{\rm nuc} := 1.66\ 10^{17} \ {\rm kg/m}^3$].

Definition at line 2123 of file eos.h.


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

Generated on 7 Dec 2019 for LORENE by  doxygen 1.6.1