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lightcurves_models [2021/08/04 23:52]
theoastro 		lightcurves_models [2022/07/22 19:13] (current)
theoastro [Ka2017_TrPi2018_model]
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 ===== List of available lightcurve models ===== ===== List of available lightcurve models =====
  
 +In the following, we present a list of kilonova models, for the most important ones, we provide references and list the input parameters.
  
-=== KaKy2016 ===+==== KaKy2016 ====
 [[https://arxiv.org/pdf/1601.07711.pdf|Kawaguchi et al., Astrophys.J. 825 (2016) 1, 52]]  [[https://arxiv.org/pdf/1601.07711.pdf|Kawaguchi et al., Astrophys.J. 825 (2016) 1, 52]] 
  
 Simplified analytical model for the description of BHNS systems.  Simplified analytical model for the description of BHNS systems. 
- 
-Input parameters:  
- 
  
 ---- ----
  
- +==== DiUj2017 =====
-=== DiUj2017 ====+
 [[https://arxiv.org/pdf/1612.03665.pdf|Dietrich and Ujevic, Class.Quant.Grav. 34 (2017) 10, 105014]] [[https://arxiv.org/pdf/1612.03665.pdf|Dietrich and Ujevic, Class.Quant.Grav. 34 (2017) 10, 105014]]
  
 Simplified analytical model for the description of BNS systems.  Simplified analytical model for the description of BNS systems. 
- 
-Input parameters:  
- 
  
 ---- ----
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 Input parameters: Input parameters:
-   mej +   mej --> ejecta mass  
-   vej  +   vej  --> ejecta velocity  
-   slope_r +   slope_r --> slope parameter 
-   kappa_r +   kappa_r --> opacity 
  
 ---- ----
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 Simple sum of two inclination-dependent Ka2017inc models.  Simple sum of two inclination-dependent Ka2017inc models. 
 The model does not include photon absorption or any kind of interaction between the different components.  The model does not include photon absorption or any kind of interaction between the different components. 
- 
  
 Input parameters: Input parameters:
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 ---- ----
-Ka2017x3inc_ejecta+==== Ka2017x3inc_ejecta ====
  
 Simple sum of three inclination-dependent Ka2017inc models. Simple sum of three inclination-dependent Ka2017inc models.
 The model does not include photon absorption or any kind of interaction between the different components. The model does not include photon absorption or any kind of interaction between the different components.
- 
  
 Input parameters: Input parameters:
-mej1 --> ejecta mass of component 1  +  mej1 --> ejecta mass of component 1  
-vej1 --> ejecta velocity of component 1 +  vej1 --> ejecta velocity of component 1 
-Xej1 --> lantganide raction of component 1  +  Xej1 --> lantganide raction of component 1  
-mej2 --> ejecta mass of component 2  +  mej2 --> ejecta mass of component 2  
-vej2 --> ejecta velocity of component 2  +  vej2 --> ejecta velocity of component 2  
-Xej2 --> lantganide raction of component 2 +  Xej2 --> lantganide raction of component 2 
-mej2 --> ejecta mass of component 3 +  mej2 --> ejecta mass of component 3 
-vej2 --> ejecta velocity of component 3 +  vej2 --> ejecta velocity of component 3 
-Xej2 --> lantganide raction of component 3 +  Xej2 --> lantganide raction of component 3 
-iota --> inclination angle+  iota --> inclination angle
  
-Bu2019_model_ejecta+---- 
 +==== Bu2019_model_ejecta ====
  
-Input parameters:  +Input parameters:   
-meh --> ejecta mass  +  mej --> ejecta mass  
-T --> temperature +  T --> temperature 
  
-Bu2019inc+---- 
 + 
 +==== Bu2019inc ====
  
 Input parameters:  Input parameters: 
-mej --> ejecta mass  +  mej --> ejecta mass  
-phi -->  +  phi --> angle between dynamical tidal and shock ejecta 
-theta --> +  theta --> viewing angle 
  
-Bu2019_op_model_ejecta+---- 
 + 
 +==== Bu2019_op_model_ejecta ====
  
 kappaLF, gammaLF, kappaLR, gammaLR kappaLF, gammaLF, kappaLR, gammaLR
  
  
-Bu2019_ops_model_ejecta+==== Bu2019_ops_model_ejecta ====
 kappaLF, kappaLR, gammaLR kappaLF, kappaLR, gammaLR
 +----
  
 +==== Bu2019lf
 +  mej_dyn -> dynamical ejecta 
 +  mej_wind --> wind ejecta 
 +  phi --> angle between shock and tidal ejecta 
 +  theta --> viewing angle 
  
-Bu2019lf +----
-mej_dyn,mej_wind,phi,theta+
  
 +==== Bu2019lr ====
  
-Bu2019lr +  mej_dyn -> dynamical ejecta  
-mej_dyn,mej_wind,phi,theta+  mej_wind --> wind ejecta  
 +  phi --> angle between shock and tidal ejecta  
 +  theta --> viewing angle 
  
  
-Bu2019lm +==== Bu2019lm ==== 
-mej_dyn,mej_wind,phi,theta+  mej_dyn -> dynamical ejecta  
 +  mej_wind --> wind ejecta  
 +  phi --> angle between shock and tidal ejecta  
 +  theta --> viewing angle 
  
 +==== Bu2019lw ====
  
-Bu2019lw +  mej_dyn -> dynamical ejecta  
-mej_wind,phi,theta+  mej_wind --> wind ejecta  
 +  phi --> angle between shock and tidal ejecta  
 +  theta --> viewing angle 
  
 +==== Bu2021ka_model_ejecta ====
  
-Bu2021ka_model_ejecta+  mej_dyn -> dynamical ejecta  
 +  mej_wind --> wind ejecta  
 +  phi --> angle between shock and tidal ejecta  
 +  theta --> viewing angle  
 +  kappa --> angle for opacity rescaling
  
-mej_dyn,mej_wind,phi,theta,kappa+----
  
 +==== Bu2019inc_TrPi2018 ====
  
-Bu2019inc_TrPi2018+Combination of Bulla2019_inc and TrPri2018, i.e., combining a GRB jet and a kilonova. 
  
 +---- 
  
-sn_model(z,t0,x0,x1,c):+==== TrPi2018_model ====
  
-boxfit_model(theta_0, E, n, theta_obs, p, epsilon_B, epsilon_E, ksi_N):+input parameters: theta_v, E0, theta_c, theta_w, n, p, epsilon_E, epsilon_B
  
-TrPi2018_model(theta_v, E0, theta_c, theta_w, n, p, epsilon_E, epsilon_B):+----  
 +==== Ka2017_TrPi2018_model ==== 
 +input parameters: mej,vej,Xlan,theta_v, E0, theta_c, theta_w, n, p, epsilon_E, epsilon_B
  
-Ka2017_TrPi2018_model(mej,vej,Xlan,theta_v, E0, theta_c, theta_w, n, p, epsilon_E, epsilon_B):+---- 
 +==== Bu2019inc_TrPi2018_model ==== 
 +input parameters: mej,phi,theta_v, E0, theta_c, theta_w, n, p, epsilon_E, epsilon_B
  
 +----
 +==== Ka2017_TrPi2018_A_model ====
 +input parameters: mej,vej,Xlan,theta_v, E0, theta_c, theta_w, n, p, epsilon_E, epsilon_B, A 
  
-Bu2019inc_TrPi2018_model(mej,phi,theta_v, E0, theta_c, theta_w, n, p, epsilon_E, epsilon_B): +---- 
- +==== Ka2017_A_model ==== 
-Ka2017_TrPi2018_A_model(mej,vej,Xlan,theta_v, E0, theta_c, theta_w, n, p, epsilon_E, epsilon_B, A): +input parameters: mej,vej,Xlan,A
- +
-Ka2017_A_model(mej,vej,Xlan,A) +
 Ka2017 model in which the total luminosity is scalled with an additional factor A, i.e., Ka2017 model in which the total luminosity is scalled with an additional factor A, i.e.,
 +
 L_{bol} = A * L_{Ka2017,bol} L_{bol} = A * L_{Ka2017,bol}
  
-Me2017_A_model(mej,vej,beta,kappa_r,A):+---- 
 + 
 +==== Me2017_A_model ==== 
 +input parameters: mej,vej,beta,kappa_r,A
 --> is a _ejecta model without the suffix --> is a _ejecta model without the suffix
  
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 L_{bol} = A * L_{Me2017,bol} L_{bol} = A * L_{Me2017,bol}
  
- 
-get_Wo2020dyn_model 
- 
-get_Wo2020dw_model 
  
Last modified: le 2021/08/04 23:52

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