Commit 2ec4c611 by Laura Ketzer

### evolved some more populations & worked on notebook to visualize the results

parent d9edc4c8
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 ... @@ -95,19 +95,16 @@ def mass_planet_RK4_forward_LO14(epsilon, K_on, beta_on, planet_object, initial_ ... @@ -95,19 +95,16 @@ def mass_planet_RK4_forward_LO14(epsilon, K_on, beta_on, planet_object, initial_ M_05k1 = M + 0.5*k1 M_05k1 = M + 0.5*k1 M_env_05k1 = M_05k1 - M_core M_env_05k1 = M_05k1 - M_core f_env_05k1 = (M_env_05k1/M_05k1)*100 # new mass fraction f_env_05k1 = (M_env_05k1/M_05k1)*100 # new mass fraction Mdot2 = mass_loss_rate_forward_LO14(t+0.5*dt, epsilon, K_on, beta_on, planet_object, f_env_05k1, track_dict) Mdot2 = mass_loss_rate_forward_LO14(t+0.5*dt, epsilon, K_on, beta_on, planet_object, f_env_05k1, track_dict) k2 = (dt*Myr_to_sec * Mdot2)/M_earth k2 = (dt*Myr_to_sec * Mdot2)/M_earth M_05k2 = M + 0.5*k2 M_05k2 = M + 0.5*k2 M_env_05k2 = M_05k2 - M_core M_env_05k2 = M_05k2 - M_core f_env_05k2 = (M_env_05k2/M_05k2)*100 # new mass fraction f_env_05k2 = (M_env_05k2/M_05k2)*100 # new mass fraction Mdot3 = mass_loss_rate_forward_LO14(t+0.5*dt, epsilon, K_on, beta_on, planet_object, f_env_05k2, track_dict) Mdot3 = mass_loss_rate_forward_LO14(t+0.5*dt, epsilon, K_on, beta_on, planet_object, f_env_05k2, track_dict) k3 = (dt*Myr_to_sec * Mdot3)/M_earth k3 = (dt*Myr_to_sec * Mdot3)/M_earth M_k3 = M + k3 M_k3 = M + k3 M_env_k3 = M_k3 - M_core M_env_k3 = M_k3 - M_core f_env_k3 = (M_env_k3/M_k3)*100 # new mass fraction f_env_k3 = (M_env_k3/M_k3)*100 # new mass fraction Mdot4 = mass_loss_rate_forward_LO14(t+dt, epsilon, K_on, beta_on, planet_object, f_env_k3, track_dict) Mdot4 = mass_loss_rate_forward_LO14(t+dt, epsilon, K_on, beta_on, planet_object, f_env_k3, track_dict) k4 = (dt*Myr_to_sec * Mdot4)/M_earth k4 = (dt*Myr_to_sec * Mdot4)/M_earth ... ...
 **result_files:** - OwWu17_smass_cks - OwWu17_smass_cks_lowerLx (here I fixed an issue with Lx and Lxuv -> Owen Lsat is XUV, so I needed to convert to Lx first, before passing into Platypos, since Platypos automatically converts from X-ray to XUV) t_start = 1 Myr t_final = 3 Gyr smass distr: mu=1.0, sigma=0.3 Mcore = 3 - OwWu17_smass_OwWusmass t_start = 1 Myr t_final = 3 Gyr smass distr: mu=1.3, sigma^2=0.3 Mcore = 3 - OwWu17_smass_cks_Mcore5: t_start = 1 Myr t_final = 3 Gyr smass distr: mu=1.0, sigma=0.3 Mcore = 5 - OwWu17_smass_cks_Mcore3_5Gyr t_start = 1 Myr t_final = 5 Gyr smass distr: mu=1.0, sigma=0.3 Mcore = 3 \ No newline at end of file
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