Trim trailing whitespace

EOS/breakout/actual_eos.H

@@ -130,7 +130,7 @@ void actual_eos (I input, T& state)
             }
         }
 
-        // Try to avoid the expensive log function.  Since we don't need entropy 
+        // Try to avoid the expensive log function.  Since we don't need entropy
         // in hydro solver, set it to an invalid but "nice" value for the plotfile.
         if constexpr (has_entropy<T>::value) {
             state.s = 1.0_rt;

EOS/eos_composition.H

@@ -26,7 +26,7 @@ struct eos_xderivs_t {
 /// The auxiliary state provides an alternate description to the composition,
 /// in terms of Ye, abar, and binding energy / nucleon
 ///
-template <class state_t> 
+template <class state_t>
 AMREX_GPU_HOST_DEVICE AMREX_INLINE
 void set_aux_comp_from_X(state_t& state) {
 

EOS/helmholtz/actual_eos.H

@@ -29,13 +29,13 @@ using namespace eos_rp;
 // derivatives), number density of electrons and positron pair (along
 // with their derivatives), adiabatic indices, specific heats, and
 // relativistically correct sound speed are also returned.
-// 
+//
 // this routine assumes planckian photons, an ideal gas of ions,
 // and an electron-positron gas with an arbitrary degree of relativity
 // and degeneracy. interpolation in a table of the helmholtz free energy
 // is used to return the electron-positron thermodynamic quantities.
 // all other derivatives are analytic.
-// 
+//
 // references: cox & giuli chapter 24 ; timmes & swesty apj 1999
 
 const std::string eos_name = "helmholtz";
@@ -510,7 +510,7 @@ void apply_ions (T& state)
     Real sion    = (pion * deni + eion) * tempi + kergavo * ytot1 * y;
     Real dsiondd = (dpiondd * deni - pion * deni * deni + deiondd) * tempi -
                    kergavo * deni * ytot1;
-    Real dsiondt = (dpiondt * deni + deiondt) * tempi -  
+    Real dsiondt = (dpiondt * deni + deiondt) * tempi -
                    (pion * deni + eion) * tempi * tempi +
                    1.5e0_rt * kergavo * tempi * ytot1;
 
@@ -759,7 +759,7 @@ void apply_coulomb_corrections (T& state)
         decoulda = s * dpcoulda;
         decouldz = s * dpcouldz;
 
-        s        = -avo_eos * kerg / (state.abar * plasg) * 
+        s        = -avo_eos * kerg / (state.abar * plasg) *
                     (1.5e0_rt * c2 * x - a2 * (b2 - 1.0e0_rt) * y);
         dscouldd = s * plasgdd;
         dscouldt = s * plasgdt;

EOS/polytrope/actual_eos.H

@@ -39,7 +39,7 @@ void actual_eos_init ()
     // Available pre-defined polytrope options:
 
     // 1: Non-relativistic, fully degenerate electron gas
-    // 2: Relativistic, fully degenerate electron gas 
+    // 2: Relativistic, fully degenerate electron gas
 
     if (polytrope_type > 0) {
         mu_e = polytrope_mu_e;
@@ -88,7 +88,7 @@ bool is_input_valid (I input)
 
 
 //---------------------------------------------------------------------------
-// Public interfaces 
+// Public interfaces
 //---------------------------------------------------------------------------
 
 inline

EOS/ztwd/actual_eos.H

@@ -1,10 +1,10 @@
 #ifndef ACTUAL_EOS_H
 #define ACTUAL_EOS_H
 
-// This is the equation of state for zero-temperature white dwarf 
+// This is the equation of state for zero-temperature white dwarf
 // matter composed of degenerate electrons:
 // P = A * (x * (2x**2 - 3)(x**2 + 1)**1/2 + 3 sinh**-1(x))
-// 
+//
 // where rho = B x**3 and the constants are given by:
 //
 // A = pi m_e**4 c**5 / (3 h**3) = 6.0 x 10^22 dyne cm**-2
@@ -16,7 +16,7 @@
 // h = (8A / B) (1 + x**2)**(1/2)
 //
 // The internal energy is calculated using the standard relation:
-// 
+//
 // h = e + P / rho
 
 #include <AMReX.H>
@@ -26,7 +26,7 @@
 using namespace amrex;
 
 const std::string eos_name = "ztwd";
-  
+
 const Real A = M_PI * std::pow(C::m_e, 4) * std::pow(C::c_light, 5) / (3.0_rt * std::pow(C::hplanck, 3));
 const Real B2 = 8.0_rt * M_PI * std::pow(C::m_e, 3) * std::pow(C::c_light, 3) * C::m_p  / (3.0_rt * std::pow(C::hplanck, 3));
 const Real iter_tol = 1.e-10_rt;

conductivity/stellar/actual_conductivity.H

@@ -41,7 +41,7 @@ actual_conductivity (T& state)
   // ocond  = conductive contribution to the opacity (in cm**2/g)
   // opac   = the total opacity (in cm**2/g)
   // conductivity = thermal conductivity (in erg/cm/K/sec)
-  // 
+  //
 
     // various physical and derived constants
     // con2 = con1*sqrt(4*pi*e*e/me)

constants/fundamental_constants.H

@@ -50,10 +50,10 @@ namespace C
 
     // mass of electron
     constexpr amrex::Real m_e = 9.10938291e-28;  // g
-  
+
     // atomic mass unit
     constexpr amrex::Real m_u = 1.6605390666e-24; // g
-  
+
     // electron charge
     // NIST: q_e = 1.602176565e-19 C
     //

integration/VODE/actual_integrator.H

@@ -93,7 +93,7 @@ void actual_integrator (BurnT& state, Real dt)
     integrator_to_burn(vode_state, state);
 
 #ifdef NSE
-    // compute the temperature based on the energy release -- we need 
+    // compute the temperature based on the energy release -- we need
     // this in case we failed in our burn here because we entered NSE
 
 #ifdef AUX_THERMO

integration/VODE/vode_dvstep.H

@@ -247,7 +247,7 @@ int dvstep (BurnT& state, DvodeT& vstate)
                 (std::abs(vstate.y(i)) > vode_increase_change_factor * std::abs(y_save(i)) ||
                  std::abs(vstate.y(i)) < vode_decrease_change_factor * std::abs(y_save(i)))) {
 #ifdef MICROPHYSICS_DEBUG
-#ifndef AMREX_USE_GPU 
+#ifndef AMREX_USE_GPU
                std::cout << "rejecting step based on species " << i << " from " << y_save(i) << " to " << vstate.y(i) << std::endl;
 #endif
 #endif

integration/integrator_type.H

@@ -18,7 +18,7 @@ void update_density_in_time(const Real time, BurnT& state)
     //
     // we are always integrating from t = 0, so there is no offset
     // time needed here.  The indexing of ydot_a is based on
-    // the indices in burn_t and is 0-based    
+    // the indices in burn_t and is 0-based
     state.y[SRHO] = amrex::max(state.rho_orig + state.ydot_a[SRHO] * time, EOSData::mindens);
 
     // for consistency

interfaces/burn_type.H

@@ -249,7 +249,7 @@ void eos_to_burn (const T& eos_state, BurnT& burn_state)
 
 
 
-// Given a burn type, copy the data relevant to the eos type. 
+// Given a burn type, copy the data relevant to the eos type.
 // Note that when doing simplified SDC integration, we should
 // avoid using this interface because the energy includes a
 // contribution from the advection term. However this is useful
@@ -315,7 +315,7 @@ AMREX_GPU_HOST_DEVICE AMREX_FORCE_INLINE
 void normalize_abundances_sdc_burn (BurnT& state)
 {
 
-    // Constrain the partial densities in burn_t state to sum to the 
+    // Constrain the partial densities in burn_t state to sum to the
     // density.
     //
     // This is meant to be used upon exit, and we assume that

interfaces/eos_type.H

@@ -109,7 +109,7 @@ struct eos_rep_t:eos_base_t {
 
     amrex::Real abar{};
     amrex::Real zbar{};
-  
+
 #ifdef NSE_NET
     amrex::Real mu_p{};   //chemical potential of proton
     amrex::Real mu_n{};   //chemical potential of neutron

interfaces/tfactors.H

@@ -68,10 +68,10 @@ struct tf_t {
     amrex::Real lnt9;
 };
 
-AMREX_GPU_HOST_DEVICE inline 
+AMREX_GPU_HOST_DEVICE inline
 tf_t get_tfactors(amrex::Real temp)
 {
-    tf_t tf; 
+    tf_t tf;
 
     tf.temp = temp;
 
@@ -82,13 +82,13 @@ tf_t get_tfactors(amrex::Real temp)
     // tf.t95   = tf.t9*tf.t94;
     tf.t95   = tf.t92*tf.t93;
     // tf.t96   = tf.t9*tf.t95;
-    
+
     tf.t912  = std::sqrt(tf.t9);
     tf.t932  = tf.t9*tf.t912;
     tf.t952  = tf.t9*tf.t932;
     // tf.t972  = tf.t9*tf.t952;
     tf.t972  = tf.t92*tf.t932;
-    
+
     tf.t913  = std::cbrt(tf.t9);
     tf.t923  = tf.t913*tf.t913;
     tf.t943  = tf.t9*tf.t913;
@@ -100,51 +100,51 @@ tf_t get_tfactors(amrex::Real temp)
     // tf.t934  = tf.t914*tf.t914*tf.t914;
     // tf.t954  = tf.t9*tf.t914;
     // tf.t974  = tf.t9*tf.t934;
-    
+
     // tf.t915  = std::pow(tf.t9, 0.2_rt);
     // tf.t935  = tf.t915*tf.t915*tf.t915;
     // tf.t945  = tf.t915 * tf.t935;
     // tf.t965  = tf.t9 * tf.t915;
-    
+
     // tf.t916  = std::pow(tf.t9, 1.0_rt/6.0_rt);
     // tf.t976  = tf.t9 * tf.t916;
     // tf.t9i76 = 1.0e0_rt/tf.t976;
-    
+
     // tf.t917  = std::pow(tf.t9, 1.0_rt/7.0_rt);
     // tf.t927  = tf.t917*tf.t917;
     // tf.t947  = tf.t927*tf.t927;
-    
+
     // tf.t918  = std::sqrt(tf.t914);
     // tf.t938  = tf.t918*tf.t918*tf.t918;
     // tf.t958  = tf.t938*tf.t918*tf.t918;
-    
+
     tf.t9i   = 1.0e0_rt/tf.t9;
     tf.t9i2  = tf.t9i*tf.t9i;
     // tf.t9i3  = tf.t9i2*tf.t9i;
-    
+
     tf.t9i12 = 1.0e0_rt/tf.t912;
     tf.t9i32 = tf.t9i*tf.t9i12;
     // tf.t9i52 = tf.t9i*tf.t9i32;
     // tf.t9i72 = tf.t9i*tf.t9i52;
-    
+
     tf.t9i13 = 1.0e0_rt/tf.t913;
     tf.t9i23 = tf.t9i13*tf.t9i13;
     tf.t9i43 = tf.t9i*tf.t9i13;
     tf.t9i53 = tf.t9i*tf.t9i23;
-    
+
     // tf.t9i14 = 1.0e0_rt/tf.t914;
     // tf.t9i34 = tf.t9i14*tf.t9i14*tf.t9i14;
     // tf.t9i54 = tf.t9i*tf.t9i14;
-    
+
     // tf.t9i15 = 1.0e0_rt/tf.t915;
     // tf.t9i35 = tf.t9i15*tf.t9i15*tf.t9i15;
     // tf.t9i45 = tf.t9i15 * tf.t9i35;
     // tf.t9i65 = tf.t9i*tf.t9i15;
-    
+
     // tf.t9i17 = 1.0e0_rt/tf.t917;
     // tf.t9i27 = tf.t9i17*tf.t9i17;
     // tf.t9i47 = tf.t9i27*tf.t9i27;
-    
+
     // tf.t9i18 = 1.0e0_rt/tf.t918;
     // tf.t9i38 = tf.t9i18*tf.t9i18*tf.t9i18;
     // tf.t9i58 = tf.t9i38*tf.t9i18*tf.t9i18;

networks/aprox13/actual_network.H

@@ -174,7 +174,7 @@ namespace Rates {
 }
 
 namespace RHS {
-    
+
     AMREX_GPU_HOST_DEVICE AMREX_INLINE
     constexpr rhs_t rhs_data (int rate)
     {

networks/aprox19/actual_network.H

@@ -230,7 +230,7 @@ namespace Rates {
 }
 
 namespace RHS {
-    
+
     AMREX_GPU_HOST_DEVICE AMREX_INLINE
     constexpr rhs_t rhs_data (int rate)
     {

networks/aprox21/actual_network.H

@@ -226,7 +226,7 @@ namespace Rates {
 }
 
 namespace RHS {
-    
+
     AMREX_GPU_HOST_DEVICE AMREX_INLINE
     constexpr rhs_t rhs_data (int rate)
     {

networks/rhs.H

@@ -78,7 +78,7 @@ constexpr int is_rate_used ()
 
 // Determine the index of a given intermediate reaction. We use the
 // order of the original rate definitions
-    
+
 // Counts up the number of intermediate reactions. An intermediate
 // reaction is defined as any reaction which contributes to the
 // construction of some other reaction. Note that an intermediate

networks/triple_alpha_plus_cago/actual_network.H

@@ -102,7 +102,7 @@ namespace Rates
 };
 
 namespace RHS {
-    
+
     AMREX_GPU_HOST_DEVICE AMREX_INLINE
     constexpr rhs_t rhs_data (int rate)
     {