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Introduction
The holographic duality provides a unique method to investigate the dynamics of strongly coupled field theories, which links geometrical quantities to quantum observables. The uses of this interplay to study thermal phases of strongly coupled field theories by their holographically dual AdS black hole/brane geometries have attracted lots of attention since it was first porposed. It was then suggested that the small perturbations of the AdS metric are dual to the hydrodynamics or linear response theories of the boundary CFTs. Also, by probed strings in the AdS background, the diffusion behavior of Brownian particles in the boundary fields can be derived. In particular, the time evolution of entanglement entropy between Brownian particles and boundary fields had been studied by means of the probed string method.
lr_xp_fitting=0.03#0.03
lair=0.1irc=0cm=10uvd=0.1optimizer_exp_fitting=optim.Adam(model_fitting.parameters(),lr=lr_xp_fitting)#RMSprop #Adam
MSELoss=nn.MSELoss()defbuild_train_step_exp_fitting(model,loss_fn,optimizer):deftrain_step_exp_fitting(eta,phi,pi,y):#Training Model
model_fitting.train()# Prediction
yhat=model_fitting(eta,phi,pi)#Computing Loss Function
loss=loss_fn(y,yhat[0])+lair*yhat[1]+yhat[2]#Computing Gradient
loss.backward()#Optimization
optimizer.step()optimizer.zero_grad()returnloss.item()returntrain_step_exp_fittingtrain_step_exp_fitting=build_train_step_exp_fitting(model_fitting,MSELoss,optimizer_exp_fitting)print(model_fitting.state_dict())
plt.plot(loss_epoch,lw=2,label='Loss Function')plt.title('Time Evolution of Loss Function')plt.legend(bbox_to_anchor=(1.05,1),loc='upper left',borderaxespad=0.)plt.xlabel('epoch')plt.ylabel('Loss Function')plt.tight_layout()plt.savefig("loss_rnq09_3n_1.png")plt.show()
deft(F):signr=np.heaviside(F-ir_cutoff,0)signl=np.heaviside(-F-ir_cutoff,0)returnsignr+signlFp=np.arange(-0.6,0.6,0.001)#step
plt.plot(Fp,t(Fp),lw=5,label='$t(F)$')plt.title('Function of Final Layer')plt.legend(bbox_to_anchor=(1.05,1),loc='upper left',borderaxespad=0.)plt.xlabel('F')plt.ylabel('$t(F)$')#plt.tight_layout()
#plt.savefig("Tanh.png")
plt.show()
Setup
We consider the scalar field only dependent on the holographic direction
in asymptotic AdS black hole background
where the emblackening function have following properties
Specially,
in RN case. Note that, in extremal case, .
Reproduced Metric and EoM
The EoM for is
Now, we’re wanna let . Consider the following coordinate transformation