  After studying the energy-momentum relation of charged particles'
Hamilton-Jacobi equations, we discuss the laws of thermodynamics and the weak
cosmic censorship conjecture in torus-like black holes. We find that both the
first law of thermodynamic as well as the weak cosmic censorship conjecture are
valid in both the normal phase space and extended phase space. However, the
second law of thermodynamics is only valid in the normal phase space. Our
results show that the first law and weak cosmic censorship conjecture do not
depend on the phase spaces while the second law depends. What's more, we find
that the shift of the metric function that determines the event horizon take
the same form in different phase spaces, indicating that the weak cosmic
censorship conjecture is independent of the phase space.
