Quantum refrigerator embedded in spin-star environments: Scalings of temperature and refrigeration time

We examine a quantum absorption refrigerator that comprises three qubits, each of which is connected with a separate spin-star environment. The refrigerator exhibits the feature of transient cooling, i.e., lowering of the temperature of the first qubit in sufficiently small timescales. Since the spin-star environment is inherently non-Markovian in nature, steady-state cooling is not achieved. A key advantage of our model is that the symmetries of the Hamiltonian enable a solution of the reduced density matrices of the refrigerator qubits, even in the presence of a large number of environmental spins. We derive the condition for autonomous refrigeration and analyze how the optimal cold qubit temperature scales with the number of bath qubits. We find a power law scaling towards a constant asymptotic value. We also find the scaling of the minimum time required for cooling as a function of the number of bath spins. Further, we scrutinize the heat currents associated with each of the three qubits.