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Assumptions (1) and (2) do not affect the spacing between the peaks in G, but they do affect the relative peak heights at BZ =0. The peak spacings contain enough information to extract all the energy splittings illustrated in Fig. 5.
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The case Γ2 / Γ1 =1 is clearly outside the region of validity of our Γ2 / Γ1 1 treatment but is included in the plot nonetheless in order to make the trends clear.
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In a finite system, a naive estimate gives a ΔR / TK finite-size correction to the local susceptibility from the second term in Eq. 23.
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The spin-chain mapping (Refs.) of Ref. is easily modified to simulate the canonical ensemble for the Kondo problem. Fixing the number of fermions in the Kondo box corresponds to simulating the spin chain at fixed magnetization, while the grand-canonical case corresponds to a fixed magnetic field. During the loop update, the magnetization of the spin chain is updated when loops wrap around the imaginary time direction (they have temporal winding). If we prevent our loops from winding temporally, the magnetization of the spin chain stays fixed, and we are simulating the canonical ensemble in the Kondo problem. A simple approach to restricting loops to the zero temporal winding sector is to finish the growth of a loop and then reject loops that wind in time. A more efficient approach and the one that we have used here is to force the loops to bounce back if they cross a certain time slice. It is possible to show that this algorithm satisfies detailed balance and at the same time forbids temporal winding.
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