Finite-size errors in QMC
From QMC
Discussion during CECAM QMC Workshop 2007
Contents |
[edit] Introduction
- Without twist averaging, what is the best way to get finite k-pt correction from DFT or HF?
- Pros and cons of MPC vs S(k)
- Is the quadratic coefficient at k=0?
- Residual correction 1/N?
- Kinetic energy correction form Jastrow.
- Any additional problems for charged defects.
[edit] R. Needs
[edit] Two approaches for removing Coulomb finite-size effects
- MPC: PRB 53, 1814 (1996); PRB 55 R4851 (1997)
- Interaction of electrons with their exchange-correlation holes should be exactly 1/r, but Ewald interaction converges only slowly to 1/4
- Use Ewald interaction to evaluate Hartree energy
- Use 1/r interaction within minimum image convention to evaluate interaction of each electron with its exchange-correlation hole.
- Chiesa correction (think in reciprocal space): PRL 97, 076404 (2006)
- Leading-order error due to omission of G=0
[edit] Equivalence of the two approaches
- MPC is perfect if exchange-correlation hole fits into simulation cell; addition the Chiesa correction to the Ewalk energy is an approximation to the MPC.
- If exchange-correlation hole does not fit into simulation cell, MPC is not perfect; Chiesa correction can still make use of the known form of the structure factor at small k.
- The two approaches give very similar results in practice.
[edit] Conclusions
- Leading-order Chiesa kinetic-energy correction works well at low densities but not high density.
- Real-space method for k-point sampling errors?
[edit] D. Ceperley
[edit] Condensed version of PRL 97, 076404 (2006)
- Coulomb correction:
- Kinetic-energy correction:
- Key region is at
and others
- Make an interpolation, e.g.,
[edit] R. Gaudoin
Modeling the spherically averaged structure factor
