part ii s rg and low momentum interactions
play

Part II: (S)RG and Low-Momentum Interactions To understand the - PowerPoint PPT Presentation

Part II: (S)RG and Low-Momentum Interactions To understand the properties of complex nuclei from first principles Renormalizing NN Interactions Basic ideas of RG Low-momentum interactions Similarity RG interactions Benefits of low cutoffs


  1. Part II: (S)RG and Low-Momentum Interactions To understand the properties of complex nuclei from first principles Renormalizing NN Interactions Basic ideas of RG Low-momentum interactions Similarity RG interactions Benefits of low cutoffs G-matrix renormalization How will we approach this problem: QCD à à NN (3N) forces à à Renormalize à à “Solve” many-body problem à à Predictions

  2. Renormalization of Meson-Exchange Potentials Ok, high momentum is a pain. I wonder what would happen to low-energy observables… Low-to-high momentum makes life difficult for low-energy nuclear theorists, so let’s get rid of it Can we just make a sharp cut and see if it works? Sharp cut V filter ( k 0 , k ) ≡ 0; k, k 0 > 2 . 2 MeV

  3. Renormalization of Meson-Exchange Potentials Can we just make a sharp cut? · Nope! Low-energy physics is not correct 1 S 0 − 1 k = 2 fm 60 phase shift (degrees) AV18 phase shifts Glad I didn’t bet money 40 on that… I wonder what went wrong 20 0 after low-pass filter − 20 0 100 200 300 E lab (MeV)

  4. Renormalization of Meson-Exchange Potentials Can we just make a sharp cut? · Nope! Low-energy physics is not correct 1 S 0 − 1 k = 2 fm 60 phase shift (degrees) AV18 phase shifts Glad I didn’t bet money 40 on that… I wonder what went wrong 20 0 after low-pass filter − 20 0 100 200 300 E lab (MeV) Phase shifts involve couplings of low-to-high momenta Λ 1 h k | V | q ih q | V | k 0 i h k | V | q ih q | V | k 0 i X X h k | V | k 0 i + + ✏ k 0 � ✏ q ✏ k 0 � ✏ q q =0 q = Λ Lesson: Must ensure low-energy physics is preserved!

  5. Renormalization of Meson-Exchange Potentials To do properly, from T -matrix equation, define low-momentum equation: Lower UV cutoff, but preserve low-energy physics!

  6. Renormalization of Meson-Exchange Potentials To do properly, from T -matrix equation, define low-momentum equation: Require : d d Λ T = 0 Lower UV cutoff, but preserve low-energy physics! Leads to renormalization group equation for low-momentum interactions V Λ low k ( k 0 , Λ ) T Λ ( Λ , k ) d low k ( k 0 , k ) = 2 d Λ V Λ 1 − ( k/ Λ ) 2 π

  7. Renormalization of Meson-Exchange Potentials Run cutoff to lower values – decouples high-momentum modes Start from some initial V NN at high cutoff Λ 0 Λ ≈ Λ Data “Universality” at low momentum

  8. Renormalization of Meson-Exchange Potentials Diagonal Off-diagonal These are all our favorite OBE NN potentials… These are all our favorite OBE NN potentials… at low momentum Universal collapse in both diagonal/off-diagonal components, most partial waves

  9. Renormalization of Chiral EFT Potentials Diagonal Off-diagonal These are all our favorite Chiral EFT NN potentials… These are all our favorite Chiral EFT NN potentials… at low momentum Differences remain in off-diagonal matrix elements. Why?

  10. Renormalization of Chiral EFT Potentials Diagonal Off-diagonal These are all our favorite Chiral EFT NN potentials… These are all our favorite Chiral EFT NN potentials… at low momentum Differences remain in off-diagonal matrix elements Sensitive to agreement for phase shifts (not all fit perfectly)

  11. Renormalization of NN Potentials symbols: V low k " = 2 fm -1 Why is it mostly a shift? V e ff = V L + δ V c . t . ( Λ ) Overall effect of evolving to low momentum Main effect is shift in momentum space

  12. Renormalization of NN Potentials symbols: V low k " = 2 fm -1 Why is it mostly a shift? V e ff = V L + δ V c . t . ( Λ ) Overall effect of evolving to low momentum Main effect is shift in momentum space – delta function Removes hard core (unconstrained short-range physics)!

  13. Improvements in Perturbation Theory Explore improvements in symmetric infinite matter calculations Order by order in many-body perturbation theory (MBPT) No clear convergence with increasing order in bare potential

  14. Improvements in Perturbation Theory Explore improvements in symmetric infinite matter calculations Order by order in many-body perturbation theory (MBPT) No clear convergence with increasing order in bare potential Significant improvement with low-momentum interactions!

  15. Improvements in Perturbation Theory Explore improvements in symmetric infinite matter calculations Order by order in many-body perturbation theory (MBPT) Ok, the interactions look perturbative, but something is wrong here… No clear convergence with increasing order in bare potential Significant improvement with low-momentum interactions!

  16. Improvements in Perturbation Theory Explore improvements in symmetric infinite matter calculations Order by order in many-body perturbation theory (MBPT) Ok, the interactions look perturbative, but something is wrong here… No clear convergence with increasing order in bare potential Significant improvement with low-momentum interactions! Does not saturate – what might be missing?

  17. Improvements in Perturbation Theory H ( Λ ) = T + V NN ( Λ ) + V 3N ( Λ ) + V 4N ( Λ ) + · · · Ok, the interactions look perturbative, but something is wrong here… No clear convergence with increasing order in bare potential Significant improvement with low-momentum interactions! Does not saturate – what might be missing?

  18. Similarity Renormalization Group Wegner, Glazek/Wilson (1990s) Complementary method to decouple low from high momenta ails in lecture 2) (technical k ’ k ’ k k ! 2 ! 1 ! 2 ! 1 ! 0 ! 0 Similarity Renormalization Group Decouples high-momentum Drives Hamiltonian to band-diagonal

  19. Similarity Renormalization Group Wegner, Glazek/Wilson (1990s) Apply a continuous unitary transformation, parameterized by s: H = T + V → H ( s ) = U ( s ) HU † ( s ) ≡ T + V ( s ) where differentiating (exercise) yields: η ( s ) ≡ d U ( s ) d H ( s ) U † ( s ) where = [ η ( s ) , H ( s )] d s d s Never explicitly construct unitary transformation Instead choose generator to obtain desired behavior : η ( s ) = [ G ( s ) , H ( s )] Many options, e.g., Drives H(s) to band-diagonal form η ( s ) = [ T, H ( s )]

  20. Illustration of SRG Flow Drive H to band-diagonal form with kinetic-energy generator: η ( s ) = [ T, H ( s )] λ 2 = 1 With alternate definition of flow parameter: √ s 1 S 0 Argonne V 18 λ = 8 . 0 fm − 1

  21. Illustration of SRG Flow Drive H to band-diagonal form with standard choice: η ( s ) = [ T, H ( s )] λ 2 = 1 With alternate definition of flow parameter: √ s 1 S 0 Argonne V 18 λ = 4 . 0 fm − 1

  22. Illustration of SRG Flow Drive H to band-diagonal form with standard choice: η ( s ) = [ T, H ( s )] λ 2 = 1 With alternate definition of flow parameter: √ s 1 S 0 Argonne V 18 λ = 3 . 0 fm − 1

  23. Illustration of SRG Flow Drive H to band-diagonal form with standard choice: η ( s ) = [ T, H ( s )] λ 2 = 1 With alternate definition of flow parameter: √ s 1 S 0 Argonne V 18 λ = 2 . 5 fm − 1

  24. Illustration of SRG Flow Drive H to band-diagonal form with standard choice: η ( s ) = [ T, H ( s )] λ 2 = 1 With alternate definition of flow parameter: √ s 1 S 0 Argonne V 18 λ = 2 . 0 fm − 1

  25. Other Generator Choices: Block Diagonal Create block diagonal form like V lowk ? ✓ ◆ PH ( s ) P 0 G ( s ) = H BD = 0 QH ( s ) Q With alternate definition of flow parameter: λ 2 = 1 √ s 3 S 1 λ = 10 . 0 fm − 1 Argonne V 18

  26. Other Generator Choices: Block Diagonal Create block diagonal form like V lowk ? ✓ ◆ PH ( s ) P 0 G ( s ) = H BD = 0 QH ( s ) Q With alternate definition of flow parameter: λ 2 = 1 √ s 3 S 1 λ = 5 . 0 fm − 1 Argonne V 18

  27. Other Generator Choices: Block Diagonal Create block diagonal form like V lowk ? ✓ ◆ PH ( s ) P 0 G ( s ) = H BD = 0 QH ( s ) Q With alternate definition of flow parameter: λ 2 = 1 √ s 3 S 1 λ = 2 . 0 fm − 1 Argonne V 18

  28. SRG Renormalization of Chiral EFT Potentials ⇒ ≈ Diagonal V λ ( k , k ) Off-Diagonal V λ ( k , 0 ) 1.0 1.0 − 1 − 1 λ = 5.0 fm λ = 5.0 fm 0.5 1 S 0 0.5 1 S 0 These are all our 0.0 0.0 V λ (k,k) [fm] V λ (k,0) [fm] favorite Chiral EFT − 0.5 − 0.5 NN potentials… − 1.0 − 1.0 550/600 [E/G/M] 550/600 [E/G/M] 600/700 [E/G/M] 600/700 [E/G/M] − 1.5 − 1.5 500 [E/M] 500 [E/M] 600 [E/M] 600 [E/M] − 2.0 − 2.0 0.0 0.5 1.0 1.5 2.0 2.5 3.0 3.5 0.0 0.5 1.0 1.5 2.0 2.5 3.0 3.5 − 1 ] − 1 ] Diagonal V λ k k Off-Diagonal V λ k 0 k [fm k [fm 1.0 1.0 − 1 − 1 λ = 1.5 fm λ = 1.5 fm These are all our 0.5 1 S 0 0.5 1 S 0 favorite Chiral EFT 0.0 0.0 V λ (k,k) [fm] V λ (k,0) [fm] NN potentials… − 0.5 − 0.5 SRG evolved − 1.0 − 1.0 550/600 [E/G/M] 550/600 [E/G/M] 600/700 [E/G/M] 600/700 [E/G/M] − 1.5 − 1.5 500 [E/M] 500 [E/M] 600 [E/M] 600 [E/M] − 2.0 − 2.0 0.0 0.5 1.0 1.5 2.0 2.5 3.0 3.5 0.0 0.5 1.0 1.5 2.0 2.5 3.0 3.5 − 1 ] − 1 ] k [fm k [fm Exhibit similar “universal” behavior as low-momentum interactions!

  29. Renormalization of Nuclear Interactions H ( Λ ) = T + V NN ( Λ ) + V 3N ( Λ ) + V 4N ( Λ ) + · · · Evolve momentum resolution scale of chiral interactions from initial Λ χ Remove coupling to high momenta, low-energy physics unchanged Bogner, Kuo, Schwenk, Furnstahl AV AV 18 18 Universal at low-momentum N 3 LO LO V low k ( Λ ): lower cutoffs advantageous for nuclear structure calculations

Download Presentation
Download Policy: The content available on the website is offered to you 'AS IS' for your personal information and use only. It cannot be commercialized, licensed, or distributed on other websites without prior consent from the author. To download a presentation, simply click this link. If you encounter any difficulties during the download process, it's possible that the publisher has removed the file from their server.

Recommend


More recommend