many-nucleon interactions via the srg trento, italy july 13, 2011

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Lawrence Livermore National Laboratory Physical and Life Sciences/Physics Many-Nucleon Interactions via the SRG Trento, Italy July 13, 2011 Eric Jurgenson Collaborators: P. Maris, R. Furnstahl, P. Navratil, E. Ormand, J. Vary Prepared by LLNL under Contract DE-AC52-07NA27344 Performance Measures x.x, x.x, and x.x

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Performance Measures x.x, x.x, and x.x. Many-Nucleon Interactions via the SRG Trento, Italy July 13, 2011. Eric Jurgenson Collaborators: P. Maris, R. Furnstahl, P. Navratil, E. Ormand, J. Vary. Prepared by LLNL under Contract DE-AC52-07NA27344. Ab initio: from the begining. Start with χEFTs - PowerPoint PPT Presentation

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Page 1: Many-Nucleon Interactions via the SRG Trento, Italy July 13, 2011

Lawrence Livermore National Laboratory

Physical and Life Sciences/Physics

Many-Nucleon Interactions via the SRGTrento, Italy

July 13, 2011

Eric JurgensonCollaborators: P. Maris, R. Furnstahl, P. Navratil, E. Ormand, J. Vary

Prepared by LLNL under Contract DE-AC52-07NA27344

Performance Measures x.x, x.x, and x.x

Page 2: Many-Nucleon Interactions via the SRG Trento, Italy July 13, 2011

2Option:UCRL# S&T – PLS/Physics

Ab initio: from the begining

Start with χEFTs SRG is well suited to the many-

body hierarchy

Page 3: Many-Nucleon Interactions via the SRG Trento, Italy July 13, 2011

3Option:UCRL# S&T – PLS/Physics

What is the Similarity Renormalization Group (SRG) ?

PRC 75,061001 (2007) [arXiv: nucl-th/0611045]

Hs = UsHUs+ ≡ Trel + Vs

s = 1λ4( )

ηs = [Gs,Hs] ⇒ dHs

ds= T,Hs[ ],Hs[ ]

Unitary Transformations:

dHs

ds= [η s,Hs] where

ηs = dUs

dsUs

+ = −η s+

Implement as flow equations

With Gs any Hermitian operator

Gs = Trel ,Hdiag ,Hosc,HBD,T +VNN ,exp[T],L

Page 4: Many-Nucleon Interactions via the SRG Trento, Italy July 13, 2011

4Option:UCRL# S&T – PLS/Physics

SRG evolves Hamiltonians unitarily

Hs = UsHUs+ ⇒ dHs

ds= T,Hs[ ],Hs[ ]

s = 1λ4( )

Page 5: Many-Nucleon Interactions via the SRG Trento, Italy July 13, 2011

5Option:UCRL# S&T – PLS/Physics

SRG evolves Hamiltonians unitarily

Hs = UsHUs+ ⇒ dHs

ds= T,Hs[ ],Hs[ ]

s = 1λ4( )

Page 6: Many-Nucleon Interactions via the SRG Trento, Italy July 13, 2011

6Option:UCRL# S&T – PLS/Physics

SRG evolves Hamiltonians unitarily

Hs = UsHUs+ ⇒ dHs

ds= T,Hs[ ],Hs[ ]

s = 1λ4( )

Page 7: Many-Nucleon Interactions via the SRG Trento, Italy July 13, 2011

7Option:UCRL# S&T – PLS/Physics

SRG evolves Hamiltonians unitarily

Hs = UsHUs+ ⇒ dHs

ds= T,Hs[ ],Hs[ ]

s = 1λ4( )

Page 8: Many-Nucleon Interactions via the SRG Trento, Italy July 13, 2011

8Option:UCRL# S&T – PLS/Physics

SRG evolves Hamiltonians unitarily

Hs = UsHUs+ ⇒ dHs

ds= T,Hs[ ],Hs[ ]

s = 1λ4( )

Page 9: Many-Nucleon Interactions via the SRG Trento, Italy July 13, 2011

9Option:UCRL# S&T – PLS/Physics

SRG evolves Hamiltonians unitarily

Hs = UsHUs+ ⇒ dHs

ds= T,Hs[ ],Hs[ ]

s = 1λ4( )

Page 10: Many-Nucleon Interactions via the SRG Trento, Italy July 13, 2011

10Option:UCRL# S&T – PLS/Physics

SRG evolves Hamiltonians unitarily

Hs = UsHUs+ ⇒ dHs

ds= T,Hs[ ],Hs[ ]

s = 1λ4( )

Page 11: Many-Nucleon Interactions via the SRG Trento, Italy July 13, 2011

11Option:UCRL# S&T – PLS/Physics

SRG evolves Hamiltonians unitarily

Hs = UsHUs+ ⇒ dHs

ds= T,Hs[ ],Hs[ ]

s = 1λ4( )

Page 12: Many-Nucleon Interactions via the SRG Trento, Italy July 13, 2011

12Option:UCRL# S&T – PLS/Physics

SRG evolves Hamiltonians unitarily

Hs = UsHUs+ ⇒ dHs

ds= T,Hs[ ],Hs[ ]

s = 1λ4( )

Page 13: Many-Nucleon Interactions via the SRG Trento, Italy July 13, 2011

13Option:UCRL# S&T – PLS/Physics

SRG evolves Hamiltonians unitarily

Hs = UsHUs+ ⇒ dHs

ds= T,Hs[ ],Hs[ ]

s = 1λ4( )

Page 14: Many-Nucleon Interactions via the SRG Trento, Italy July 13, 2011

14Option:UCRL# S&T – PLS/Physics

SRG evolves Hamiltonians unitarily

Hs = UsHUs+ ⇒ dHs

ds= T,Hs[ ],Hs[ ]

s = 1λ4( )

Page 15: Many-Nucleon Interactions via the SRG Trento, Italy July 13, 2011

15Option:UCRL# S&T – PLS/Physics

SRG evolves Hamiltonians unitarily

Hs = UsHUs+ ⇒ dHs

ds= T,Hs[ ],Hs[ ]

s = 1λ4( )

Page 16: Many-Nucleon Interactions via the SRG Trento, Italy July 13, 2011

16Option:UCRL# S&T – PLS/Physics

SRG evolves Hamiltonians unitarily

Hs = UsHUs+ ⇒ dHs

ds= T,Hs[ ],Hs[ ]

s = 1λ4( )

Page 17: Many-Nucleon Interactions via the SRG Trento, Italy July 13, 2011

17Option:UCRL# S&T – PLS/Physics

Many-Body Forces (ANFs)

ANFs arise from eliminating DoF’s Omitting them leads to model

dependence (Tjon line) 3NF help saturate nuclear matter All many-body methods must deal

with them SRG induces ANFs! :

dHs

ds= a+a, a+a+aa

2−body1 2 3 ∑∑

⎣ ⎢

⎦ ⎥, a+a + a+a+aa

2−body1 2 3 ∑

⎣ ⎢ ⎢

⎦ ⎥ ⎥=K + a+a+a+aaa

3−body1 2 4 3 4 +K

RG flows extend consistently to many-body spaces State of the art now includes evolved 3NFs!

Page 18: Many-Nucleon Interactions via the SRG Trento, Italy July 13, 2011

18Option:UCRL# S&T – PLS/Physics

Triton

SRG improves convergence

PRL 103, 82501 (2009) [arXiv: 09005.1873]

Page 19: Many-Nucleon Interactions via the SRG Trento, Italy July 13, 2011

19Option:UCRL# S&T – PLS/Physics

Helium

SRG induces many-body forces – how big are they?

PRL 103, 82501 (2009) [arXiv: 09005.1873]

Page 20: Many-Nucleon Interactions via the SRG Trento, Italy July 13, 2011

20Option:UCRL# S&T – PLS/Physics

Convergence in 6Li

Increased NA2max to 300 and NA3max to 40 Simple extrapolations show spread in λ Example here for one ħΩ – need optimal for each λ

Page 21: Many-Nucleon Interactions via the SRG Trento, Italy July 13, 2011

21Option:UCRL# S&T – PLS/Physics

Lithium

Optimal ħΩ shifts with evolution

Extrapolations use this info Error bars are consistent

with previous work λ dependence reduced from 4 to <1 MeV

PRC, to appear [arXiv: 1011.4085]

Page 22: Many-Nucleon Interactions via the SRG Trento, Italy July 13, 2011

22Option:UCRL# S&T – PLS/Physics

Carbon

Difference is subtle here but trackable - plot difference of λ=1.5 - 2.2 vs. parameters

Page 23: Many-Nucleon Interactions via the SRG Trento, Italy July 13, 2011

23Option:UCRL# S&T – PLS/Physics

Nmax/ħΩ dependence

Interesting spread behavior in the basis space Clues to the source of convergence artifacts

Page 24: Many-Nucleon Interactions via the SRG Trento, Italy July 13, 2011

24Option:UCRL# S&T – PLS/Physics

New Generators

Scale c3 and c4

Plot the effect on the spread

Many choices of Gs

HO basis complicates the choice

More to come…

Page 25: Many-Nucleon Interactions via the SRG Trento, Italy July 13, 2011

25Option:UCRL# S&T – PLS/Physics

Hierarchy Preservation: A=3

Show hierarchy and suppression of high momentum strength

Expectation values of contributions to evolution

d V3

dλ= V 2,V2[ ] − V 3,V3[ ]

PRC, to appear [arXiv: 1011.4085]

Page 26: Many-Nucleon Interactions via the SRG Trento, Italy July 13, 2011

26Option:UCRL# S&T – PLS/Physics

Hierarchy Preservation: A=4

Repeat for A=4 Well defined hierarchy No positive feedback loops

d V4

dλ= V 2,V3[ ] + V 3,V2[ ] + V 3,V3[ ] − V 4 ,V4[ ]

Page 27: Many-Nucleon Interactions via the SRG Trento, Italy July 13, 2011

27Option:UCRL# S&T – PLS/Physics

Hierarchy Preservation: induced vs. initial 3NF

Compare Initial with Induced Similar composition of contributions

Page 28: Many-Nucleon Interactions via the SRG Trento, Italy July 13, 2011

28Option:UCRL# S&T – PLS/Physics

Carbon Revisited

Induced ANFs are as expected from existing work

Extrapolation in ħΩ should show reduction in spread

Larger systems are needed to determine 3/4NF needs…

Page 29: Many-Nucleon Interactions via the SRG Trento, Italy July 13, 2011

29Option:UCRL# S&T – PLS/Physics

Adding 3NFs to the many-body problem…

Coupled Cluster (CC)

Density Functional Theory (DFT)

NCSM/RGM (reactions)

Page 30: Many-Nucleon Interactions via the SRG Trento, Italy July 13, 2011

30Option:UCRL# S&T – PLS/Physics

Conclusion

Recap SRG improves convergence Variational and model space

independent Truncations are well

understood/controlled Induced forces are of natural

size, though details still to be investigated

Great freedom in SRG form for such work

Outlook Monitor hierarchy of induced

higher-body forces (MFDn, Bigstick, IT-NCSM)

Coupled cluster results with SRG evolved 3NF inputs

Apply these 3NFs to reactions (NCSM+RGM)

Explore various ideas about the choice of Gs