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Ab Initio Description of Open-Shell Nuclei: Merging In-Medium SRG and No-Core Shell Model E. Gebrerufael 1 K. Vobig 1 H. Hergert 2 R. Roth 1 1 Institut für Kernphysik, TU Darmstadt 2 NSCL/FRIB Laboratory and Department of Physics & Astronomy, MSU Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 1 12 C

Ab Initio Description of Open-Shell Nuclei: Merging In ...crunch.ikp.physik.tu-darmstadt.de/tnp/pres/2016_msu_gebrerufael.pdf · Ab Initio Description of Open-Shell Nuclei: Merging

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Page 1: Ab Initio Description of Open-Shell Nuclei: Merging In ...crunch.ikp.physik.tu-darmstadt.de/tnp/pres/2016_msu_gebrerufael.pdf · Ab Initio Description of Open-Shell Nuclei: Merging

Ab Initio Description of Open-Shell Nuclei: Merging In-Medium SRG and No-Core Shell Model

E. Gebrerufael1 K. Vobig1 H. Hergert2 R. Roth1

1 Institut für Kernphysik, TU Darmstadt 2 NSCL/FRIB Laboratory and Department of Physics & Astronomy, MSU

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 1

12C

Page 2: Ab Initio Description of Open-Shell Nuclei: Merging In ...crunch.ikp.physik.tu-darmstadt.de/tnp/pres/2016_msu_gebrerufael.pdf · Ab Initio Description of Open-Shell Nuclei: Merging

Motivation Why should we merge IM-SRG and NCSM?

NCSM

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 2

- limited to light nuclei

- factorial growth of model space

- computationally demanding

- difficult to obtain model-space

convergence

Page 3: Ab Initio Description of Open-Shell Nuclei: Merging In ...crunch.ikp.physik.tu-darmstadt.de/tnp/pres/2016_msu_gebrerufael.pdf · Ab Initio Description of Open-Shell Nuclei: Merging

Motivation Why should we merge IM-SRG and NCSM?

+ easy access to heavy nuclei

+ soft computational scaling with A

+ computationally very efficient

+ decoupling in A-body space

IM- NCSM

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 2

- limited to light nuclei

- factorial growth of model space

- computationally demanding

- difficult to obtain model-space

convergence

SRG

Page 4: Ab Initio Description of Open-Shell Nuclei: Merging In ...crunch.ikp.physik.tu-darmstadt.de/tnp/pres/2016_msu_gebrerufael.pdf · Ab Initio Description of Open-Shell Nuclei: Merging

Motivation Why should we merge IM-SRG and NCSM?

+ easy access to heavy nuclei

+ soft computational scaling with A

+ computationally very efficient

+ decoupling in A-body space

IM- NCSM

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 2

- limited to light nuclei

- factorial growth of model space

- computationally demanding

- difficult to obtain model-space

convergence

SRG

- not exact method

- only for ground state

- spectroscopy not straight forward

- currently limited to even nuclei

Page 5: Ab Initio Description of Open-Shell Nuclei: Merging In ...crunch.ikp.physik.tu-darmstadt.de/tnp/pres/2016_msu_gebrerufael.pdf · Ab Initio Description of Open-Shell Nuclei: Merging

Motivation Why should we merge IM-SRG and NCSM?

+ easy access to heavy nuclei

+ soft computational scaling with A

+ computationally very efficient

+ decoupling in A-body space

IM- NCSM

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 2

- limited to light nuclei

- factorial growth of model space

- computationally demanding

- difficult to obtain model-space

convergence

SRG

- not exact method

- only for ground state

- spectroscopy not straight forward

- currently limited to even nuclei

+ exact method

+ easy access to excited states

+ spectroscopy for free

+ no limitation to even nuclei

Page 6: Ab Initio Description of Open-Shell Nuclei: Merging In ...crunch.ikp.physik.tu-darmstadt.de/tnp/pres/2016_msu_gebrerufael.pdf · Ab Initio Description of Open-Shell Nuclei: Merging

Motivation Why should we merge IM-SRG and NCSM?

+ easy access to heavy nuclei

+ soft computational scaling with A

+ computationally very efficient

+ decoupling in A-body space

IM- NCSM

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 2

- limited to light nuclei

- factorial growth of model space

- computationally demanding

- difficult to obtain model-space

convergence

- not exact method

- only for ground state

- spectroscopy not straight forward

- currently limited to even nuclei

+ exact method

+ easy access to excited states

+ spectroscopy for free

+ no limitation to even nuclei

Page 7: Ab Initio Description of Open-Shell Nuclei: Merging In ...crunch.ikp.physik.tu-darmstadt.de/tnp/pres/2016_msu_gebrerufael.pdf · Ab Initio Description of Open-Shell Nuclei: Merging

Overview

No-Core Shell Model (NCSM)

In-Medium Similarity Renormalization Group (IM-SRG)

Novel Approach: IM-NCSM

Results

o Evolution of Ground-State Energy

o Evolution of Excitation Energies

o Spectra

Summary and Outlook

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 3

Page 8: Ab Initio Description of Open-Shell Nuclei: Merging In ...crunch.ikp.physik.tu-darmstadt.de/tnp/pres/2016_msu_gebrerufael.pdf · Ab Initio Description of Open-Shell Nuclei: Merging

No-Core Shell Model Basics

construct matrix representation of Hamiltonian using basis of HO/HF Slater determinants truncated w.r.t. excitation quanta Nmax

solve large-scale eigenvalue problem for a few smallest eigenvalues

… is one of the most powerful exact ab initio methods

for the p- and lower sd-shell

Barrett, Vary, Navratil, ...

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 4

Page 9: Ab Initio Description of Open-Shell Nuclei: Merging In ...crunch.ikp.physik.tu-darmstadt.de/tnp/pres/2016_msu_gebrerufael.pdf · Ab Initio Description of Open-Shell Nuclei: Merging

No-Core Shell Model Basics

construct matrix representation of Hamiltonian using basis of HO/HF Slater determinants truncated w.r.t. excitation quanta Nmax

solve large-scale eigenvalue problem for a few smallest eigenvalues

range of applicability limited by factorial growth of basis with Nmax & A

adaptive importance-truncation extends the range of NCSM by

reducing the model space to physically relevant states

… is one of the most powerful exact ab initio methods

for the p- and lower sd-shell

Barrett, Vary, Navratil, ...

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 4

Page 10: Ab Initio Description of Open-Shell Nuclei: Merging In ...crunch.ikp.physik.tu-darmstadt.de/tnp/pres/2016_msu_gebrerufael.pdf · Ab Initio Description of Open-Shell Nuclei: Merging

In-Medium Similarity Renormalization Group Basics

flow equation for Hamiltonian:

… uses flow equation for normal-ordered Hamiltonian to decouple

the reference state from its excitations

Tsukiyama, Bogner, Schwenk, Hergert,..

Eskendr Gebrerufael - TU Darmstadt - March 2016 5

Page 11: Ab Initio Description of Open-Shell Nuclei: Merging In ...crunch.ikp.physik.tu-darmstadt.de/tnp/pres/2016_msu_gebrerufael.pdf · Ab Initio Description of Open-Shell Nuclei: Merging

In-Medium Similarity Renormalization Group Basics

flow equation for Hamiltonian:

… uses flow equation for normal-ordered Hamiltonian to decouple

the reference state from its excitations

Tsukiyama, Bogner, Schwenk, Hergert,..

flow parameter

Eskendr Gebrerufael - TU Darmstadt - March 2016 5

generator designed to decouple the reference state

Page 12: Ab Initio Description of Open-Shell Nuclei: Merging In ...crunch.ikp.physik.tu-darmstadt.de/tnp/pres/2016_msu_gebrerufael.pdf · Ab Initio Description of Open-Shell Nuclei: Merging

In-Medium Similarity Renormalization Group Basics

flow equation for Hamiltonian:

… uses flow equation for normal-ordered Hamiltonian to decouple

the reference state from its excitations

H in multi-reference normal-ordered form w.r.t. [Kutzelnigg,Mukherjee]

Tsukiyama, Bogner, Schwenk, Hergert,..

flow parameter

Eskendr Gebrerufael - TU Darmstadt - March 2016 5

generator designed to decouple the reference state

Page 13: Ab Initio Description of Open-Shell Nuclei: Merging In ...crunch.ikp.physik.tu-darmstadt.de/tnp/pres/2016_msu_gebrerufael.pdf · Ab Initio Description of Open-Shell Nuclei: Merging

In-Medium Similarity Renormalization Group Basics

flow equation for Hamiltonian:

… uses flow equation for normal-ordered Hamiltonian to decouple

the reference state from its excitations

H in multi-reference normal-ordered form w.r.t. [Kutzelnigg,Mukherjee]

Tsukiyama, Bogner, Schwenk, Hergert,..

flow parameter

Eskendr Gebrerufael - TU Darmstadt - March 2016 5

generator designed to decouple the reference state

Page 14: Ab Initio Description of Open-Shell Nuclei: Merging In ...crunch.ikp.physik.tu-darmstadt.de/tnp/pres/2016_msu_gebrerufael.pdf · Ab Initio Description of Open-Shell Nuclei: Merging

In-Medium Similarity Renormalization Group Basics

flow equation for Hamiltonian:

… uses flow equation for normal-ordered Hamiltonian to decouple

the reference state from its excitations

H in multi-reference normal-ordered form w.r.t. [Kutzelnigg,Mukherjee]

Tsukiyama, Bogner, Schwenk, Hergert,..

flow parameter

Eskendr Gebrerufael - TU Darmstadt - March 2016 5

generator designed to decouple the reference state

Page 15: Ab Initio Description of Open-Shell Nuclei: Merging In ...crunch.ikp.physik.tu-darmstadt.de/tnp/pres/2016_msu_gebrerufael.pdf · Ab Initio Description of Open-Shell Nuclei: Merging

In-Medium Similarity Renormalization Group Basics

flow equation for Hamiltonian:

… uses flow equation for normal-ordered Hamiltonian to decouple

the reference state from its excitations

H in multi-reference normal-ordered form w.r.t. [Kutzelnigg,Mukherjee]

Tsukiyama, Bogner, Schwenk, Hergert,..

flow parameter

Eskendr Gebrerufael - TU Darmstadt - March 2016 5

generator designed to decouple the reference state

Page 16: Ab Initio Description of Open-Shell Nuclei: Merging In ...crunch.ikp.physik.tu-darmstadt.de/tnp/pres/2016_msu_gebrerufael.pdf · Ab Initio Description of Open-Shell Nuclei: Merging

Novel Approach: IM-NCSM How should we merge…

NCSM define

reference state

IM-SRG evolve

operators

NCSM extract

observables

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 6

Page 17: Ab Initio Description of Open-Shell Nuclei: Merging In ...crunch.ikp.physik.tu-darmstadt.de/tnp/pres/2016_msu_gebrerufael.pdf · Ab Initio Description of Open-Shell Nuclei: Merging

diagonalize Hamiltonian in small model space

ground state defines reference state

Novel Approach: IM-NCSM How should we merge…

NCSM define

reference state

IM-SRG evolve

operators

NCSM extract

observables

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 6

Page 18: Ab Initio Description of Open-Shell Nuclei: Merging In ...crunch.ikp.physik.tu-darmstadt.de/tnp/pres/2016_msu_gebrerufael.pdf · Ab Initio Description of Open-Shell Nuclei: Merging

diagonalize Hamiltonian in small model space

ground state defines reference state

Novel Approach: IM-NCSM How should we merge…

evolve Hamiltonian and other operators

pre-diagonalization in A-body space

NCSM define

reference state

IM-SRG evolve

operators

NCSM extract

observables

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 6

Page 19: Ab Initio Description of Open-Shell Nuclei: Merging In ...crunch.ikp.physik.tu-darmstadt.de/tnp/pres/2016_msu_gebrerufael.pdf · Ab Initio Description of Open-Shell Nuclei: Merging

diagonalize Hamiltonian in small model space

ground state defines reference state

Novel Approach: IM-NCSM How should we merge…

evolve Hamiltonian and other operators

pre-diagonalization in A-body space

NCSM define

reference state

IM-SRG evolve

operators

NCSM extract

observables

diagonalize IM-SRG evolved Hamiltonian

obtain eigenstates and extract observables

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 6

Page 20: Ab Initio Description of Open-Shell Nuclei: Merging In ...crunch.ikp.physik.tu-darmstadt.de/tnp/pres/2016_msu_gebrerufael.pdf · Ab Initio Description of Open-Shell Nuclei: Merging

Nmax=0 Slater determinants

Novel Approach: IM-NCSM Hamiltonian Matrix in A-Body Basis: 12C

Slater determinants

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 7

Nmax=2 Nmax=4

Nm

ax=4

N

max

=2

Nm

ax=0

Page 21: Ab Initio Description of Open-Shell Nuclei: Merging In ...crunch.ikp.physik.tu-darmstadt.de/tnp/pres/2016_msu_gebrerufael.pdf · Ab Initio Description of Open-Shell Nuclei: Merging

Novel Approach: IM-NCSM Hamiltonian Matrix in A-Body Basis: 12C

Nmax=0 eigenstates Slater determinants

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 7

Nmax=2 Nmax=4

Nm

ax=4

N

max

=2

Nm

ax=0

Page 22: Ab Initio Description of Open-Shell Nuclei: Merging In ...crunch.ikp.physik.tu-darmstadt.de/tnp/pres/2016_msu_gebrerufael.pdf · Ab Initio Description of Open-Shell Nuclei: Merging

Novel Approach: IM-NCSM Hamiltonian Matrix in A-Body Basis: 12C

Nmax=0 eigenstates Slater determinants

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 7

Nmax=2 Nmax=4

Nm

ax=4

N

max

=2

Nm

ax=0

Page 23: Ab Initio Description of Open-Shell Nuclei: Merging In ...crunch.ikp.physik.tu-darmstadt.de/tnp/pres/2016_msu_gebrerufael.pdf · Ab Initio Description of Open-Shell Nuclei: Merging

Novel Approach: IM-NCSM Hamiltonian Matrix in A-Body Basis: 12C

Nmax=0 eigenstates Slater determinants

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 7

Nmax=2 Nmax=4

Nm

ax=4

N

max

=2

Nm

ax=0

Page 24: Ab Initio Description of Open-Shell Nuclei: Merging In ...crunch.ikp.physik.tu-darmstadt.de/tnp/pres/2016_msu_gebrerufael.pdf · Ab Initio Description of Open-Shell Nuclei: Merging

Novel Approach: IM-NCSM Hamiltonian Matrix in A-Body Basis: 12C

Nmax=0 eigenstates Slater determinants

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 7

Nmax=2 Nmax=4

Nm

ax=4

N

max

=2

Nm

ax=0

Page 25: Ab Initio Description of Open-Shell Nuclei: Merging In ...crunch.ikp.physik.tu-darmstadt.de/tnp/pres/2016_msu_gebrerufael.pdf · Ab Initio Description of Open-Shell Nuclei: Merging

Novel Approach: IM-NCSM Hamiltonian Matrix in A-Body Basis: 12C

Nmax=0 eigenstates Slater determinants

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 7

Nmax=2 Nmax=4

Nm

ax=4

N

max

=2

Nm

ax=0

Page 26: Ab Initio Description of Open-Shell Nuclei: Merging In ...crunch.ikp.physik.tu-darmstadt.de/tnp/pres/2016_msu_gebrerufael.pdf · Ab Initio Description of Open-Shell Nuclei: Merging

Novel Approach: IM-NCSM Hamiltonian Matrix in A-Body Basis: 12C

Nmax=0 eigenstates Slater determinants

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 7

Nmax=2 Nmax=4

Nm

ax=4

N

max

=2

Nm

ax=0

Page 27: Ab Initio Description of Open-Shell Nuclei: Merging In ...crunch.ikp.physik.tu-darmstadt.de/tnp/pres/2016_msu_gebrerufael.pdf · Ab Initio Description of Open-Shell Nuclei: Merging

Novel Approach: IM-NCSM Hamiltonian Matrix in A-Body Basis: 12C

Nmax=0 eigenstates Slater determinants

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 7

Nmax=2 Nmax=4

Nm

ax=4

N

max

=2

Nm

ax=0

Page 28: Ab Initio Description of Open-Shell Nuclei: Merging In ...crunch.ikp.physik.tu-darmstadt.de/tnp/pres/2016_msu_gebrerufael.pdf · Ab Initio Description of Open-Shell Nuclei: Merging

Novel Approach: IM-NCSM Hamiltonian Matrix in A-Body Basis: 12C

Nmax=0 eigenstates Slater determinants

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 7

Nmax=2 Nmax=4

Nm

ax=4

N

max

=2

Nm

ax=0

Page 29: Ab Initio Description of Open-Shell Nuclei: Merging In ...crunch.ikp.physik.tu-darmstadt.de/tnp/pres/2016_msu_gebrerufael.pdf · Ab Initio Description of Open-Shell Nuclei: Merging

Novel Approach: IM-NCSM Hamiltonian Matrix in A-Body Basis: 12C

Nmax=0 eigenstates Slater determinants

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 7

Nmax=2 Nmax=4

Nm

ax=4

N

max

=2

Nm

ax=0

Page 30: Ab Initio Description of Open-Shell Nuclei: Merging In ...crunch.ikp.physik.tu-darmstadt.de/tnp/pres/2016_msu_gebrerufael.pdf · Ab Initio Description of Open-Shell Nuclei: Merging

Novel Approach: IM-NCSM Hamiltonian Matrix in A-Body Basis: 12C

Nmax=0 eigenstates Slater determinants

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 7

Nmax=2 Nmax=4

Nm

ax=4

N

max

=2

Nm

ax=0

Page 31: Ab Initio Description of Open-Shell Nuclei: Merging In ...crunch.ikp.physik.tu-darmstadt.de/tnp/pres/2016_msu_gebrerufael.pdf · Ab Initio Description of Open-Shell Nuclei: Merging

Novel Approach: IM-NCSM Hamiltonian Matrix in A-Body Basis: 12C

Nmax=0 eigenstates Slater determinants

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 7

Nmax=2 Nmax=4

Nm

ax=4

N

max

=2

Nm

ax=0

Page 32: Ab Initio Description of Open-Shell Nuclei: Merging In ...crunch.ikp.physik.tu-darmstadt.de/tnp/pres/2016_msu_gebrerufael.pdf · Ab Initio Description of Open-Shell Nuclei: Merging

Novel Approach: IM-NCSM Hamiltonian Matrix in A-Body Basis: 12C

Nmax=0 eigenstates Slater determinants

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 7

Nmax=2 Nmax=4

Nm

ax=4

N

max

=2

Nm

ax=0

Page 33: Ab Initio Description of Open-Shell Nuclei: Merging In ...crunch.ikp.physik.tu-darmstadt.de/tnp/pres/2016_msu_gebrerufael.pdf · Ab Initio Description of Open-Shell Nuclei: Merging

Novel Approach: IM-NCSM Hamiltonian Matrix in A-Body Basis: 12C

Nmax=0 eigenstates Slater determinants

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 7

Nmax=2 Nmax=4

Nm

ax=4

N

max

=2

Nm

ax=0

Page 34: Ab Initio Description of Open-Shell Nuclei: Merging In ...crunch.ikp.physik.tu-darmstadt.de/tnp/pres/2016_msu_gebrerufael.pdf · Ab Initio Description of Open-Shell Nuclei: Merging

Novel Approach: IM-NCSM Hamiltonian Matrix in A-Body Basis: 12C

for sufficiently large flow parameter eigenvalues in Nmax=0, 2 and 4 equal

Nmax=0 eigenstates Slater determinants

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 7

Nmax=2 Nmax=4

Nm

ax=4

N

max

=2

Nm

ax=0

Page 35: Ab Initio Description of Open-Shell Nuclei: Merging In ...crunch.ikp.physik.tu-darmstadt.de/tnp/pres/2016_msu_gebrerufael.pdf · Ab Initio Description of Open-Shell Nuclei: Merging

Novel Approach: IM-NCSM Hamiltonian Matrix in A-Body Basis: 12C

for sufficiently large flow parameter eigenvalues in Nmax=0, 2 and 4 equal

Nmax=0 eigenstates Slater determinants

IM-SRG decouples reference state from Nmax =2 and 4 spaces

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 7

Nmax=2 Nmax=4

Nm

ax=4

N

max

=2

Nm

ax=0

Page 36: Ab Initio Description of Open-Shell Nuclei: Merging In ...crunch.ikp.physik.tu-darmstadt.de/tnp/pres/2016_msu_gebrerufael.pdf · Ab Initio Description of Open-Shell Nuclei: Merging

Novel Approach: IM-NCSM Hamiltonian Matrix in A-Body Basis: 12C

for sufficiently large flow parameter eigenvalues in Nmax=0, 2 and 4 equal

Nmax=0 eigenstates Slater determinants

IM-SRG decouples reference state from Nmax =2 and 4 spaces

Why do E(s) and Nmax=0 eigenvalue differ?

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 7

Nmax=2 Nmax=4

Nm

ax=4

N

max

=2

Nm

ax=0

Page 37: Ab Initio Description of Open-Shell Nuclei: Merging In ...crunch.ikp.physik.tu-darmstadt.de/tnp/pres/2016_msu_gebrerufael.pdf · Ab Initio Description of Open-Shell Nuclei: Merging

Novel Approach: IM-NCSM Hamilton Matrix in A-Body Basis: 12C

Nmax=0 states couple to

reference state

first basis state = reference state

Nmax=0 eigenstates

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 8

Page 38: Ab Initio Description of Open-Shell Nuclei: Merging In ...crunch.ikp.physik.tu-darmstadt.de/tnp/pres/2016_msu_gebrerufael.pdf · Ab Initio Description of Open-Shell Nuclei: Merging

Novel Approach: IM-NCSM Hamilton Matrix in A-Body Basis: 12C

Nmax=0 states couple to

reference state

first basis state = reference state

Nmax=0 eigenstates

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 8

Page 39: Ab Initio Description of Open-Shell Nuclei: Merging In ...crunch.ikp.physik.tu-darmstadt.de/tnp/pres/2016_msu_gebrerufael.pdf · Ab Initio Description of Open-Shell Nuclei: Merging

Novel Approach: IM-NCSM Hamilton Matrix in A-Body Basis: 12C

Nmax=0 states couple to

reference state

E(s) and Nmax=0 eigenvalue

cannot be identical

first basis state = reference state

Nmax=0 eigenstates

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 8

Page 40: Ab Initio Description of Open-Shell Nuclei: Merging In ...crunch.ikp.physik.tu-darmstadt.de/tnp/pres/2016_msu_gebrerufael.pdf · Ab Initio Description of Open-Shell Nuclei: Merging

Novel Approach: IM-NCSM Hamilton Matrix in A-Body Basis: 12C

Nmax=0 states couple to

reference state

E(s) and Nmax=0 eigenvalue

cannot be identical

diagonalization of evolved Hamiltonian

necessary

first basis state = reference state

Nmax=0 eigenstates

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 8

Page 41: Ab Initio Description of Open-Shell Nuclei: Merging In ...crunch.ikp.physik.tu-darmstadt.de/tnp/pres/2016_msu_gebrerufael.pdf · Ab Initio Description of Open-Shell Nuclei: Merging

Overview

No-Core Shell Model (NCSM)

In-Medium Similarity Renormalization Group (IM-SRG)

Novel Approach: IM-NCSM

Results

o Evolution of Ground-State Energy

o Evolution of Excitation Energies

o Spectra

Summary and Outlook

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 9

Page 42: Ab Initio Description of Open-Shell Nuclei: Merging In ...crunch.ikp.physik.tu-darmstadt.de/tnp/pres/2016_msu_gebrerufael.pdf · Ab Initio Description of Open-Shell Nuclei: Merging

Results Evolution of Ground-State Energy

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 10

Page 43: Ab Initio Description of Open-Shell Nuclei: Merging In ...crunch.ikp.physik.tu-darmstadt.de/tnp/pres/2016_msu_gebrerufael.pdf · Ab Initio Description of Open-Shell Nuclei: Merging

Results Evolution of Ground-State Energy

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 10

Page 44: Ab Initio Description of Open-Shell Nuclei: Merging In ...crunch.ikp.physik.tu-darmstadt.de/tnp/pres/2016_msu_gebrerufael.pdf · Ab Initio Description of Open-Shell Nuclei: Merging

Results Evolution of Ground-State Energy

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 10

drastically enhanced model-space convergence for IM-NCSM

Page 45: Ab Initio Description of Open-Shell Nuclei: Merging In ...crunch.ikp.physik.tu-darmstadt.de/tnp/pres/2016_msu_gebrerufael.pdf · Ab Initio Description of Open-Shell Nuclei: Merging

Results Evolution of Ground-State Energy

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 10

drastically enhanced model-space convergence for IM-NCSM

Page 46: Ab Initio Description of Open-Shell Nuclei: Merging In ...crunch.ikp.physik.tu-darmstadt.de/tnp/pres/2016_msu_gebrerufael.pdf · Ab Initio Description of Open-Shell Nuclei: Merging

Results Evolution of Ground-State Energy

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 10

drastically enhanced model-space convergence for IM-NCSM

NCSM with explicit 3N

Page 47: Ab Initio Description of Open-Shell Nuclei: Merging In ...crunch.ikp.physik.tu-darmstadt.de/tnp/pres/2016_msu_gebrerufael.pdf · Ab Initio Description of Open-Shell Nuclei: Merging

Results Evolution of Ground-State Energy

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 10

drastically enhanced model-space convergence for IM-NCSM

NO2B approximation + induced many-body contribution = 4.0 MeV (≈ 5 %)

NCSM with explicit 3N

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Results Evolution of Ground-State Energy

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 10

drastically enhanced model-space convergence for IM-NCSM

NO2B approximation + induced many-body contribution = 4.0 MeV (≈ 5 %)

for s > 0.3 MeV-1 induced many-body contribution becomes significant

NCSM with explicit 3N

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Results Evolution of Ground-State Energy

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 10

drastically enhanced model-space convergence for IM-NCSM

NO2B approximation + induced many-body contribution = 4.0 MeV (≈ 5 %)

for s > 0.3 MeV-1 induced many-body contribution becomes significant

NCSM with explicit 3N

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Results Evolution of Ground-State Energy

E(s) more robust than in 12C case

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 11

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Results Evolution of Ground-State Energy

E(s) more robust than in 12C case

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 11

NCSM with explicit 3N

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Results Evolution of Ground-State Energy

E(s) more robust than in 12C case

NO2B approximation + induced many-body contribution = 2.3 MeV (< 2 %)

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 11

NCSM with explicit 3N

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Results Evolution of Ground-State Energy

E(s) more robust than in 12C case

NO2B approximation + induced many-body contribution = 2.3 MeV (< 2 %)

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 11

NCSM with explicit 3N

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Results Evolution of Excitation Energies

E* of 2+ increases abruptly at the end due to kink in ground-state energy

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 12

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Results Evolution of Excitation Energies

E* of 2+ increases abruptly at the end due to kink in ground-state energy

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 12

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Results Evolution of Excitation Energies

E* of 2+ increases abruptly at the end due to kink in ground-state energy

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 12

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Results Evolution of Excitation Energies

E* of 2+ increases abruptly at the end due to kink in ground-state energy

E* converges monotonically from above w.r.t. Nmax for evolved Hamiltonian

variational principle valid for E* since ground-state energy converged

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 12

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Results Evolution of Excitation Energies

E* of 2+ increases abruptly at the end due to kink in ground-state energy

E* converges monotonically from above w.r.t. Nmax for evolved Hamiltonian

variational principle valid for E* since ground-state energy converged

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 12

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Results Evolution of Excitation Energies

E* of 2+ increases abruptly at the end due to kink in ground-state energy

E* converges monotonically from above w.r.t. Nmax for evolved Hamiltonian

variational principle valid for E* since ground-state energy converged

first excited 0 + very sensitive to flow parameter Hoyle state? Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 12

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Results Evolution of Excitation Energies

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 13

large dependence on s in Nmax=0

dependence on s reduces with increasing Nmax

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Results Evolution of Excitation Energies

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 13

large dependence on s in Nmax=0

dependence on s reduces with increasing Nmax

E* converges monotonically from above for evolved Hamiltonian

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Results Evolution of Excitation Energies

analyze E* as function of Nmax

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 13

large dependence on s in Nmax=0

dependence on s reduces with increasing Nmax

E* converges monotonically from above for evolved Hamiltonian

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Results Spectra

IM-NCSM

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 14

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Results Spectra

IM-NCSM

uncertainty band due to flow-parameter variation between smax/2 and smax

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 14

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Results Spectra

NCSM IM-NCSM

uncertainty band due to flow-parameter variation between smax/2 and smax

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 14

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Results Spectra

NCSM IM-NCSM

uncertainty band due to flow-parameter variation between smax/2 and smax

2+ and 1+ in IM-NCSM and NCSM in good agreement

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 14

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Results Spectra

NCSM IM-NCSM

uncertainty band due to flow-parameter variation between smax/2 and smax

2+ and 1+ in IM-NCSM and NCSM in good agreement

second 0+ in IM-NCSM closer to experiment (Hoyle?)

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 14

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Results Spectra

NCSM IM-NCSM

uncertainty band due to flow-parameter variation between smax/2 and smax

2+ and 1+ in IM-NCSM and NCSM in good agreement

second 0+ in IM-NCSM closer to experiment (Hoyle?)

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 14

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Results Spectra

first 2+ and 4+ robust and well converged in IM-NCSM

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 15

NCSM IM-NCSM

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Results Spectra

first 2+ and 4+ robust and well converged in IM-NCSM

higher-lying states show small flow-parameter dependence

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 15

NCSM IM-NCSM

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Results Spectra

first 2+ and 4+ robust and well converged in IM-NCSM

higher-lying states show small flow-parameter dependence

1+ not yet observed experimentally theoretical prediction

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 15

NCSM IM-NCSM

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Results Spectra

first 2+ and 4+ robust and well converged in IM-NCSM

higher-lying states show small flow-parameter dependence

1+ not yet observed experimentally theoretical prediction

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 15

NCSM IM-NCSM

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Summary

introduced new many-body technique IM-NCSM = IM-SRG + NCSM

exploits the advantages of both approaches

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 16

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Summary

introduced new many-body technique IM-NCSM = IM-SRG + NCSM

exploits the advantages of both approaches

IM-SRG decouples reference state from higher Nmax

extremely enhanced Nmax convergence for subsequent NCSM

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 16

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Summary

introduced new many-body technique IM-NCSM = IM-SRG + NCSM

exploits the advantages of both approaches

IM-SRG decouples reference state from higher Nmax

extremely enhanced Nmax convergence for subsequent NCSM

Nmax≤4 sufficient to extract converged ground-state energies

variational principle becomes valid for excitation energies

since ground-state energy converged

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 16

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Outlook

o variation of several parameters: generator,

o consistent evolution radius, electromagnetic, … operators

o detailed analysis of the Hoyle state in 12C

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 17

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Outlook

o variation of several parameters: generator,

o consistent evolution radius, electromagnetic, … operators

o detailed analysis of the Hoyle state in 12C

o extend applicability of IM-NCSM to odd nuclei

using particle-attached particle-removed formalism

o include three-body operators in IM-SRG

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 17

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Thanks to my group & collaborator • S. Alexa, S. Dentinger, T. Hüther, L. Kreher,

L. Mertes, S. Ruppert, R. Roth, S. Schulz,

H. Spiess, H. Spielvogel, C. Stumpf, A. Tichai,

R. Trippel, K. Vobig, R. Wirth

Institut für Kernphysik, TU Darmstadt

• H. Hergert

NSCL/FRIB, Michigan State University

Thank You For Your Attention

JURECA LOEWE-CSC LICHTENBERG

COMPUTING TIME

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 18

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Appendix

Appendix

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 19

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Results NCSM vs. IM-NCSM vs. MR-IM-SRG

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 20

NCSM @ Nmax extrap. IM-NCSM @ Nmax=4 MR-IM-SRG (HFB, White) Experiment

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Results Dependence on Single-Particle Basis

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 21

For small flow parameter Nmax convergence slow in HF basis

induced many-body in HF 4 MeV and in HO < 1 MeV

NCSM with 3N

HF

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Results Dependence on Single-Particle Basis

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 21

For small flow parameter Nmax convergence slow in HF basis

induced many-body in HF 4 MeV and in HO < 1 MeV

NCSM with 3N

Nmax-Extrapolation at s=0

HO

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Results Dependence on

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 22

quite insensitive on

E(s) equal to eigenvalue obtained in for small flow parameter s

since the reference state is an eigenstate obtained in model space

HF

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Results Dependence on

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 22

quite insensitive on

E(s) equal to eigenvalue obtained in for small flow parameter s

since the reference state is an eigenstate obtained in model space

HF

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Results Dependence on

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 23

quite insensitive on

E(s) equal to eigenvalue obtained in for small flow parameter s

since the reference state is an eigenstate obtained in model space

HO

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Results Dependence on

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 23

quite insensitive on

E(s) equal to eigenvalue obtained in for small flow parameter s

since the reference state is an eigenstate obtained in model space

HO

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Results Dependence on

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 23

quite insensitive on

E(s) equal to eigenvalue obtained in for small flow parameter s

since the reference state is an eigenstate obtained in model space

HO

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Results Spectra

excellent agreement between IM-NCSM and NCSM

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 24

NCSM IM-NCSM

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Results Spectra

4+ simply not calculated in NCSM

first excited 0+ shows same behaviour as in 12C

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 25

NCSM IM-NCSM

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Results IM-NCSM: Particle-Attached Particle-Removed Form.

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 26

7 8

6

parent

eigenvalues for small flow parameter independent on parent nucleus

eigenvalues for large flow paremter show dependence on parent nucleus

deviation at the level of 4 MeV (< 4%)

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Results IM-NCSM: Particle-Attached Particle-Removed Form.

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 27

parent

7 8

6

deviation at the level of 5 MeV (< 5%)

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Results IM-NCSM: Particle-Attached Particle-Removed Form.

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 28

7 8

6

parent

deviation at the level of 5 MeV (< 5%)

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Results Evolution of Excitation Energies – On Absolute Scale

2+ perfectly converged on absolute scale

induced many-body contribution different for each state

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 29

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Slater det.

Novel Approach: IM-NCSM Hamilton Matrix in A-Body Basis: 16O

E(s) converges monotonically against Nmax=2 eigenvalue

Nmax=2 Slater determinants

IM-SRG decouples reference state

from Nmax =2 space

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 30

Nmax=0

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Slater det.

Novel Approach: IM-NCSM Hamilton Matrix in A-Body Basis: 16O

E(s) converges monotonically against Nmax=2 eigenvalue

Nmax=2 Slater determinants

IM-SRG decouples reference state

from Nmax =2 space

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 30

Nmax=0

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Slater det.

Novel Approach: IM-NCSM Hamilton Matrix in A-Body Basis: 16O

E(s) converges monotonically against Nmax=2 eigenvalue

Nmax=2 Slater determinants

IM-SRG decouples reference state

from Nmax =2 space

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 30

Nmax=0

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Slater det.

Novel Approach: IM-NCSM Hamilton Matrix in A-Body Basis: 16O

E(s) converges monotonically against Nmax=2 eigenvalue

Nmax=2 Slater determinants

IM-SRG decouples reference state

from Nmax =2 space

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 30

Nmax=0

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Nmax=0 Slater determinants

Novel Approach: IM-NCSM Hamilton Matrix in A-Body Basis: 12C

Nmax=2 Slater determinants

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 31

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Novel Approach: IM-NCSM Hamilton Matrix in A-Body Basis: 12C

Nmax=0 eigenstates

Nmax=2 Slater determinants

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 31

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Novel Approach: IM-NCSM Hamilton Matrix in A-Body Basis: 12C

Nmax=0 eigenstates

Nmax=2 Slater determinants

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 31

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Novel Approach: IM-NCSM Hamilton Matrix in A-Body Basis: 12C

Nmax=0 eigenstates

Nmax=2 Slater determinants

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 31

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Novel Approach: IM-NCSM Hamilton Matrix in A-Body Basis: 12C

Nmax=0 eigenstates

Nmax=2 Slater determinants

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 31

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Novel Approach: IM-NCSM Hamilton Matrix in A-Body Basis: 12C

Nmax=0 eigenstates

Nmax=2 Slater determinants

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 31

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Novel Approach: IM-NCSM Hamilton Matrix in A-Body Basis: 12C

Nmax=0 eigenstates

Nmax=2 Slater determinants

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Novel Approach: IM-NCSM Hamilton Matrix in A-Body Basis: 12C

Nmax=0 eigenstates

Nmax=2 Slater determinants

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Novel Approach: IM-NCSM Hamilton Matrix in A-Body Basis: 12C

Nmax=0 eigenstates

Nmax=2 Slater determinants

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Novel Approach: IM-NCSM Hamilton Matrix in A-Body Basis: 12C

Nmax=0 eigenstates

Nmax=2 Slater determinants

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Novel Approach: IM-NCSM Hamilton Matrix in A-Body Basis: 12C

Nmax=0 eigenstates

Nmax=2 Slater determinants

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Novel Approach: IM-NCSM Hamilton Matrix in A-Body Basis: 12C

Nmax=0 eigenstates

Nmax=2 Slater determinants

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Novel Approach: IM-NCSM Hamilton Matrix in A-Body Basis: 12C

Nmax=0 eigenstates

Nmax=2 Slater determinants

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Novel Approach: IM-NCSM Hamilton Matrix in A-Body Basis: 12C

for sufficient large flow parameter eigenvalues in Nmax=0 and Nmax=2 equal

Nmax=0 eigenstates

Nmax=2 Slater determinants

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Novel Approach: IM-NCSM Hamilton Matrix in A-Body Basis: 12C

for sufficient large flow parameter eigenvalues in Nmax=0 and Nmax=2 equal

Nmax=0 eigenstates

Nmax=2 Slater determinants

IM-SRG decouples reference state (not only)

from Nmax =2 space

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Novel Approach: IM-NCSM Hamilton Matrix in A-Body Basis: 12C

for sufficient large flow parameter eigenvalues in Nmax=0 and Nmax=2 equal

Nmax=0 eigenstates

Nmax=2 Slater determinants

IM-SRG decouples reference state (not only)

from Nmax =2 space

-> why do E(s) and Nmax=0 eigenvalue differ?

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free-space SRG

NC

SM

normal ordering

IM-SRG NCSM

IM-NCSM Procedure

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free-space SRG

NC

SM

normal ordering

IM-SRG NCSM

IM-NCSM Procedure

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free-space SRG

NC

SM

normal ordering

IM-SRG NCSM

IM-NCSM Procedure

IM-SRG to get rid of spurious states:

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free-space SRG

NC

SM

normal ordering

IM-SRG

CI

NCSM

IM-NCSM Procedure

IM-SRG to get rid of spurious states:

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IM-NCSM Current Implementation of Imaginary Time

natural orbitals: ni occupation number

… missing terms contain irreducible density matrix

Eskendr Gebrerufael - TU Darmstadt - Oct. 2016 33