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Some Open Problems in Nuclear Some Open Problems in Nuclear Large Amplitude Collective Motion Large Amplitude Collective Motion Aurel Bulgac Aurel Bulgac University of Washington University of Washington Funding: DOE grants No. DE-FG02-97ER41014 (UW Funding: DOE grants No. DE-FG02-97ER41014 (UW NT Group) NT Group) DE-FC02-07ER41457 (SciDAC-UNEDF) DE-FC02-07ER41457 (SciDAC-UNEDF) Sukjin YOON (UW) Sukjin YOON (UW) Kenneth J. ROCHE (PNNL-Seattle) Kenneth J. ROCHE (PNNL-Seattle) Yongle YU (Wuhan Institute of Physics and Mathematics) Yongle YU (Wuhan Institute of Physics and Mathematics) Yuan Lung LUO (UW) Yuan Lung LUO (UW) Piotr MAGIERSKI (Warsaw and UW) Piotr MAGIERSKI (Warsaw and UW) Ionel STETCU (UW) Ionel STETCU (UW)

Some Open Problems in Nuclear Large Amplitude Collective Motion Aurel Bulgac University of Washington Funding: DOE grants No. DE-FG02-97ER41014 (UW NT

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Some Open Problems in Nuclear Some Open Problems in Nuclear Large Amplitude Collective MotionLarge Amplitude Collective Motion

Aurel BulgacAurel BulgacUniversity of WashingtonUniversity of Washington

Funding: DOE grants No. DE-FG02-97ER41014 (UW NT Group)Funding: DOE grants No. DE-FG02-97ER41014 (UW NT Group) DE-FC02-07ER41457 (SciDAC-UNEDF)DE-FC02-07ER41457 (SciDAC-UNEDF)

Sukjin YOON (UW)Sukjin YOON (UW)Kenneth J. ROCHE (PNNL-Seattle)Kenneth J. ROCHE (PNNL-Seattle)

Yongle YU (Wuhan Institute of Physics and Mathematics)Yongle YU (Wuhan Institute of Physics and Mathematics)Yuan Lung LUO (UW)Yuan Lung LUO (UW)Piotr MAGIERSKI (Warsaw and UW) Piotr MAGIERSKI (Warsaw and UW) Ionel STETCU (UW)Ionel STETCU (UW)

Our grand challenge: Our grand challenge:

With new tools we should address qualitatively new questions!With new tools we should address qualitatively new questions!

What core problems can we address of central interest to What core problems can we address of central interest to National Security and (Nuclear) Science as well? National Security and (Nuclear) Science as well?

Can we compute reliably the mass, charge, excitation andCan we compute reliably the mass, charge, excitation andquantum numbers (spins and parities) distributions of quantum numbers (spins and parities) distributions of fragments in induced neutron and gamma induced fission? fragments in induced neutron and gamma induced fission?

These would be of direct interest to Nuclear Forensics.These would be of direct interest to Nuclear Forensics.

There seem to be some light at the end of the tunnel!There seem to be some light at the end of the tunnel!

Outline:Outline:

• Where do we stand right now with the theory? Where do we stand right now with the theory?

o Open problems in LACM. Open problems in LACM. o Current approaches and their limitations. Current approaches and their limitations. o The computational tools we have developed so far for today’s leadership class The computational tools we have developed so far for today’s leadership class computers and beyond.computers and beyond.

• Our long-range vision for the study of: Our long-range vision for the study of:

o Nuclear dynamics - large and small amplitude collective motion (LACM), reactions Nuclear dynamics - large and small amplitude collective motion (LACM), reactions and fission and fission o Vortex creation and dynamics in neutron stars (pinning and de-pinning mechanism)Vortex creation and dynamics in neutron stars (pinning and de-pinning mechanism)o Cold atoms in static and dynamic traps and optical lattices and other condensed Cold atoms in static and dynamic traps and optical lattices and other condensed matter systems. matter systems.

Coulomb excitation of Coulomb excitation of 4848Cr by an ultra-relativistic heavy ionCr by an ultra-relativistic heavy ion

XX

YY

ZZ

A few details of the calculation:A few details of the calculation:

• We solved the time-dependent 3D SLDA (HFB) equations for We solved the time-dependent 3D SLDA (HFB) equations for 4848CrCr• Only Coulomb interaction between the projectile and target Only Coulomb interaction between the projectile and target (10 fm impact parameter)(10 fm impact parameter)• We described We described 4848Cr with approximately 3,600 quasiparticle wave functionsCr with approximately 3,600 quasiparticle wave functions(this is already about an order of magnitude above all current TDHF (this is already about an order of magnitude above all current TDHF calculations, and we still have about two or more orders of magnitude in storecalculations, and we still have about two or more orders of magnitude in storeto expand easily)to expand easily)• We used 3,600 processors on Franklin at NERSC for about 10 hoursWe used 3,600 processors on Franklin at NERSC for about 10 hours(both weak and strong scaling properties of the code are essentially perfect(both weak and strong scaling properties of the code are essentially perfectup to about 50,000 processors so far)up to about 50,000 processors so far)

Present theoretical approaches and phenomenology for Present theoretical approaches and phenomenology for LACM and fission studies:LACM and fission studies:

o Pure phenomenogical stochastic dynamics :Pure phenomenogical stochastic dynamics : Langevin/Kramers equationsLangevin/Kramers equations Stochastic/Langevin TDHF Stochastic/Langevin TDHF

o Adiabatic Time-Dependent Hartree-Fock-Bogoliubov (ATDHFB) theoryAdiabatic Time-Dependent Hartree-Fock-Bogoliubov (ATDHFB) theory The basic assumption is that LACM/nuclear fission can be described with a The basic assumption is that LACM/nuclear fission can be described with a many-body wave function with the GCM- structure:many-body wave function with the GCM- structure:

Coll. 1 Slater det. 1 11

,..., ,..., , ,...,n

i n A ni

dq q q x x q q

o Microscopic-macroscopic Microscopic-macroscopic modelmodel not based on not based on ab intio ab intio inputinput no self-consistencyno self-consistency physical intuition drives the definition of relevant degrees of freedomphysical intuition drives the definition of relevant degrees of freedom

Extended, … Stochastic TDHF approaches Extended, … Stochastic TDHF approaches

Wong and Tang, Phys. Rev. Lett. 40, 1070 (1978)Wong and Tang, Phys. Rev. Lett. 40, 1070 (1978)Ayik, Z. Phys. A 298, 83 (1980)Ayik, Z. Phys. A 298, 83 (1980)......Ayik Phys. Lett. B658, 174 (2008)Ayik Phys. Lett. B658, 174 (2008)

*

,( , , ) ,

( , , ) , ( ) ,

( )

1( ) ( ) (1 ) (1 )

2

kk

k kl lkl

kl kl k

kl ij kj li i j j i

x ti h x y t x t

t

x y t x t n t x t

n t n

n t n t n n n n

Gaussian random numbersGaussian random numbersdefined a prescribed temperaturedefined a prescribed temperaturein a Fermi-Dirac distribution in a Fermi-Dirac distribution

Subsequently these equations are Subsequently these equations are projectedprojected on a collective subspace and on a collective subspace and a Langevin equation is introduced for the collective DoF a Langevin equation is introduced for the collective DoF

Talk of E. Vardaci at FISSION 2009Talk of E. Vardaci at FISSION 2009

• Computing the potential energy surface alone for only Computing the potential energy surface alone for only 33 collective degrees of freedom collective degrees of freedom is equivalent to computing the entire nuclearis equivalent to computing the entire nuclear mass table. mass table.

P. Moller and collaborators need more than 5,000,000 shapes in a P. Moller and collaborators need more than 5,000,000 shapes in a fivefive dimensional space. dimensional space.

Is this the right and the entire complete set of collective coordinates?Is this the right and the entire complete set of collective coordinates?

P.Moller P.Moller et al. et al. Phys. Rev. C Phys. Rev. C 7979, 064304 (2009), 064304 (2009)

While ATDHFB approximation has a great number of positive While ATDHFB approximation has a great number of positive aspects, it comes with a long series of great deficiencies:aspects, it comes with a long series of great deficiencies:

• The determination of the number of relevant degrees of freedom is as a rule determined The determination of the number of relevant degrees of freedom is as a rule determined by the practioner using intuition/prejudice or prevailing attitudes. by the practioner using intuition/prejudice or prevailing attitudes.

There are knows methods on how to mechanize this process and eliminate arbitrariness,There are knows methods on how to mechanize this process and eliminate arbitrariness,but they are extremely difficult to implement in practice.but they are extremely difficult to implement in practice.

Hinohara, Nakatsukasa, Matsuo, andHinohara, Nakatsukasa, Matsuo, andMatsuyanagi, Phys. Rev. C  Matsuyanagi, Phys. Rev. C  8080, 014305 (2009), 014305 (2009)

Coll. 1 Slater det. 1 11

,..., ,..., , ,...,n

i n A ni

dq q q x x q q

• In order to determine the collective part of the wave function one needs to solve In order to determine the collective part of the wave function one needs to solve the Hill-Wheeler integral equation in the corresponding the Hill-Wheeler integral equation in the corresponding nn-dimensional space.-dimensional space.

This is routinely (but not always) performed by invoking a further approximation This is routinely (but not always) performed by invoking a further approximation (Gaussian Overlap Approximation) the accuracy of which is difficult to assess and (Gaussian Overlap Approximation) the accuracy of which is difficult to assess and one generates a Schrödinger equation in collective coordinates.one generates a Schrödinger equation in collective coordinates.

• ATDHFB theory is based on the assumption that an expansion in velocities is accurate ATDHFB theory is based on the assumption that an expansion in velocities is accurate up to second order terms. However there are clear examples where this is wrong. up to second order terms. However there are clear examples where this is wrong.

• The inertial tensor is usually hard to evaluate and often approximate methods are The inertial tensor is usually hard to evaluate and often approximate methods are used.used.

•It is obvious that a significantly larger number of degrees of freedom areIt is obvious that a significantly larger number of degrees of freedom arenecessary to describe LACM and fission in particular. necessary to describe LACM and fission in particular.

One would like to have as well: charge asymmetry, shapes of the fragments, One would like to have as well: charge asymmetry, shapes of the fragments, excitation energy of the fragments, …excitation energy of the fragments, …

In this case the ATHFB approach becomes clearly unmanageable, even for In this case the ATHFB approach becomes clearly unmanageable, even for computers envision in the next decade, and the veracity of the approximation computers envision in the next decade, and the veracity of the approximation is questionable is questionable . .

G.F. Bertsch, F. Barranco, and R.A. Broglia, G.F. Bertsch, F. Barranco, and R.A. Broglia, How Nuclei Change ShapeHow Nuclei Change Shapein in Windsurfing the Fermi SeaWindsurfing the Fermi Sea, eds. T.T.S. Kuo and J. Speth, eds. T.T.S. Kuo and J. Speth

•It is not obvious that the Slater determinant wave function should minimize the It is not obvious that the Slater determinant wave function should minimize the energy. Entropy production, level crossings, symmetry breaking.energy. Entropy production, level crossings, symmetry breaking.

Generic adiabatic large amplitude potential energy Generic adiabatic large amplitude potential energy SURFACESSURFACES

• In LACM adiabaticity/isentropic or isothermal behavior is not a guaranteedIn LACM adiabaticity/isentropic or isothermal behavior is not a guaranteed• The most efficient mechanism for transitions at level crossing is due to pairingThe most efficient mechanism for transitions at level crossing is due to pairing• Level crossings are a great source of : entropy production (dissipation), dynamical Level crossings are a great source of : entropy production (dissipation), dynamical symmetry breaking , non-abelian gauge fields (Dirac monopoles reside at level crossings)symmetry breaking , non-abelian gauge fields (Dirac monopoles reside at level crossings)

Evolution operator of an interacting many-body systemEvolution operator of an interacting many-body system(after a Trotter expansion and a Hubbard-Stratonovich transformation)(after a Trotter expansion and a Hubbard-Stratonovich transformation)

exp ( ) ( ) exp ( ) ( )2

exp ( )

f i ab ab abcd cdabcdn ab

ab abcd cd a bab cd

tiH t t d n i n V n

i t T V n

This representation is not unique!This representation is not unique!

The one-body evolution operator is arbitrary!!!The one-body evolution operator is arbitrary!!!

Kerman, Levit, and Troudet, Ann. Phys. Kerman, Levit, and Troudet, Ann. Phys. 148148, 443 (1983), 443 (1983)

What is the What is the bestbest one-body propagator? one-body propagator?

Stationary phase approximation leads to some form of Stationary phase approximation leads to some form of Time-Dependent Meanfield Time-Dependent Meanfield

However, there is a bright spot if one is interested in one-body However, there is a bright spot if one is interested in one-body observables alone observables alone

Time-Dependent Density Functional Theory (TDDFT) asserts Time-Dependent Density Functional Theory (TDDFT) asserts that there exists an that there exists an exactexact description, which formally looks like description, which formally looks like Time-Dependent Selfconsistent Meanfield.Time-Dependent Selfconsistent Meanfield.

A.K. Rajagopal and J. Callaway, Phys. Rev. B A.K. Rajagopal and J. Callaway, Phys. Rev. B 77, 1912 (1973), 1912 (1973)V. Peuckert, J. Phys. C V. Peuckert, J. Phys. C 1111, 4945 (1978) , 4945 (1978) E. Runge and E.K.U. Gross, Phys. Rev. Lett. E. Runge and E.K.U. Gross, Phys. Rev. Lett. 5252, 997 (1984), 997 (1984)

http://www.tddft.orghttp://www.tddft.org

There is a problem however!There is a problem however!

Nobody knows how the true Time-Dependent (or not) Density FunctionalNobody knows how the true Time-Dependent (or not) Density Functionalreally looks like and there are no known exact algorithms for its generation.really looks like and there are no known exact algorithms for its generation.

But we know that it exits for sure. But we know that it exits for sure.

3

ii i

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( ) ( ( , ), ( , ), ( , ), ( , )) ( , ) ( , ) ...

u ( , )[ ( , ) ( , ) ]u ( , ) [ ( , ) ( , )]v ( , )

[ ( , ) ( , )]u ( , ) [ ( , ) ( , ) ]v ( ,

ext

ext ext

ext ext

E t d r n r t r t r t j r t V r t n r t

r th r t V r t r t r t r t r t i

t

r t r t r t h r t V r t r t

iv ( , ))

r ti

t

For time-dependent phenomena one has to add currents.For time-dependent phenomena one has to add currents.

DFT has however a serious restriction. One can not extract any information DFT has however a serious restriction. One can not extract any information about two-body observables.about two-body observables.

For example, if we were to study the fission of a nucleus, we will in principle For example, if we were to study the fission of a nucleus, we will in principle determine the average masses of the daughters, but we will have no information determine the average masses of the daughters, but we will have no information about the width of the mass distribution. about the width of the mass distribution.

There is a relatively simple solution in time-dependent There is a relatively simple solution in time-dependent meanfield theory due to Balian and Veneroni (late 1980’s and early 1990’s) meanfield theory due to Balian and Veneroni (late 1980’s and early 1990’s)

1

0 1

1 1

0 1

2

0 020

( ) ( )

ˆ ˆ( , ) exp ( )exp

( , ) ( , )

1lim Tr ( ) ( , )

2

TDHF

TDHF

BVt

t t

t i Q t i Q

t t

Q t t

This method allows in principle the evaluation of both averages and widths.This method allows in principle the evaluation of both averages and widths.

John C. Tully suggested the following recipe for condensed matter John C. Tully suggested the following recipe for condensed matter and chemistry applicationsand chemistry applicationsJ. Chem. Phys. J. Chem. Phys. 9393, 1061 (1990), 1061 (1990)

( , , ) ( , )i ii

r R t c R t r R

exp ( ) ( ) exp ( ) ( )2

exp ( )

f i ab ab abcd cdabcdn ab

ab abcd cd a bab cd

tiH t t d n i n V n

i t T V n

The best solution however is to implement and treat the auxiliary fields The best solution however is to implement and treat the auxiliary fields as stochastic Stochastic TD-SLDAas stochastic Stochastic TD-SLDA

In 3D this is a problem for the petaflop to exaflop supercomputers In 3D this is a problem for the petaflop to exaflop supercomputers

For the sake of discussion let us see what we could in principle be able toFor the sake of discussion let us see what we could in principle be able tocalculate?calculate?

• We do not need to determine any collective coordinates, potential energy We do not need to determine any collective coordinates, potential energy surfaces, inertia tensor, non-abelian gauge fields, etc. as the system will find surfaces, inertia tensor, non-abelian gauge fields, etc. as the system will find naturally the right collective manifoldnaturally the right collective manifold

• We will not need to assume either isentropic, isothermal, … meanfield solutions. We will not need to assume either isentropic, isothermal, … meanfield solutions. Instead the temperature and entropy of the collective subsystem will evolve according Instead the temperature and entropy of the collective subsystem will evolve according to the rules of QM. This will be the most natural framework to describe dissipationto the rules of QM. This will be the most natural framework to describe dissipationin collective nuclear motion.in collective nuclear motion.

• We should be able to compute directly the mass, charge distributions and the We should be able to compute directly the mass, charge distributions and the excitation energy distributions of each fragmentexcitation energy distributions of each fragment

•We should be able to follow in real time a real experimental situation, We should be able to follow in real time a real experimental situation, such as induced fission or fusionsuch as induced fission or fusion

All this is naturally not limited to nuclear physics alone, this is a All this is naturally not limited to nuclear physics alone, this is a general approach to solve a large class of many-body problems general approach to solve a large class of many-body problems numerically exactly, with quantifying errors, within the next decade numerically exactly, with quantifying errors, within the next decade … … or sooner.or sooner.

Stochastic fields within a real time path integral approach

Nx = 70

Totals fncs = 718,112 , PEs = 102,590 , Memory = 167.44 TB /PE fncs = 7 , Memory = 2.00 GB

INS / PE : .5118990983368 e+12 Total INS : 5.251572849837231 e+17

FP_OP / PE : .1924037159156 e+12Total FP_OP : 1.97386972157814 e+17

Per Time Step ComputationalComplexity

Per Ensemble

Per Time Step Extrapolation for n = 1000

*between 1 and 2 minutes per step at this scale -can be improved almost ideally by strong scaling

fncs = 718,112,000

PEs = 102,590,000

Memory = 1.288706560512 e+18 B

Total INS / TS : 5.25157284983723 e+20Total FP_OP / TS : 1.97386972157814 e+20