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Shell Effects – Erice 1. Magic Numbers of Boson Clusters. a) He cluster mass selection via diffraction. b) The magic 4 He dimer. c) Magic numbers in larger 4 He clusters? The Auger evaporation picture. Giorgio Benedek with J. Peter Toennies (MPI-DSO, Göttingen)

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Shell Effects – Erice 1

Magic Numbers of Boson Clusters

a) He cluster mass selection via diffraction

b) The magic 4He dimer

c) Magic numbers in larger 4He clusters? The Auger evaporation picture

Giorgio Benedek with

J. Peter Toennies (MPI-DSO, Göttingen)

Oleg Kornilov (UCB, Berkeley)

Elena Spreafico (UNIMIB, Milano)



from J. P. Toennies mass 8 and larger



Searching for Large mass 8 and larger4He Clusters: 4HeN

N = 4,5,6….

from J. P. Toennies

He2+


from J. P. Toennies mass 8 and larger


Effective Slit Widths vs Particle Velocity mass 8 and larger

He Atom

versus

He Dimer

64

C

3

-

V (particle-wall) =

3

X

63

D

S

eff

3

C =0.12 meV nm

=2.5

3

]

He

62

m

nm

n

[

f

f

e

s

61

h

t

d

i

W

60

t

He

i

l

2

S

e

59

v

i

t

c

e

<R> = 52.0

+

f

f

E

58

2

~

E

-

2

b

4m

<R>

57

.

-3

=1.2 10 K

=1.1

10-3 K

56

o

o

0

500

1000

1500

2000

Particle Velocity v [m/s]

Scattering length a = 2 <R> = 97 A

Grisenti, Schöllkopf, Toennies Hegerfeldt, Köhler and Stoll

Phys. Rev. Lett. 85 2284 (2000)

2003-07-02-T1-Schr.

0.4 A

10-3 K

1

°

104 A

Grisenti; Schöllkopf, Toennies, Hegerfeldt, Köhler and Stoll, Phys. Rev. Lett. 85 2284 (2000)


The mass 8 and larger4He dimer: the world‘s weakest bound and

largest ground state molecule

Since <R> is much greater than Rout the dimer

is a classically forbidden molecule

<R>

A frail

GIANT!

High SR

from J. P. Toennies


To Further Study the Dimer it is Interesting mass 8 and larger

to Scatter from an Object Smaller than the Dimer: an Atom!

A.Kalinin, O. Kornilov, L. Rusin, J. P. Toennies, and G. Vladimirov, Phys. Rev. Lett. 93, 163402 (2004)


from J. P. Toennies mass 8 and larger

The Kr atom can pass through

the middle of the molecule

without its being affected

The dimer is nearly invisible:

magic!

trim

end of lecture 6


b) Magic numbers (or stability regions) mass 8 and larger

  •  Classical noble gas (van der Waals) clusters:

  • - geometrical constraints only

    • - magic numbers = highest point symmetry

 Quantum Bose clusters (4He)N are superfluid

- no apparent geometrical constraint

- no shell-closure argument

are there magic numbers or stability regions for boson clusters?

Shell Effects – Erice 2


4 he clusters
4 mass 8 and largerHe clusters

T0= 6.7K

P0 ≥ 20bar

T= 0.37K

- formed in nozzle beam

vacuum expansion

- stabilized through

evaporative cooling

clusters are superfluid!

Shell Effects – Erice 3


Theory (QMC): no magic numbers predicted for 4He clusters!

- R. Melzer and J. G. Zabolitzky (1984)

- M. Barranco, R. Guardiola, S. Hernàndez, R. Mayol, J. Navarro, and M. Pi. (2006)

Binding energy per atom vs. N:

a monotonous slope, with no peaks nor regions of larger stability!

Shell Effects – Erice 4


More recent highly accurate diffusion Monte Carlo (T=0) calculation

rules out existence of magic numbers due to stabilities:

Cluster Number Size N

R. Guardiola,O. Kornilov, J. Navarro and J. P. Toennies, J. Chem Phys, 2006


Diffraction experiments with neutral ( calculation4Ne)N clusters

show instead stability regions!

Shell Effects – Erice 5


Magic numbers, excitation levels, and other properties of small neutral

4He clusters

Rafael Guardiola

Departamento de Física Atómica y Nuclear, Facultad de Fisica, Universidad de Valencia, 46100 Burjassot,

Spain

Oleg Kornilov

Max-Planck-Institut fur Dynamik und Selbstorganisation, Bunsenstrasse 10, 37073 Gottingen, Germany

Jesús Navarro

IFIC (CSIC-Universidad de Valencia), Apartado 22085, 46071 Valencia, Spain

J. Peter Toennies

Max-Planck-Institut fur Dynamik und Selbstorganisation, Bunsenstrasse 10, 37073 Gottingen, Germany


R. Brühl, R. Guardiola, A. Kalinin, O. Kornilov, J. Navarro, T. Savas and J. P. Toennies,

Phys. Rev. Lett. 92, 185301 (2004)

Shell Effects – Erice 6


The size of Navarro, T. Savas and J. P. Toennies, 4He clusters

QMC (V. R. Pandharipande, J.G. Zabolitzky, S. C. Pieper, R. B. Wiringa, and U. Helmbrecht,

Phys. Rev. Lett. 50, 1676 (1973)

R(N) = (1.88Å) N 1/3 + (1.13 Å) / (N 1/3 1)

Shell Effects – Erice 7


Single-particle excitation theory of evaporation and cluster stability

spherical box model

Magic numbers!

Shell Effects – Erice 8


Atomic radial distributions stability

4Hen

3Hen

Barranco et al (2006)


Fitting a spherical-box model (SBM) to QMC calculations stability

Condition: same number of quantum single-particle levels

this can be achieved with:

- a(N) = QMC average radius

- V0(N) = μBof bulk liquid

- a constant effective mass m*

From:

Shell Effects – Erice 12


QMC (Pandharipande et al 1988) stability

the linear fit of QMC shell energies () for (4He)70 rescaled to the bulk liquid μB gives

m*~ 3.2 m

this m*/m value works well for all N since

Shell Effects – Erice 13


The Auger-evaporation mechanism stability

exchange-symmetric two-atom wavefunction


6-12 Lennard-Jones potential stability

= 40 Å3

C6 = 1.461 a.u.

d0<r <R(N)

Integration volume

R(N) = cluster radius

Shell Effects – Erice 10


Tang-Toennies potential stability

Replaced by co-volume (excluded volume)

Shell Effects – Erice 11


- Center-of-mass reference stability

total L = even

μ() = 7.3 K

m* = 3.2  4 a.u.

- Auger-evaporation probability

Shell Effects – Erice 14


Shell Effects – Erice 15 stability

- Cluster kinetics in a supersonic beam

stationary

fission and coalescence neglected:

cluster relative velocity very small

- Cluster size distribution:

- Comparison to experiment:

Jacobian factor

Gaussian spread (s  0.002)

Ionisation efficiency


Calculated stability4He cluster size distribution at different temperatures

Shell Effects – Erice 16




at each insertion of a new bound state stability

Guardiola et al thermodynamic approach

HeN-1 + He ↔ HeN

Formation-evaporation equilibrium:

Equilibrium constant:

ZN = partition function:

Magic Numbers

Guardiola et al., JCP (2006)

SIF 2008 Genova - 14


In conclusion we have seen that… stability

 High-resolution grating diffraction experiments allow to study the

stability of 4He clusters

 Experimental evidence for the stability of the4He dimer and the existence of magic numbers in 4He boson clusters

  • A kinetic theory based on the Auger evaporation mechanism for a spherical-box model qualitatively accounts for the experimental cluster size distributions

 Substantial agreement with Guardiola et al thermodynamic approach:

magic numbers related to the insertion of new bound states with increasing N


Electron Microscope Picture of the SiN stabilityx Transmission Gratings

Courtesy of Prof. H. Smith and Dr. Tim Savas, M. I. T.


Lecture 2: Helium Droplets stability

Grebenev, Toennies & Vilesov

Science 279, 2083 (1998)


Helium Droplets stability

T0 ≤ 35 K

P0 ≥ 20 bar

Droplets are cooled

by evaporation to

=0.37 K (4He),

=0.15 K (3He)

Brink and Stringari,

Z. Phys. D 15, 257 (1990)


Some Microscopic Manifestations of Superfluidity stability

  • Free Rotations of Molecules

  • The Roton Gap (Phonon Wing)

  • Anomalously Small Moments of Inertia

How many atoms are needed for superfluidity?

How will this number depend on the observed

property?



OCS stability

Sharp spectral features indicate

that the molecule rotates without

friction

The closer spacing of the lines

indicates a factor 2.7 larger

moment of inertia

Is this a new microscopic manifestation of superfluidity?


2.Evidence for Superfluidity in Pure stability4He Droplets:

Near UV Spectrum of the S1 S0 Transition of Glyoxal

Since IR absorption lines are so sharp, what about electronic transitions?


The experimental sideband reflects the DOS of Elementary Excitations

Roton gap:

signature of superfluidity

rotational lines


Magic number in fermionic Excitations3He clusters

(Barranco et al, 2006)

(p + 1)(p + 2)(p + 3)/3

= 2, 8, 20, 40, 70, 112, 168, 240, 330, ...

stable for N > 30


Mixed Excitations4He/3He Droplets: Two Production Methods

Small 4He Clusters: N< 100

Large 4He Clusters: 100< N< 5000


4 ExcitationsHe / 3He phase separation

Barranco et al (2006)

4HeN3He


Stable Excitations4He + 3He mixed clusters

Barranco et al (2006)

4

3

2

1

0

1

3


Aggregation of Excitations4He Atoms Around an OCS Molecule

Inside a 3He Droplet

3He

OCS surrounded by a cage of 4He


IR Spectra of OCS in Excitations3He Droplets

with Increasing Numbers of 4He Atoms

~ 60 He atoms are needed to restore free rotations:

Number needed for superfluidity?

Grebenev Toennies and Vilesov Science, 279, 2083 (1998)


The Appearance of a Phonon Wing Heralds the Opening up of the Roton Gap

roton

maxon

Relative Depletion [%]

Wavenumber [cm-1]

According to this criterium 90 4He Atoms are needed for Superfluidity!

Pörtner, Toennies and Vilesov, in preparation


maxons: in both the Roton Gap4He and 3He

rotons: in 4He only


Localized phonon in the Roton Gap3He at the impurity molecule

Space localization  spectral localization!



electron – collective excitation coupling phonon width!

molecule

He atoms

spatial decay of molecule electronic wavefunctions


Inelastic part of dipolar matrix element: phonon width!

Sideband absorption coefficient:

Dynamic form factor:

interatomic potential

Response function:

non-interacting atoms

E = E(q)

Collective excitations:


Barranco et al phonon width!

“Shell” model for dynamics

n

n +1


particle-hole excitation spectrum phonon width!

collective excitation (phonon) spectrum



Non-condensed phonon width!

Bose condensed


para-Hydrogen phonon width!

Decrease in the moment

of inertia indicates

superfluidity

The reduced coordination

In small droplets favors

superfluid response

cartoon H2 on OCS


Aggregation of p-H phonon width!2 molecules around an OCS molecule inside a mixed 4He/3He droplet


(5-6 H phonon width!2)

(5-6 H2)

(3-4 H2)

(3 H2)


Average Moments of Inertia phonon width!

IaIb Ic

840 1590 1590

55 1590 1590

880 2500 2500

This is the first evidence

for superfluidity of p-H2


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