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In the format provided by the authors and unedited.
Stable Compound of Helium and Sodium at High Pressure Xiao Dong,1, 2, 3 Artem R. Oganov,3-6*, Alexander F. Goncharov,7,8, Elissaios Stavrou,7,9 Sergey Lobanov,7,10
Gabriele Saleh,5 Guang-Rui Qian,3 Qiang Zhu,3, Carlo Gatti,11 Volker L. Deringer12, Richard Dronskowski12,
Xiang-Feng Zhou,1, 3* Vitali Prakapenka,13 Zuzana Konôpková,14 Ivan Popov,15 Alexander I. Boldyrev15 and
Hui-Tian Wang1,16*
1School of Physics and MOE Key Laboratory of Weak-Light Nonlinear Photonics, Nankai University, Tianjin 300071, China
2Center for High Pressure Science and Technology Advanced Research, Beijing 100193, China
3Department of Geosciences, Stony Brook University, Stony Brook, New York 11794-2100, USA
4Skolkovo Institute of Science and Technology, 3 Nobel St., Moscow 143026, Russia
5Moscow Institute of Physics and Technology, 9 Institutskiy Lane, Dolgoprudny city, Moscow Region, 141700, Russia
6International Centre for Materials Discovery, Northwestern Polytechnical University, Xi’an, 710072, China
7Geophysical Laboratory, CIW, 5251 Broad Branch Road, Washington, D.C. 20015, USA
8 Key Laboratory of Materials Physics and Center for Energy Matter in Extreme Environments, Institute of Solid
State Physics, Chinese Academy of Sciences, 350 Shushanghu Road, Hefei, Anhui 230031, China
9Lawrence Livermore National Laboratory, Physical and Life Sciences Directorate, P.O. Box 808 L-350, Livermore, California 94550, United States
10Sobolev Institute of Geology and Mineralogy Siberian Branch Russian Academy of Sciences, 3 Pr. Ac. Koptyga, Novosibirsk 630090, Russia.
11Istituto di Scienze e Tecnologie Molecolari del CNR (CNR-ISTM) e Dipartimento di Chimica, Universita’ di Milano, via Golgi 19, 20133 Milan, Italy
12Chair of Solid-State and Quantum Chemistry, RWTH Aachen, D-52056 Aachen, Germany
13Center for Advanced Radiation Sources, University of Chicago, Chicago, IL 60637, USA
14Photon Science DESY, D-22607 Hamburg, Germany
15Department of Chemistry and Biochemistry, Utah State University, Logan, Utah 84322, USA.
16 Collaborative Innovation Center of Advanced Microstructures, Nanjing University, Nanjing, 210093, China
Stable compound of helium and sodium at high pressure
© 2017 Macmillan Publishers Limited, part of Springer Nature. All rights reserved.
SUPPLEMENTARY INFORMATIONDOI: 10.1038/NCHEM.2716
NATURE CHEMISTRY | www.nature.com/naturechemistry 1
0
10
20
30
Fre
que
ncy(
TH
z)
WKWXLW
Supplementary fig. 1. Phonon dispersion curves of Na2He at 300 GPa, computed using PHONOPY and VASP.
0 200 400 600 800
-0.137
-0.136
-0.135
-0.134
-0.133
-0.132
-0.131
-0.130
G(e
V/a
tom
)
temperature(K)
Supplementary fig. 2. Predicted Gibbs free energy of formation of Na2He as a function of temperature at the
pressure of 300 GPa.
Supplem
GPa after
reflecting
is in cont
Supplem
were reco
mentary fig. 3.
r laser heatin
g Re gasket),
tact with He m
mentary fig. 4.
orded at 300 K
. Microphoto
ng to >1500 K
which consis
medium that i
-200
Ram
an In
tens
ity (a
rb. u
nits
)
Raman spec
K using differ
graph of the
K. The sampl
sts of mixture
is seen as a tr
0
Na
ctra of Na2He
rent excitatio
DAC high-p
le (dark area
of tI19 Na an
ransparent are
Na2He+
Raman Shi
200
a
e at 140 GPa.
n wavelength
ressure cavity
close to the c
nd Na2He det
ea near the edg
+Na 140 GPa
ift (cm-1)
400
532 nm 488nm
660 nm
Na
The sample
hs.
y in reflected
center of the
termined by X
ge of the gask
600
a2He
was laser he
d and transmi
diamond cule
XRD and Ram
ket.
ated to >1500
itted light at
et surrounded
man spectrosc
0 K. The spe
140
d by
copy,
ectra
Supplem
conventio
mentary fig. 5.
onal cell. The
He
Na
2e
Computed ch
e color bar giv
harge density
ves the scale.
(eÅ -3) of Na
a2He at 300 GGPa, plotted inn the [110] pla
0.37
0.20
0.54
ane of the
0.0 0.2 0.4 0.6 0.8 1.0-0.1
0.0
0.1
0.2
0.3
0.4
H
form
atio
n(e
V/a
tom
)
composition, He/(Na+He)
Supplementary fig. 6. Predicted enthalpies of formation in the Na-He system at 200 GPa - i.e., the elements sodium
(left-hand side) and helium (right-hand side) are set as the energy zero.Na2He is predicted to be thermodynamically
stable.
Supplementary fig. 7. Predicted enthalpies of formation in the (a) K-Ne and (b) Na-Ne system at 1000 GPa. In both
cases, there is no structure with negative formation enthalpy relative to the elements (that is, below zero) over the
entire compositional range. There are no K–Ne or Na–Ne compounds.
0.0 0.2 0.4 0.6 0.8 1.0
0.0
0.5
1.0
1.5
Hfo
rmat
ion(
eV/a
tom
)
composition, Ne/(Na+Ne)
0.0 0.2 0.4 0.6 0.8 1.0
0.0
0.5
1.0
1.5
Hfo
rmat
ion(
eV
/ato
m)
composition, Ne/(K+Ne)
a b
Supplem
The upp
electrons
interstitia
mentary fig. 8.
er bands sho
s. Such band s
ally localized
-53
-43
-33
-23
-13
-3
7
Ener
gy (
eV
)
L
W
. Electronic b
own include
structures are
electrons). T
L
band structure
both valence
e typical of sa
The inset show
X
e of Na2He a
e and conduc
alts, in this ca
ws charge den
KW
at 300 GPa, in
ction bands,
ase we have a
nsity of the hig
ndicating pre
are mostly d
an electride (a
ghest-occupie
Na 2s
Na 2p
He 1s
W
edominant cha
due to inters
a salt made o
ed bands.
aracter of ban
stitially locali
f ionic cores
nds.
ized
and
Supplem
zero. Tot
Bader vo
volumes1
Supplem
Na-He an
approxim
mentary fig. 9.
tal DOS unit
olumes (inclu1, 2. For inters
mentary fig. 1
nd He-ES int
mation (TB-LM
0
2
4
0.0
0.1
0.2
0.0
0.2
0.4
0.0
0.4
0.8
D
ensi
ty o
f st
ates
Total and pro
ts are states/e
uding intersti
titial electron
0. Calculated
teractions, ob
MTO-ASA p
-2 0
ojected densit
eV. In this ca
itial electron
ns, we use hyd
d integrated
tained using
program). ES
0 2
Total
Na_s Na_p Na_d
He_s He_p
Energy
InterstitiaInterstitia
ties of states (
alculation, w
s) and calcu
drogen orbital
crystal orbita
tight-binding
represents “e
4 6
y (eV)
al_sal_p
(DOS) of Na2
e project the
ulate the corr
ls to project.
al Hamilton
g linear muffi
empty sphere
8
2He at 300 GP
Kohn-Sham
responding de
populations (
in-tin orbital m
es”, which are
10
Pa. The Ferm
m wave functi
ensity of sta
(ICOHP) for
method in the
e inserted in
mi energy is se
ions onto ato
ates within th
r Na-ES, Na-
e atomic sphe
the center of
et as
omic
hese
-Na,
eres
f the
empty Na
He and E
Supplem
at high an
pressures
simple-cu
the LMT
dominate
both case
above are
sketched
Supplem
pressure.
subseque
a8 cubes to de
ES 1s (2p, 3d
mentary fig. 11
nd ultrahigh p
s of around 10
ubic Na fram
TO computatio
ed by electros
es, the He 1s o
e practically z
here and elab
mentary fig. 12
We take a
ently relaxing
escribe the lo
downfolded).
1. Simplified d
pressures. Na
00 GPa (left-hework to the
ons above). W
static interacti
orbitals are no
zero); nonethe
borated in the
ener
gy(e
V)
2. Energies of
3*3*3 face-
the structure
calized electr
. For further i
drawing, illus
atoms are dr
hand side), th
1s orbitals us
When pressure
ions, in line w
ot involved in
eless, the pres
e main text.
0 1013
14
15
16
17
18
19
ener
gy(e
V)
f the Na-3s an
-centered cub
at the specifi
rons (2e). The
interpretation
strating the bo
awn in gray,
here are coval
sed to describ
e is increased
with the increa
n the covalent
sence of He i
20 30 40
pressure
nd He-1s orbi
bic (fcc) supe
fic pressure.
e valence con
n of the ICOH
onding pictur
He atoms in g
ent contributi
e localized in
further (righased charge tr
t interactions
s the key dete
0 50 60
e(GPa)
Na 3sHe LUM
itals relative t
er-cell of He
nfigurations ar
HP results, see
re obtained fro
green, and int
ions from the
nterstitial elec
t-hand side),
ransfer as dis
(and thus the
erminant for t
70 80
MO
to He matrix
e and replace
re Na 3s (3p,
e the cartoon b
om COHP an
terstitial elect
3s orbitals of
ctrons (“2e”; d
the compoun
cussed in the
e correspondin
the stabilizati
HOMO level
e the central
3d downfold
below.
nalysis for Na2
trons in blue.
f the
denoted “ES”
nd becomes
main text. In
ng ICOHPs
on mechanism
l as a function
l atom with
ded),
2He
At
” in
n
m
n of
Na,
Supplementary table 1. Description of the experimental runs.
Run # Pressure
(GPa)
Na Phase Na
Lattice
parameter
Na Vp.a.
Heating
Conditi
ons
Na2He
Lattice
parameter
Na2He
Volume
Comments
APS
5 141 tI19 7.0820, 3.488 9.064 After LH 4.296 79.285 Na2He observed after LH.
W used as pressure marker.
4 155 tI19
7.028, 3.420
8.753
After LH 4.260 77.309 Na2He observed before
and after LH at each
pressure
4 150 tI19
tI19 at Na2He
7.010, 3.438
7.000, 3.430
8.753
8.708
After LH 4.245 76.495 Na2He observed before
and after LH at each
pressure
4 140 tI19
tI19 at Na2He
7.100, 3.482
7.090, 3.475
9.089
9.051
After LH 4.315 80.342 Na2He observed before
and after LH at each
pressure
4 130 tI19 at Na2He
oP8 at Na2He
7.180, 3.480
4.750, 3.010,
5,240
9.277
9.364
Before
LH
4.345 82.029 The first heating for the
run#4.
Na2He observed before
and after LH.
4 110 cI16 5.462 10.184 RT - - Na2He not observed
4 100 FCC Na 3.484 10.57 RT - - Na2He not observed
3 135 tI19
oP8?
7.19, 3.5 9.37 After LH 4.29 78.953 Na phases are away from
Na2He and at lower
pressure. Estimated lattice
parameters suggest lower
pressure for Na.
3 113 FCC Na
oP8 or tI19
3.498 10.70
After
LH
4.41 85.76 Large pressure gradient.
Different phases at
different points. Na2He
is seen near the position
where traces of oP8 and/or
tI19 phases are observed.
PETRA
2 110 cI16 5.446 10.098 RT - - Na2He not observed
2 117 cI16 5.401 9.850 RT and 323 K
- - Na2He not observed
Supplementary table 2. Miller indices (hkl), interplanar distances (dcal) and peak intensities (Ical) calculated for the
Fm-3m Na2He phase at 141 GPa, with unit cell parameter a= 4.2960 Å3 together with observed interplanar distances
(dobs) and peak intensities (Iobs).
hkl dcal (Å) Ical dobs (Å) Iobs dcal-dobs 111 2.4803 1.8 2.4790 <5 0.0013 200 2.1480 100 2.1480 100 0 220 1.5188 93 1.5178 98 0.001 311 1.3143 0.5 Not observed 222 1.2401 22 1.2392 21 0.001 400 1.0740 12 1.0757 20 -0.0017 331 0.9856 0.1 Not observed 420 0.9606 23 0.9669 27 -0.0063
Supplementary table 3. Atomic radii in K-Ne and Na-Ne systems at 1000 GPa. Radii were obtained for
the most stable structures of compounds with the same stoichiometry A2Ne (A=K, Na), using the
same method as in Table I.
Compounds A Radius (Å) Ne Radius (Å) Radius ratio
(RNe/RA)
Formation enthalpy
(eV/atom)
Na2Ne 0.59 0.62 1.05 +0.23
K2Ne 0.86 0.68 0.79 +0.90
K2Ne has a better radius ratio than Na2Ne, yet has a higher enthalpy of formation. Stability of Na2He
is not just a result of favorable packing of the atoms (in that case, Na2Ne should be even more stable).
Supplementary table 4. Charge density, kinetic energy density per electron and total energy density per
electron at the bond critical points in Na2He at 300 GPa. In the first and second line, values obtained
from PBE-DFT and Hartree-Fock calculations, respectively, are reported. In the first column, the
attractor of the associated bond paths are given. All values are in atomic units. Kinetic energy density
was calculated according to the following equation: G(r)= 1/2 (’)(1)(r,r’)r=r’ . The total
energy density was obtained as H=G+V, where V was calculated according to the local form of the
virial theorem reported in ref G1.
Attractors ρBCP∙102 GBCP/ρBCP HBCP/ρBCP
He-Na 4.76
4.27
1.72
1.97
0.19
0.31
Na-Na 3.59
3.11a
1.77
2.09a
0.30
0.45a
He- Interstitial 3.57
3.32
0.71
0.84
-0.23
-0.19
Na- Interstitial 5.30
5.68
0.62
0.79
-0.30
-0.31 a Using Hartree-Fock Hamiltonians, no Na-Na bond critical points were found. We report the value of properties at Na-Na midpoint
(which corresponds to a ring critical point in this case)
Supplementary table 5. Calculated Bader charges and radii (relative to Na), at pressures of 200, 300 and
500 GPa. For comparison, we list Bader charges in hP4-Na.
pressure hp4-Na Na2He
(GPa) Item charge item charge radius radio
200
Na1 0.571 Na 0.599 1.000
Na2 0.505 He -0.174 0.852
2e -1.076 2e -1.022 0.772
300
Na1 0.603 Na 0.601 1.000
Na2 0.508 He -0.159 0.834
2e -1.108 2e -1.043 0.755
500
Na1 0.644 Na 0.612 1.000
Na2 0.511 He -0.146 0.820
2e -1.155 2e -1.079 0.740
Mulliken charges have surprisingly similar values to Bader charges, at 300 GPa they are:
He(Na2He) -0.162, Na(Na2He) +0.621, Interstitial (Na2He) -1.081
Na1(hP4-Na) +0.503, Na2(hP4-Na) +0.552, Interstitial (hP4-Na)- 1.055
Supplementary table 6. SSAdNDP and NBO results for the Na2He system at different pressures. In this study ccemd-2 basis set was used to represent the projected plane-wave density using a 7x7x7 k-point grid. This basis set was selected so that on average less than 1% of the density of each occupied plane wave band was lost in projecting into the AO basis to guarantee that the density matrix used in the SSAdNDP procedure accurately represents the original plane wave results.
0 GPa 100 GPa 300 GPa 500GPa
NBO: q(He)=0.00 q(Na)=0.00 ON(LP on He)=1.99 |e| Na: 0.95 |e| on 3S orbital 0.02 on each three 3P orbitals 2.00 |e| on 2S orbital 2.00 |e| on each three 2P orbitals He: 2.00 |e| on 1S orbital 0.01 on 2S orbital 0.00 on each three 2P orbitals SSAdNDP: I) ON(LP on He) = 1.99|e| a) ON(8c-2e over Na8 empty cube)=1.40 |e| b) ON(14c-2e over Na8He6)=1.41 |e| II) ON(8c-2e over Na8 empty cube)=1.39 |e| ON(9c-2e over Na8He cube) = 2.00 |e|
NBO: q(He)=+0.13 q(Na)=-0.07 ON(LP on He)=1.84 |e| Na: 0.43 |e| on 3S orbital 0.23 |e| on each three 3P orbitals 1.96 |e| on 2S orbital 1.98 |e| on each three 2P orbitals He: 1.84 |e| on 1S orbital 0.03 on 2S orbital 0.00 on each three 2P orbitals SSAdNDP: I) ON(LP on He) = 1.84|e| a) ON(8c-2e over Na8 empty cube)=1.80 |e| b) ON(14c-2e over Na8He6)=1.82 |e| II) ON(8c-2e over Na8 empty cube)=1.75 |e| ON(9c-2e over Na8He cube)=1.97 |e|
NBO: q(He)=+0.22 q(Na)=-0.11 ON(LP on He)=1.74 |e| Na: 0.23 |e| on 3S orbital 0.34 |e| on each three 3P orbitals 1.93|e| on 2S orbital 1.97 |e| on each three 2P orbitals He: 1.74|e| on 1S orbital 0.04 on 2S orbital 0.00 on each three 2P orbitals SSAdNDP: I) ON(LP on He) = 1.74|e| a)ON(8c-2e over Na8 empty cube)=1.88 |e| b) ON(14c-2e over Na8He6)=1.90 |e| II) ON(8c-2e over Na8 empty cube)=1.81 |e| ON(9c-2e over Na8He cube)=1.95 |e|
NBO: q(He)=+0.25 q(Na)=-0.13 ON(LP on He)=1.70 |e| Na: 0.18 |e| on 3S orbital 0.37 |e| on each three 3P orbitals 1.91 |e| on 2S orbital 1.97 |e| on each three 2P orbitals He: 1.70 |e| on 1S orbital 0.05 on 2S orbital 0.00 on each three 2P orbitals SSAdNDP: I) ON(LP on He) =1 .70|e| a)ON(8c-2e over Na8 empty cube)=1.89 |e| b) ON(14c-2e over Na8He6)=1.91 |e| II) ON(8c-2e over Na8 empty cube)=1.82 |e| ON(9c-2e over Na8He cube)=1.94 |e|
Supplementary method
PERIODIC CALCULATIONS WITH CRYSTAL14
BASIS SET
Triple zeta basis sets were used for all atoms. Such basis functions were taken from Refs. 3,4 (for Na and He,
respectively) and slightly modified to be apt for high-pressure calculations. Indeed, due to the fact that such basis
sets were optimized for solid state structures at zero pressure (Na) and for isolated atoms (He), it was not possible to
obtain convergence without modifying the exponents.
Additional basis functions centered on non-nuclear charge density maxima were employed. Such functions were
identical to the ones used for He with the only difference that the most internal, very contracted s shell was not
considered (due to the fact that interstitial electrons have no nuclei and therefore there is not a strong contraction of
electrons towards the maximum as it happens for atoms). Numerical values for exponents and contraction
coefficients for 300 GPa calculations are given in the following table (for Hartree-Fock calculations, used to obtain
bond critical points properties, an additional shrinking of the basis functions of Na was necessary to obtain
convergence. For those basis functions where a different exponent was used for Hartree-Fock calculations, its value
is reported in brackets).
Type of function exponent Contraction coefficient
Na atom
s
2.60E+04 6.18E-04
3.91E+03 4.78E-03
8.89E+02 2.45E-02
2.52E+02 9.48E-02
8.17E+01 2.69E-01
2.89E+01 4.79E-01
1.06E+01 3.33E-01
s 5.38E+01 1.95E-02
1.63E+01 9.27E-02
2.37E+00 -3.99E-01
s 9.57E-01 1.64E+00
4.08E-01 5.57E-01
s 6.75E-01
(1.62E+00)1.00E+00
s 1.97E-01
(4.02E-01)1.00E+00
p
1.38E+02 5.80E-03
3.22E+01 4.16E-02
9.98E+00 1.63E-01
3.48E+00 3.60E-01
1.23E+00 4.49E-01
p 4.01E-01 1.00E+00
(9.63E-01)
p 1.97E-01
(4.03E-01)1.00E+00
d 1.05E+00
(2.51E+00)1.00E+00
d 5.31E-01
(1.08E+01)1.00E+00
He atom
s
2.34E+02 2.59E-03
3.52E+01 1.95E-02
7.99E+00 9.10E-02
2.21E+00 2.72E-01
s 6.67E-01 1.00E+00
s 2.09E-01 1.00E+00
p 3.04E+00 1.00E+00
p 7.80E-01 1.00E+00
d 1.97E+00 1.00E+00
Interstitial electron s 6.67E-01 1.00E+00
s 2.09E-01 1.00E+00
p 3.04E+00 1.00E+00
p 7.80E-01 1.00E+00
d 1.97E+00 1.00E+00
GRID OF K-POINTS
In the following table, details regarding the k-nets for the crystal systems considered in the paper are reported. The
‘Gilat net’ is used for the calculation of the density matrix
Pressure system shrink factor in
the input
total k-points in
reciprocal space
(IBZ)
total k-points for
‘Gilat net’
300 GPa
Na2He 24 48 413 2769
Na 12 24 133 793
He 12 24 133 793
GRID FOR DFT
For the evaluation of charge density to be used in DFT calculations, we used the following input, corresponding to
unpruned grids (see http://www.crystal.unito.it/Manuals/crystal14.pdf for full description of the various parameters)
RADIAL
1
x
99
ANGULAR
1
9999.0
13
TOLLDENS
9
where x was 3.0, 3.0 and 2.0 for Na2He, Na and He, respectively.
Finally, regarding the evaluation of bielectronic integrals (TOLINTEG option), we used
TOLINTEG=12,12,12,12,22 for Na2He and hp4-Na, while for He we used TOLINTEG=11,11,11,11,22 (see
http://www.crystal.unito.it/Manuals/crystal14.pdf for full description of the various parameters)
INTERACTION OF ZERO-FLUX SURFACES, CRITICAL POINT ANALYSIS AND GENERATION OF
GRID FILES
The program TOPOND7 (incorporated in CRYSTAL 14) was used for the evaluation of properties. To obtain the
deformation density isosurfaces, the grid files were produced with TOPOND, and transformed into ‘cube’ standard
format with the program NCImilano (Ref. 5). Isosurfaces were produced with MOLISO (Ref. 6) giving the files in
‘cube’ format in input.
For the integration over zero-flux surfaces, we used 64 and 48 ϕ and θ angular points outside the β-sphere. Inside
the β-sphere, 120 radial points were used. For the number of radial points outside the β-sphere and the angular
points inside the β-sphere, we used the option IMUL=2, which corresponds to doubling the number of points with
respect to the default value.
Atomic energy was calculated according to the following equation:
E()=K()(1+V/T)
where
K()= -1/4(2 +‘2)(1)(r,r’)r=r’d . is the space enclosed by zero-flux surfaces, and V/T is the virial ratio obtained from the SCF calculation.
Supplementary References
1 Bader, R. F. Atoms in molecules. (Wiley Online Library, 1990). 2 Henkelman, G., Arnaldsson, A. & Jonsson, H. A fast and robust algorithm for Bader decomposition of charge density.
Comput. Mat. Sci. 36, 354-360 (2006). 3 Peintinger, M. F., Oliveira, D. V. & Bredow, T. Consistent Gaussian basis sets of triple‐zeta valence with polarization
quality for solid‐state calculations. J. Comput. Chem. 34, 451 (2013). 4 Woon, D. E. & Dunning, T. H. Gaussian basis sets for use in correlated molecular calculations. IV. Calculation of static
electrical response properties. J. Chem. Phys. 100, 2975 (1994). 5 Saleh, G., Lo Presti, L., Gatti, C. & Ceresoli, D. NCImilano: an electron-density-based code for the study of
noncovalent interactions. J. Appl. Crystallogr. 46, 1513 (2013). 6 Hubschle, C. & Luger, P. MolIso-a Program for Colour-mapped Iso-surfaces. J. Appl. Crystallogr. 39, 901 (2006). 7 Gatti C., Saunders V. R., Roetti C. Crystal field effects on the topological properties of the electron density in
molecular crystals, J. Chem. Phys. 101, 10686-10696 (1994)