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Mendeleev’s principle against Einsteins relativity news from the chemistry of superheavy elements H.W. Gäggeler. Reminiscences: from Mendelejeev’s periodic table to the discovery of mendelevium, the last “real” chemical element - PowerPoint PPT Presentation
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Mendeleev; Dubna 2009
Mendeleev’s principle against Einsteins relativity news from the chemistry of superheavy elements
H.W. Gäggeler
> Reminiscences: from Mendelejeev’s periodic table to the discovery of mendelevium, the last “real” chemical element
> Positioning four new chemical elements into the periodic table during the last decade. Mendelejeevs dreams become true!
> How reliable is single atom chemistry? Proof of principle with elements Hs and 112
> Einsteins influence on the chemistry of heaviest elemenst, so far up to Z=114
Laboratory for Radiochemistry and Environmental Chemistry
Mendelejeev‘s „second“ Periodic Mendelejeev‘s „second“ Periodic Table from 1871Table from 1871
D.I. Mendeleev (8 Feb. 1834 – 2 Feb. 1907)
Predictions by Mendeleev in 1871Predictions by Mendeleev in 1871
Eka-Al: Discovered by P.E. Lecoq de Eka-Al: Discovered by P.E. Lecoq de Boisbaudran in 1875, named GaBoisbaudran in 1875, named Ga
Eka-B: Discovered by L.F. Nilson in Eka-B: Discovered by L.F. Nilson in 1879, named Sc1879, named Sc
Eka-Si: Discovered by C. Winkler in Eka-Si: Discovered by C. Winkler in 18886, named Ge18886, named Ge
Major refinementsMajor refinements
Noble gases: Sir William Ramsey Noble gases: Sir William Ramsey (1894)(1894)
Henry Moseley: Atomic number, Henry Moseley: Atomic number, determined via X-rays, defines determined via X-rays, defines ordering of elements (1914)ordering of elements (1914)
Glenn T. Seaborg: Actinides series Glenn T. Seaborg: Actinides series (1945)(1945)
Periodic Table in the 1930‘sPeriodic Table in the 1930‘s
G.T. Seaborg, W. D. Loveland (1990)
H
Li
Na
K
Rb
Cs
Fr Ra Ac
Ba
Sr
Ca
Mg
Be
Sc
Y
La
Ti
Zr
Hf
V
Nb
Ta
Cr
Mo
W
Mn
Tc
Re
Fe
Ru
Os
Co Ni Cu Zn Ga Ge As
Rh Pd Ag Cd In Sn Sb
Ir Pt Au Hg Tl Pb Bi
Rf Db
B C N O F
Al Si P S Cl
Se Br
Te I
Po At87 88 89-103 104 105
55 56 57-71 72 73 74 75 76 77
37 38 39 40 41 42 43 44 45 46 47 48 49 50 51 52 53
78 79 80 81 82 83 84 85
19 20 21 22 23 24 25 26 27 28 29 30 31 32 33 34 35
11 12 13 14 15 16 17
3 4
1
5 6 7 8 9
1
2
3 4 5 6 7 8 9 10 11 12
13 14 15 16 17
LanthanideLanthanidess
AAcctinidetinidess
114
He
Ne
Ar
Kr
Xe
Rn
54
86
36
18
10
2
18
Ce Pr Nd Pm Sm Eu Gd Tb Dy Ho Er Tm Yb Lu
Th Pa U Np Pu Am Cm Bk Cf Es Fm Md No Lr
58
90
59 60 61 62
91 92 93 94
63
95 96 97 98 99 100 101
64 65 66 67 68 69
102 103
70 71
La
Ac
57
89
Periodic Periodic TTable todayable today
Mt109 110
Ds111
Rg
Sg106
Bh107
Hs108 112
- -114
116 118113 115 116
Transuranium Elemens
SuperheavyElemens
StableElemens
SphericalShell
SphericalShell
208Pb
298114
Sea of Instability
10 20 30 40
Neutron number
Pro
ton
num
ber
50 60 70 80 90 100 110 120 130 140 150 160 170 180 190 200
130
120
110
100
90
80
70
60
50
40
30
20
10
0
LogT (sec)
1/2
14
-2
-6
6
10
2
CHART OF THE NUCLIDES
Courtesy: Yu.Ts. Oganessian
Mendeleev, Dubna 2009
Discovery of new elements – the failure of chemistry!
The heaviest element discovered purely by chemical means: Mendelevium! (1955)
→ Synthesis: bombardment of 253Es with -particles. → Collection of products in a foil. → Separation of products after dissolution of foil on a cation exchange column with -HIB
Elution of actinides on a cation exchange column by -HIB
Elution in drops
Cou
nt r
ate
[cpm
]
Mendeleev, Dubna 2009
Discovery of Mendelevium on the basis of 7 atoms
A. Ghiorso et al., Phys. Rev. 98, 1518 (1955)
Fm
Es Cfunknown
H
Li
Na
K
Rb
Cs
Fr Ra Ac
Ba
Sr
Ca
Mg
Be
Sc
Y
La
Ti
Zr
Hf
V
Nb
Ta
Cr
Mo
W
Mn
Tc
Re
Fe
Ru
Os
Co Ni Cu Zn Ga Ge As
Rh Pd Ag Cd In Sn Sb
Ir Pt Au Hg Tl Pb Bi
Rf Db
B C N O F
Al Si P S Cl
Se Br
Te I
Po At87 88 89-103 104 105
55 56 57-71 72 73 74 75 76 77
37 38 39 40 41 42 43 44 45 46 47 48 49 50 51 52 53
78 79 80 81 82 83 84 85
19 20 21 22 23 24 25 26 27 28 29 30 31 32 33 34 35
11 12 13 14 15 16 17
3 4
1
5 6 7 8 9
1
2
3 4 5 6 7 8 9 10 11 12
13 14 15 16 17
LanthanideLanthanidess
AAcctinidetinidess
114
- -
He
Ne
Ar
Kr
Xe
Rn
54
86
36
18
10
2
18
Ce Pr Nd Pm Sm Eu Gd Tb Dy Ho Er Tm Yb Lu
Th Pa U Np Pu Am Cm Bk Cf Es Fm Md No Lr
58
90
59 60 61 62
91 92 93 94
63
95 96 97 98 99 100 101
64 65 66 67 68 69
102 103
70 71
La
Ac
57
89
Positioning of new elements Positioning of new elements during the last decadeduring the last decade
Bh107
Hs108
Mt109 110
Ds111
Rg112
- -
Sg106
1999199919991999
Bh107
Hs108
2002200220022002
112
- -
Techniques developed at PSI and Bern University
116
114
20020077
20020077
20092009??
20092009??
Mendeleev, Dubna 2009
Reactions used and number of atoms found in the „first ever chemical studies“ during the last decade
Bohrium (Z=107); Main experiments at PSI249Bk(22Ne;4n)267Bh (T1/2 = 17 s); 6 atoms (R. Eichler et al., Nature, 407, 64 (2000))
Hassium (Z=108); Main experiments at GSI248Cm(26Mg;5n)269Hs(T1/2 = 15 s); 7 atoms (C.E. Düllmann et al., Nature, 418, 860 (2002))
Element 112; Main experiments at FLNR/JINR242Pu(48Ca,3n)287114 (T1/2 = 0.5 s)283112 (T1/2 = 4 s); 2 atoms (R. Eichler et al., Nature, 447, 72 (2007)). Confirmed with 3 additional atoms (R. Eichler et al., Angew. Chem. Int. Ed., 47(17), 3262 (2008)
Element 114: Main experiments at FLNR/JINR242,244Pu(48Ca;3,4n)287,288,289114 (T1/2 = 0.5s;0.8s;2.6s); 3 – 4 atoms (R. Eichler et al.,submitted to Nature (2008)).
Mendeleev, Dubna 2009
How reliable is single atom chemistry?1st example: hassium chemistry
Investigation of hassium in form of its very volatile molecule HsO4
Applied technique: Thermochromatography
ThermochromatographyThermochromatography
T=100KT=100KT=300KT=300K
detectorsdetectors
Result:Result: TTdepdep HHadsads
Temperature gradient
Tyi
eld
length
Internal chromatogramInternal chromatogram
Tdep
0
10
20
30
40
50
60
70
80
90
1 2 3 4 5 6 7 8 9 10 11 12Detector
Rel.
Yie
ld [
%]
-200
-180
-160
-140
-120
-100
-80
-60
-40
-20
0
Tem
pera
ture
[°C
]
Exp:269Hs (T1/2 =9.7 s)
Exp: 172Os (T1/2=19.2 s) MCS (Os): -39.5 kJ/molMCS (Hs): -46.5 kJ/mol
Temperature profile-82±5 °C
-44±5 °C
HsOHsO44
OsOOsO44
Thermochromatography of Thermochromatography of OsOOsO44 and HsO and HsO44
C.E. Düllmann et al., Nature 418,860 (2002)
1 atom
4 atoms
2 atoms
Mendeleev, Dubna 2009
Nobel Laureate Glenn T. Seaborg, The first human being, able to celebrate „his“ element!
Mendeleev, Dubna 2009
How reliable is single atom chemistry?2nd example: element 112
Element 112 presumably is highly volatile so that it can be separated and analysed in elemental form
Applied technique: Thermochromatography
H
Li
Na
K
Rb
Cs
Fr Ra Ac
Ba
Sr
Ca
Mg
Be
Sc
Y
La
Ti
Zr
Hf
V
Nb
Ta
Cr
Mo
W
Mn
Tc
Re
Fe
Ru
Os
Co Ni Cu Zn Ga Ge As
Rh Pd Ag Cd In Sn Sb
Ir Pt Au Hg Tl Pb Bi
Rf Db
B C N O F
Al Si P S Cl
Se Br
Te I
Po At87 88 89-103 104 105
55 56 57-71 72 73 74 75 76 77
37 38 39 40 41 42 43 44 45 46 47 48 49 50 51 52 53
78 79 80 81 82 83 84 85
19 20 21 22 23 24 25 26 27 28 29 30 31 32 33 34 35
11 12 13 14 15 16 17
3 4
1
5 6 7 8 9
1
2
3 4 5 6 7 8 9 10 11 12
13 14 15 16 17
LanthanideLanthanidess
AAcctinidetinidess
114
He
Ne
Ar
Kr
Xe
Rn
54
86
36
18
10
2
18
Ce Pr Nd Pm Sm Eu Gd Tb Dy Ho Er Tm Yb Lu
Th Pa U Np Pu Am Cm Bk Cf Es Fm Md No Lr
58
90
59 60 61 62
91 92 93 94
63
95 96 97 98 99 100 101
64 65 66 67 68 69
102 103
70 71
La
Ac
57
89
Periodic Periodic TTable todayable today
Mt109 110
Ds111
Rg
Sg106
Bh107
Hs108 112
- -114
116 118113 115 116
Trend of sublimation enthalpy within group 12Trend of sublimation enthalpy within group 12
?Mendeleev says: 112 an even more volatile metal compared to Hg!
However,…..
• Pitzer (1975) says: because of relativistic effects element 112 could well behave like a noble gas.
• Reason: E112 has a filled 6d107s2 electronic shell configuration
Relativistic effects
• High atomic number: strong Coulomb attraction causes electrons to move faster.
• Causes relativistic mass increase [m=m0(1-)], withv/c; and, as a consequence, contraction of spherical orbitals (ns, np1/2)
• Energy levels of spherical orbitals are increased• Energy levels of high angular momentum orbitals
are destabilized due to shielding effects by spherical orbitals
• Strong spin-orbit splitting
0.0
0.1
0.2
0.3
0.4
0.5
0 1 2 3 4 5 6 7
r (a.u.)
7sR
7sNR
6sR
6sNR
Example: the relativistic 6s/7s contraction in Au and Rg
a
B
h2
mc2
h2
m0c2
1 v2
c2 a
B0 1
v2
c2
Consequence: Cu, Ag, Au nd10(n+1)s1 Zn+,Cd+,Hg+ however: Rg, 112+ nd9(n+1)s2 (2D5/2)
E.Eliav, U.Kaldor, P.Schwerdtfeger, B.Hess, Y.Ishikawa, Phys. Rev. Lett. 73, 3203 (1994).M.Seth, P.Schwerdtfeger, M.Dolg, K.Faegri, B.A.Hess, U.Kaldor, Chem. Phys. Lett. 250, 461 (1996).
4r 2(r)
Courtesy:P. Schwerdtfeger
direct effect(contraction)
indirect effect(expansion)
relativisticnonrelativistic
Relativistic Effects
M.Kaupp, Spektrum der Wissenschaften, 2005
P. Pyykkö
How to experimentally determine a metallic character of a volatile element at a single
atom level?
→ Determine interaction energy (adsorption enthalpy) with noble metals (e.g. Au)
→ If metallic: strong interaction (adsorption enthalpy) if non-metallic (noble gas like): weak interaction
Metal Surface
Surface: Gold
0
5
10
15
20
25
30
35
40
45
50
1 3 5 7 9 11 13 15 17 19 21 23 25 27 29 31lenght [cm]
yiel
d [
%]
0
50
100
150
200
250
300
350
400
450
500
tem
per
atu
re [
K]
Hg-192 Hads = -87 kJ/mol
Rn-219 Hads = -27 kJ/mol
Quartz Surface
0
10
20
30
40
50
60
1 2 3 4 5 6 7 8 9 10 11 12 13 14 15 16 17 18 19 20 21 22 23 24 25 26 27 28 29 30 31 32lenght [cm]
yiel
d [
%]
0
50
100
150
200
250
300
350
400
450
500
tem
per
atu
re [
K]
Hg-192 Hads = -24.5 kJ/mol
Rn-219 Hads = -20.5 kJ/mol
Tdep. Tl, Po, Pb, Bi ≥ 500 K
The EPIPHANIOMETER
219Rn
211Pb
for 211Pb (via 211Bi)
(Teflon)
No 211Pb detected for clean gas (no aerosol particles)
H.W. Gäggeler et al., J. Aerosol Sci., 20, 557 (1989)
Application to atmospheric aerosol detection at exotic sites
Window/Target (242,244Pu)
Beam (48Ca)
Beam stop
SiO2-FilterTa metal850°C
Quartz column
Cryo On-line Detector (4Cryo On-line Detector (4 COLD)COLD)
Carrier gas He/Ar (70/30)
Teflon capillary
(32 pairs PIN diodes, one side gold covered)
HgHg Loop
Temperature gradient: 35°C to – 180 °C
T
l
RnRn
The element 112,114 experimentsThe element 112,114 experiments(IVO Technique)(IVO Technique)
112,114112,114??Recoil
chamber
Quartz inlay
283112
9.52 MeV
279Ds: 0.088 s
SF94+51 MeV
283112
9.52 MeV
279Ds: 0.072 s
SF112+n.d. MeV
283112
9.38 MeV
279Ds: 0.592 s
SF108+123 MeV
283112
9.47 MeV
279Ds: 0.536 s
SF127+105 MeV
283112
9.35 MeV
279Ds: 0.773 s
SF85+12 MeV
Observed in Chemistry:Observed in Chemistry:
283112
4 s
9.54 MeV
287114
0.51 s
10.02 MeV
279Ds0.18 s
SF(>90%)205 MeV
Reported at FLNR:Reported at FLNR:Oganessian et al. 2004Oganessian et al. 2004
291116
6.3 ms
10.7 MeV
The E112 experiments in 2006/2007The E112 experiments in 2006/2007
242Pu (48Ca, 3n) 2871146.2•1018 48Ca during eff. 32 days
(8 weeks absolute)
NR =0.05NR <1E-5
ResultsResults Monte Carlo simulationfor one single component
Experiment
(-5°C)(-5°C)
(-21°C)(-21°C)(-39°C)(-39°C) (-124°C)(-124°C)
(-28°C)(-28°C)
gas flowgas flow
Courtesy: R. Eichler
-52-52+4+4-3-3 kJ/mol kJ/mol
Trend of sublimation enthalpy within group 12Trend of sublimation enthalpy within group 12
Production of E114Production of E114242Pu (48Ca, 3n) 287114
284112
0.097 sSF
288114
0.8 s
9.95 MeV
2831124 s
9.54 MeV
287114
0.51 s10.02 MeV
279Ds0.2 sSF
285112
29 s
9.16 MeV
289114
2.6 s
9.82 MeV
281Ds11 sSF
244Pu (48Ca, 3-4n) 288-289114
Yu.Ts. Oganessian et al., 2004
0 80604020 120100
0
20
40
60
80
100
120
Standard enthalpies of gaseous monoatomic elements
Atomic number
H° 2
98 [
kcal/m
ol]
B. Eichler, 1974
283112 10.93 s
9.53
287114
10.04 MeV
279Ds: 0.242 s
SF 114+103
284112: 0.11 s
SF 62+n.d.
288114
9.95 MeV
284112
: 0.10 s
SF 108+n.d.
288114
9.81 MeV
242Pu (48Ca, 3n) 287114 244Pu (48Ca, 3-4n) 288-289114
285112
9.20 MeV
289114
281Ds: 3.38 s
SF 106+44
1.43•1019 48Ca during 51 days3.1•1018 48Ca during 16 days
NR=1.8E-3
NR=1.1E-2NR=2E-2
NR=1.5E-3
Results with element 114Results with element 114Dubna 2007Dubna 2007
Det#4
Det#6
- 2008- 2008
-200-150-100-50050
-200-150-100-50050
-200-150-100-50050
0369
1215
(288114)
288114
0369
1215
R
el. y
ield
/ d
ete
cto
r, %
Te
mp
era
ture
, °C
287114
2 4 6 8 10 12 14 16 18 20 22 24 26 28 30 320369
1215
(289114-->285112)
Detector #
goldgold iceice
-88°C-88°C
-90°C-90°C
-93°C-93°C
-4°C-4°C
Results (2007/2008)Results (2007/2008)
Z=112
114Exp(2007/2008)
B. Eichler 2003R. Eichler et al. 2002V.Pershina et al 2008
Prediction and exp. result Prediction and exp. result Dubna 2007/2008Dubna 2007/2008
Strong stabilization of elemental 6d107s27p1/22 atomic state!
How to interpret low adsorption How to interpret low adsorption enthalpy of E114?enthalpy of E114?
Unexpected observation: E114 significantly different to Pb and even more volatile than E112.
Calculated van der Waals energies Calculated van der Waals energies using covalent radiiusing covalent radii11, polarizabilities, polarizabilities2 2
and ionisation potentialsand ionisation potentials22
1P.Pyykkö, M. Atsumi, Chem.Eur. J., 2009, 15, 186
2 E=114: C. Thierfelder, B. Assadollahzadeh, P. Schwerdtfeger,
S. Schäfer, R. Schäfer, Phys. Rev. A 78, 052506 (2008) E=112: V.Pershina, A. Borschevsky, E. Eliav, U. Kaldor, J. Chem. Phys. 128, 024707 (2008)
E112 on Au: -30 kJ/Mol; exp.: -52 kJ/MolE114 on Au: -23 kJ/Mol; exp.: -34 kJ/Mol
(Rn on Au: - 24 kJ/Mol; exp.: -27 kJ/Mol)
Courtesy: R. Eichler
ConclusionConclusion
- On-line gas phase chemistry has reached the sensitivity of about 1 pb
- Month-long beam times at highest possible beam intensities mandatory for chemical studies
- Single atom chemistry yields reliable chemical information
- Elements 112 and 114 surprisingly volatile
- Next: element 113 (eka-Tl). Expected volatility of At.
- Far future: chemistry from actually s-range to ms-range? (e.g. Stern-Gerlach experiment for atomic electronic configuration) [Proposal E.K. Hulet]
Acknowledgement Acknowledgement - Excerpt for Z=112/114 studies -- Excerpt for Z=112/114 studies -
PSI team: R. Eichler et al.
FLNR chemistry: S. Dmitriev, S. Shishkin
FLNR GNS team: V.K. Utyonkov et al.
FLNR VASSILISSA team: A.V. Yeremin et al.
FLNR support: Yu. Ts. Oganessian
LLNR target: K.J.Moody et al.
E112calc
-52-52+4+4-3-3 kJ/mol kJ/mol
Adsorption of E112 on AuAdsorption of E112 on Au
Eichler, R. et al. Nature 487, 72 (2007)
Result can be used to improve the prediction models
B. Eichler 1985B. Eichler 2003V. Pershina et al. 2005/08R. Eichler et al. 2002R. Eichler et al. 2002