Hypermetallic molecules

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1 1 Hypermetallic molecules (Picture courtesy of Python M)

2 2 An ab initio study of the alkaline earth oxides BeOBe, MgOMg, CaOCa, SrOSr, BaOBa, and RaORa. Bojana Ostojić (Belgrade), Per Jensen (Wuppertal), Peter Schwerdtfeger (Massey University, New Zealand), Phil Bunker (NRC, Ottawa). Hypermetallic since they have one more metal atom than they should

3 3 PERIODIC TABLE OF ELEMENTS [He]2s 2 [Ne]3s 2 [Ar]4s 2 Chemistry 1.0.1: M 2+ O 2- is formed! Why bonding to another M? [Rn]7s 2 MOM?

4 4 PERIODIC TABLE OF ELEMENTS [He]2s 2 [Ne]3s 2 Chemistry 1.0.1: M 2+ O 2- is formed! Why bonding to another M? [Ar]4s 2 Chemistry 1.0.2: Because MO is closer to M + O - [Rn]7s 2 MOM OK!

5 5 Apart from BeOBe, little known experimentally. Our interest in these molecules is three-fold: To make precise ab initio calculations on them in order to understand the electronic structure, To predict the IR and electronic spectra and to compare with the experimental spectra, To calculate Singlet-Triplet splittings and S-T interaction strengths in order to test these molecules as candidates for high precision spectral measurements aimed at looking for a time-variation in M p /m e and fine structure constant.

6 6 The ab initio slide Please direct questions to Molecule Method Basis set BeOBe CASSCF MRCI cc-pcvqz MgOMg FV-CASSCF MRCISD cc-pcvqz CaOCa FV-CASSCF MRCISD+RS2C cc-pwcvqz-dk SrOSr CASSCF MRCISD+RS2C Sadlej pvtz and Stuttgart relativistic small-core effective core potential for Sr BaOBa and RaORa CASSCF MRCI cc-pcvqz and Stuttgart small-core relativistic effective core potential ECP46MDF and ECP78MDF for Ba and Ra Nuclear-motion calculations and spectral simulations with MORBID

7 7 BeOBe, MgOMg, CaOCa, SrOSr, BaOBa, and RaORa. We find that all these MOM molecules have 1 + A linear Σg ground electronic state and a fairly low lying 3 + linear Σu first excited electronic state. S-T spin-orbit coupling too small for them to be good candidates for use in measuring the time dependence of the fundamental parameters.

8 8 BeOBe bending potential curves

9 9 BeOBe exp Experiment: Merritt, Bondybey and Heaven, JPC A113, (2009)

10 10 BeOBe Singlet spectrum Triplet spectrum At 300 K. All bands very weak

11 11 MgOMg ~ T e (a) = 671 cm -1 Diatomic 24 Mg 16 O cm -1

12 12 MgOMg 420 nm 3.7 D 310 nm 4.0 D 360 nm 4.1 D 340 nm 2.9 D

13 13 MgOMg From Discussion:

14 14 MgOMg A 1 + Σ u E 1 Π u X X 420 nm 310 nm b 3 Π g c 3 Π g a a 360 nm 340 nm

15 15 CaOCa Also think that spectrum shows linear CaCaO molecule

16 16 CaCaO (linear) Ca Ca O bent 40 Ca+ 16 O 3 44 Ca+ 16 O 3 CaO O , , Ca 16 O υ = cm -1 in gas phase υ = 707 cm -1 in N 2 matrix. 44 Ca+55% 18 O , 461 Our results for CaOCa in the X 1 + Σ g state: 44 Ca+55% 18 O 2 In solid N 2 at 17 K 720 υ 1 υ 2 υ

17 17 SrOSr singlettriplet interaction S-T interaction? ΔE ~ 2 cm -1 What is S-T matrix element? even J/odd J even N/odd N

18 18 SrOSr ST matrix element = = 0.01 cm -1 a ~ 0 0 ~ X 7 1 ΔE ~ 2 cm -1 Thus energy shift ~ (0.01) 2 /2 cm -1 = cm -1

19 19 MOM equilibrium bond length S-T splitting

20 20 BaOBa bending potential energy curves Ba 0.5+ O - Ba nm 910 nm Predicted emission wavelengths

21 21 BaOBa Gee et al. The cluster isolated chemical reaction technique. West and Poland JCP 66, 2139 (1977) Triplet Emission ~700 nm Singlet Emission ~900 nm

22 22 Spring has arrived in Wuppertal! Thank you for your attention!

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