optical zeeman spectroscopy of the (0,0) bands of the b 3 -x 3 and a 3 -x 3 transitions of...
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Optical Zeeman Spectroscopy of the (0,0) bands of the B3-X3 and A3-X3 Transitions of Titanium Monoxide, TiO
Wilton L. Virgo, Prof. Timothy C. Steimle and Prof. John M. Brown
Ap. J. 628, 2005 July 20
Zeeman Spectroscopy of TiO: Dual Purpose
• Magnetic “g” factors are useful in unraveling the nature of electronic states of metal containing molecules.– Analyze electronic state composition and
provide evidence for mixing between states.
• Optical Zeeman effect of TiO is used to probe ambient stellar magnetic fields. – Experimentally determine magnetic tuning
rates of molecular energy levels.
TiO Stokes V Spectrum of SunspotS.V. Berdyugina et. al. A&A 364, L101 2000
3000G
Calc. Stokes V Profile of (0,0) R3(10) line with magnetic field strengths .5-3.5kG
TiO (0,0) R3 band head in a sunspot
Dashed: ObservedSolid: Calculated
Origin of the Stokes V Spectrum
Profiles calculated for low-J lines of Q branch in ’(B3-X3)
Zeeman Effect in Diatomic Molecules:Berdyugina’s Astrophysical Model
mL = -BgLL, mS = -BgSS
Magnetic dipole moment operator is a sum of terms directly proportional to angular momentum operators:
In principle, Zeeman effect can be predicted a priori from field freeeigenvalues and eigenvectors given the g-values:
J JJ MnΛ S nΛ S J M m B
J ( / ( 1)B L SBM g g J J
1. Only diagonal terms in J included2. Predicts linear field dependence3. gS, gL fixed to 2.002 and 1.04. and are rigorously good
Berdyugina et. al. A&A 412, 513 (2003), A&A 385, 701 (2002).
Modeling the Zeeman Effect in TiO:Sophisticated Effective Hamiltonian Approach
1. Spin-orbit and rotational mixing significant in metal species2. Evident in large -doubling in B3 state of TiO
2 2
( .) g L g S
g μ S B S B g S B S B
L B z S B z
i il B x x y y l B
eff
e e
ZeeH
Key difference from astrophysical model:Accounts for both linear and non-linear field dependence byincluding off diagonal in J matrix elements
Eff. Hamiltonian absorbs effects of other states into the g parametersMakes allowance for all possible admixtures of electronic statesAdjustable g parameter values glean insight into the perturbations
Laser Ablation and Molecular Beam Production
Free JetExpansion
High-Resolution Spectrometer
Electromagnet
Optical Zeeman Spectroscopy
Electromagnet for Zeeman Spectroscopy (56G-1.2kG)
Electronic Transitions of TiOW
avenum
ber (c
m) x
10
-1-3
X3
B3
A3
E312.0
0.0
14.0
16.0
(D3
-band= 101ns
band= 4900 ns
C3
18.0
20.0
Zeeman Spectra: R11(1) (A32-X31)
Zeeman Spectra: Q11b(1) (0,0) ’(B30 - X31) Feature
‘Stick’ Spectra of Q11b(J) ’(B 30 - X31) Branch
A) Berdyugina model with only diagonal (in J) matrix elements and fixed g-factorsB) Steimle model w/off diagonal J=+/-1 matrix elements and determined g-factors
Results: Zeeman Fitting Parameters
State Fit A Fit BgL gL gl
A3 0.994(2) 0.994(2)B3 1.037(8) 1.035(8) -0.02(4)a
Std. dev. 18.9MHz 18.9MHza Consistent w/value predicted by Curl’s relationship:gl = -/2B = -.02
Conclusion #1: Chemistry
• gL values indicate that C3 is reasonable candidate for state that interacts strongly with both A3 and B3.
• C~A and C~B satisfy rules for S.O. mixing– C3 state differs by one spin-orbital from A3
and B3 states• A3,B3: 82341141
• C3: 823411101
– C3 state differs from A3 and B3 states by one unit of orbital angular momentum.
Conclusion #2: Astrophysics
• Significant -doubling in B30 state requires inclusion of J=+/-1 matrix elements.
• Strong off-diagonal J interaction will impose a non-linear response to magnetic field in the low-J lines. Fitted g-factors necessary to reproduce experimental observations. Unexpected by current astrophysical model.
Thank YouFunding provided by NSF Experimental Physical Chemistry