The Stark shift of a diatomic molecule

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Making cold molecules from cold atoms

description

The Stark shift of a diatomic molecule. Contributions to the Stark shift. Hamiltonian for the Stark interaction:. Energy shift by perturbation theory, to second order. Zero. Small, when i and j differ only by rotation. - PowerPoint PPT Presentation

Transcript of The Stark shift of a diatomic molecule

Page 1: The Stark shift of a diatomic molecule

Making cold molecules from cold atoms

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PhotoassociationA B h PA AB

PA

Ground state A + B

(AB)*

Photoassociation is resonant in the photon energy Usually achieved by adding an extra laser to a MOT – the PA laser Very little heating involved – the molecules are ultracold Molecules will be in low-lying rotational states Produces molecules in highly excited vibrational states

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Photoassociation – decay channels

A B h sp AB h sp

ABDecay to free atoms Decay to bound state

PA

Ground state A + B

(AB)*

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Photoassociation properties

Most efficient for high-lying vibrational states – tend to form “long-range molecules” Extremely inefficient for tightly bound states Decay to a deeply bound state of the molecular ground state is unlikely Decay to two free atoms is accompanied by a large release of energy – trap loss

Li2, Na2, K2, Rb2, Cs2, Sr2 , Ca2 , LiCs, KRb, RbCs….

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Detection methods

PRL 85, 2292 (2000)

Trap loss spectroscopy – the number of atoms in a MOT decreases when the molecules are formed. Example below: Ca2

Rev. Mod. Phys. 78, 483 (2006)

Ion detection. Ionize the molecules and count the ions produced.

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Example: production of ultracold LiCs in the ground state

PRL 101, 103004 (2008)

(a) Photoassociation into v=4 (500mW, 946nm)(b) Spontaneous decay into ground state(c) Two-photon resonant ionization5000 ground state molecules per second

v=4

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Photoassociation - advantages and limitations

X Limited to constituents that can be laser-cooled

X Production rate is usually very slow resulting in low phase-space densities

Molecules are formed at ultracold temperatures

Possible to reach the ground state (though difficult)

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Magnetoassociation through a Feshbach resonance

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Uppermost bound state Zero-energy scattering state

Reminder about s-wave scattering At ultracold temperatures, scattering is described by the s-wave scattering length, a All other partial waves are suppressed by the angular momentum barrier

u(R) (R – a)

Eupper 2

2 a2 u(R) exp(-R/a)

Toy example:

V=∞

V=V0

V=0

4 a2

1 k2 a2

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Feshbach resonance

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Reminder about level crossings 0 0

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B / B0

Free atomsBound molecules

Atoms into molecules via a Feshbach resonance