Jonathan Tennyson Molecular Line Lists for Exoplanets and Other ...

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Intensity / [cm/mole] Absorption spectra of 14 NH 3 : Temperature effect 1000000 100000 10000 1000 100 10 1 0.1 I( f ← i) = S( f ← i) −Ei / kT e Q( T) [ 1− e −hc ~ ν / kT 0.01 1 2 3 4 5 6 7 8 9 10 wave length / µm if 3 8π N ~ Aν if ] ( 4πε ) 3hc 0 1500K 1200K 900K 600K 300K
Ab initio calculations DMS PES Rovibrational wavefunctions Intensities (Einstein A if ) Method: Spectrum from the “first-principles” Variational calculations Rovibrational energies <strong>Line</strong> list Refinement
Page 2: Cool atmospheres: dominated by mole
Page 5 and 6: 2012: (nearly) every star has plane
Page 7 and 8: HD189733b: Primary transit with Spi
Page 9 and 10: Pont et al., 2007 Swain et al., 200
Page 11 and 12: Exoplanet Characterisation Observat
Page 13 and 14: Why theory, not experiment?
Page 15 and 16: Absorption (T=300K) spectrum of NH
Page 17 and 18: Absorption (T=300K) spectrum of NH
Page 19: Completeness: Absorption of ammonia
Page 23 and 24: Line list (in progress): C 2 Potent
Page 25 and 26: Potential energy Ab initio: solve f
Page 27 and 28: CH 4 : Matrix diagonalization (Symm
Page 29 and 30: C s C 2v C 3v D 3h C 2h … … Str
Page 31 and 32: Absorption of Methane (T=300 K) Int
Page 34 and 35: Energy file: N J sym n E/cm -1 v 1
Page 36 and 37: Obs: A. Coppalle & P. Vervisch, JQS
Page 38 and 39: Cross sections for NH 3 ν 2 band a
Page 40 and 41: As well as..... Remote detection of

Jonathan Tennyson Molecular Line Lists for Exoplanets and Other ...

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