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The Millimeter- and Submillimeter-Wave Spectrum of Propenal A. M. DALY, C. BERMÚDEZ, L. KOLESNIKOVÁ, AND J. L. ALONSO Grupo de Espectroscopia Molecular.

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Presentation on theme: "The Millimeter- and Submillimeter-Wave Spectrum of Propenal A. M. DALY, C. BERMÚDEZ, L. KOLESNIKOVÁ, AND J. L. ALONSO Grupo de Espectroscopia Molecular."— Presentation transcript:

1 The Millimeter- and Submillimeter-Wave Spectrum of Propenal A. M. DALY, C. BERMÚDEZ, L. KOLESNIKOVÁ, AND J. L. ALONSO Grupo de Espectroscopia Molecular Laboratorios de Espectroscopia y Bioespectroscopia Edificio Quifima. Parque Científico Universidad de Valladolid SPAIN ISMS 2014

2 Propenal Acrolein trans cis 0 cm -1 600 cm -1 Simplest conjugated adlehyde Sugar descomposition Amino acid formation MethionineGlutamic acid ISMS 2014

3 Is propenal in the ISM? Propanal [4] 6 lines 2 lines Propinal [4] 1 line Sagitarius B2 Green Bank 18-26 GHz ISMS 2014 Propenal [4] [1] Sagdeev R.Z. et al. Nature 1986; [2] Matthews H.E. et al. ApJ 1985; [3]Hollis J.M.et al. ApJ 2000; [4]Hollis J.M. et al. ApJ 2004 Glycoaldehyde [3] Acetaldehyde [2] Formaldehyde [1]

4 Detection of propenal Propenal 2 lines 2 1 1 – 1 1 0 3 1 3 – 2 1 2 Sagitarius B2 Green Bank 18-26 GHz 26079.449(1) MHz 18221.164(2) MHz ISMS 2014 No more lines belonging to propenal have been detected in the ISM [4]Hollis J.M. et al. ApJ 2004

5 1955 [5] 1957 [6] 1966 [7] 1975 [8] 1982 [9] 1984 [10] ISMS 2014 Previous spectroscopy data trans cis 0 cm -1 600 cm -1 μ a = 3.06(4)D [6] μ b = 0.54(14)D μ a = 2.010(5)D [9] μ b = 1.573(3)D Rotational spectroscopy 36 GHz, t gs, t ν 18 36 GHz, t gs, t ν 18, t 2ν 18, t 3ν 18 27 GHz, t gs, t 1-9ν 18, isotopologes 13 C, 18 O, D 50 GHz, c gs, c ν 18 180 GHz, t gs Year 50 GHz, c gs, c ν 18 isotopologes 13 C, 18 O, D GHz measured [5] Fine et al. JChemPhys. 1955; [6] Wagner R. et al. JChemPhys 1957; [7] Cherniak E.A. et al. JChemPhys 1966; [8] Winniwisser M. et al. Z. Naturforsch. 1975; [9] Bolm et al. ChemPhysL 1982; [10] Blom et al. JACS 1984

6 Previous spectroscopy data trans cis 0 cm -1 600 cm -1 μ a = 3.06(4)D [6] μ b = 0.54(14)D μ a = 2.010(5)D [9] μ b = 1.573(3)D ISMS 2014 High resolution Far-IR Spectroscopy [11] t ν 18 t ν 13 t ν 13 + t ν 18 t 3ν 18 t ν 12 t ν 17 t 4ν 18 t ν 13 + t 2ν 18 t 2ν 13 t gs t 2ν 18 [11] McKellar A.R.W. et al. JMolSpectrosc. 2008.

7 Our goals ISMS 2014 Improving propenal rotational parameters Facilitate the detection of more transitions belonging to propenal ALMA project

8 Our goals ISMS 2014 Improving propenal rotational parameters trans cis 0 cm -1 600 cm -1 Analyze the rotational spectrum of higher energy vibrational excited states Extent the measurements of the vibrational excited states t gs and t ν 18 Measurements at higher frequency range of the t gs isotopologues at natural abundance Analyze the rotational parameters of c gs at higher frequency ranges

9 Vibrational excited state energies ISMS 2014 Interactions C-type Coriolis and Fermi trans

10 Stark spectrometer frequency range has been extended up to ~110 GHz Stark modulation spectroscopy ISMS 2014

11 Stark modulation spectroscopy Trans-propenal t ν 18 t ν 13 t ν 18 + t ν 13 t 3ν 18 t ν 12 t ν 17 t ν 13 + t 2ν 18 t 2ν 13 t gs t 2ν 18 t 4ν 18 4 1 4 – 3 1 3 t ν 13 t ν 12 t ν 17 t 2ν 13

12 MMW and sub-MMW spectrum MMW and sub-MMW spectrometer (50 – 1000 GHz) AM chains Synthesizer 50-110 GHz, 135 – 480 GHz, 500 – 700 GHz room temperature 15 mTorr Lock-in amplifier Sample cells Detector ISMS 2014 RJ05 Lucie Kolesniková Medical Science Building 2:28pm

13 t 3ν 18 ISMS 2014 MMW and sub-MMW spectrum t ν 13 t 2ν 18 t ν 13 + t ν 18 t gs t ν 18 Δν (MHz)

14 ISMS 2014 MMW and sub-MMW spectrum t ν 18 t gs t 2ν 18 t ν 13 t ν 13 + t ν 18 t 3ν 18

15 Interactions ISMS 2014 G c /MHz-365.03(44 ) G c J /MHz0.00273(45 ) G c K /MHz-0.2957(74 ) F ab /MHz-4.676(73 ) W/MHz82914.88(73 ) W +- /MHz0.09921(46 ) W +- J /MHz-4.77(188) ·10 -6 W +- K /MHz2.345(69) ·10 -3 W J /MHz-0.3067(208) W JK /MHz-2.655(50 ) ·10 -3 W KK /MHz0.5124(97 ) W/MHz134543.7(102) W +- /MHz0.2125(59 ) W +- J /MHz-0.143(46 ) ·10 -6 W J /MHz-0.5387(59 ) W JK /MHz-2.964(177) ·10 -3 W KK /MHz-41.45(138) F ab /MHz2.5449(50 ) G c /MHz556.928(90 ) G c /MHz-0.00099(83 ) G b /MHz-0.00657(42 ) G b /MHz0.03454(65 ) G b K /MHz-0.000135(204)

16 E/MHz[157.1704856][314.221907][323.0193961][468.94762][482.826622] A/MHz47353.68940(245)45782.7002(100)44391.655(141)48738.976(140)43110.34(97)46941.35(89) B/MHz4659.499457(87)4666.24203(33)4673.03078(136)4659.19801(138)4679.7384(80)4665.1109(78) C/MHz4242.689474(78)4259.627077(290)4276.62788(181)4238.34635(179)4293.4019(96)4255.9631(93) Δ J /kHz1.0420990(300)1.086567(95)1.132468(159)1.027465(157)1.19007(40)1.06501(34) Δ JK /kHz -8.78184(86)-8.53124(133)-8.2104(98)-10.3003(91)-7.681(42)-10.284(42) Δ K /kHz 358.149(149)-79.96(40)-331.2(49)828.1(78)-255.9(162)74.8(95) δ J /kHz0.1202562(102)0.118495(62)0.116641(136)0.118088(134)0.116358(203)0.112165(260) δ K /kHz5.7747(36)-0.6888(275)-6.237(62)11.559(65)-6.536(131)3.053(84) Φ J /mHz0.3142(39)0.5668(141)0.3803(120)0.4040(124)0.5938(161)0.3101(191) Φ JK /mHz8.62(164)128.9(59)-251(149)-39.1(171)-88.7(178)835.5(178) Φ KJ /mHz-507.4(62)460.5(193)2293(64)-1107(67)3002(109)-2120(107) Φ K /Hz-75.5(35)-555.8(60)[-75.5]348.1(153)4194(227)5030(261) φ J /mHz0.07667(159)0.1066(78)-0.017(225)0.0653(249)0.2119(225)0.193(32) φ JK /mHz8.78(85)44.7(49)[8.78] φ K /Hz1.977(222)16.56(79)-33.77(207)-2.45(248)4.37(272)133.9(315) L JJK / μ Hz 0.0532(244)-0.468(35) L JK / μ Hz -46.40(173)-162.81(160) L K /mHz828(32)2707.8(264) Fitting ISMS 2014 t ν 18 t gs t 2ν 18 t ν 13 t ν 13 + t ν 18 t 3ν 18 NσNσ 8571,213 98kHz

17 Alone6 states fitRef [8]Ref [11] A/MHz 47353.7105(14)45782.7002(100) 47353.7106(44) 45783.0348(87) B/MHz 4659.499489(51)4666.24203(33) 4659.49924(19) 4666.24289(96) C/MHz 4242.689471(46)4259.627077(290) 4242.68964(19) 4259.6272(10) Δ J /kHz 1.042053(16)1.086567(95) 1.04153(33) 1.086028(93) Δ JK /kHz -8.78484(6)-8.53124(133) -8.78252(28) -8.5460(50) Δ K /kHz 360.421(38)-79.96(40) 359.91(46) -65.72(21) δ J /kHz 0.1202785(66)0.118495(62) 0.119849(84) 0.11831(67) δ K /kHz 5.7400(22)-0.6888(275) 5.7986(22) -0.851(21) Φ J /mHz 0.2960(21)0.5668(141)... Φ JK /mHz -6.489(39)128.9(59) -12.3(53) Φ KJ /mHz -509.6(10)460.5(193) -475.6(93) Φ K /Hz...-555.8(60) φ J /mHz 0.07535(96)0.1066(78) φ JK /mHz 3.43(54)44.7(49) φ K /Hz 16.56(79) L JJK / μ Hz -0.468(35) L JK / μ Hz -162.81(160) L K /mHz 2707.8(264) Ground state trans ISMS 2014 [8] Winniwisser M. et al. Z. Naturforsch. 1975; [11] McKellar A.R.W. et al. JMolSpectrosc. 2008

18 13 C isotopologues ISMS 2014

19 Cis isomer ISMS 2014

20 Rotational parameters ISMS 2014 t gsTrans 13 C 1 Trans 13 C 2 Trans 13 C 3 c gs A/MHz 47353.7105(14) a 47254.920(93)46518.557(92)46781.158(97)22831.6481(43) B/MHz 4659.499489(51) 4520.79373(27) 4642.43806(33) 4644.74078(37) 6241.04754(35) C/MHz 4242.689471(46) 4126.64224(32) 4221.74680(32) 4225.83687(37) 4902.20752(21) Δ J /kHz 1.042053(16) 0.988653(90) 1.03242(13) 1.03950(14) 5.11348(24) Δ JK /kHz -8.78484(38) -8.9420(15) -8.7379(15) -8.6746(34) -29.1849(12) Δ K /kHz 360.421(53) 366.31(52) 320.7(10) 312.46(36) 108.03(12) δ J /kHz 0.1202785(66) 0.111299(30) 0.121082(25) 0.120490(39) 1.48125(12) δ K /kHz 5.7400(22) 5.534(19) 5.556(13) 5.404(23) 11.3388(74) ΦJ/mHz 0.2960(21) 0.228(15) 0.399(22) 0.171(26) 1.649(89) ΦKJ/mHz -509.6(10) -399.7(80)-525.9(73) -413.(27)-1152.7(21) ΦJK/mHz -6.489(39)[0.] 92.30(47) φJ/mHz 0.07535(96)[0.] 1.111(43) φJK/mHz 3.43(54)[0.] -18.6(20) N lines c 1152,13401,10446,10419,10573,13 σ fit c /kHz 29,942,244,542,138,7 3 2 1

21 ISMS 2014 Summary The spectrum of propenal has been measured up to 700GHz Rotational parameters of the vibrational excited states below 600cm -1 has been obtained The analysis of c gs t gs and its isotopologues has been updated up to 700MHz Now it is time for you to find more lines of propenal in the interestllar medium

22 Acknowledgments Grants CTQ 2010- 19008 BES 2011-047685 CSD 2009-00038 Molecular Astrophysics Grants VA070A08 and CIP13/01 Grupo de Espectroscopia Molecular (GEM) Laboratorios de Espectroscopia y Bioespectroscopia, Unidad Asociada CSIC, UVa,Valladolid, Spain


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