Modeling gas-surface processes. Theory and Experiments for adsorption energies determination of nitrile / isonitrile isomers.

Size: px
Start display at page:

Download "Modeling gas-surface processes. Theory and Experiments for adsorption energies determination of nitrile / isonitrile isomers."

Transcription

1 Modeling gas-surface processes Theory and Experiments for adsorption energies determination of nitrile / isonitrile isomers. Y. Ellinger, A. Markovits, F. Pauzat, M. Doronin (Laboratoire de Chimie Théorique - LCT) M. Bertin, M. Doronin, J.-H. Fillion (Observatoire de Paris LERMA) M16 by NASA

2 Nitriles and Isonitriles Molecules in the ISM (as of 02/2016) Almost 20% of the ~ 200 organics detected have a CN triple bond. 37 species split in 30 R-CN 7 R-NC If R is saturated the list is reduced to CH 3 CN (Solomon et al 1971) CH 3 CH 2 CN (Johnson et al 1977) n-c 3 H 7 CN and i-c 3 H 7 CN (Belloche et al 2009; 2014) CH 3 NC (Cernicharo et al 1988)

3 Abundance ratios as constraints to chemical models HCN/HNC (the most studied) Variations from ~1 in cold molecular clouds to ~n x 1000 in PDRs CH 3 CN/CH 3 NC Variations negligibles ~50 in all situations Why?

4 Possible reasons Observational bias: Radio observations are blind to molecules depleted on the grains Observational fact: The abundance ratios are different for the gas phase and for the depleted species (Dipole moment: µ ~ 4 D for CH 3 CN/CH 3 NC) Possible origin: Selective adsorption between isomers

5 Interstellar surfaces Original work by Greenberg (1976) Silicates: Molster et al (2002) Water ices: Schutte (1999); Gigg et al (2004) Watanabe & Kouchi (2008); Boogert et al (2015) Carbonaceous matter: Leger & Puget (1984); Allamandola et al (1985); Papoular et al (1995) Experiments TPD: Temperature Programmed Desorption Numerical simulations First principle periodic DFT calculations M. Lattelais, M. Bertin, et al. A&A, 532, A12 (2011) M. Bertin, M. Doronin, et al; A&A, 598, A18 (2017) M. Bertin, M. Doronin, et al; A&A, in press (2017)

6 TPD: Temperature Programmed Desorption (ices) Mass spectrometer RAIRS RAIRS H 2 O ice Polycrystalline Au T = 80 K T 1 K.min - 1 Adsorption/desorption behaviours of each isomer Estimation of adsorption energy in the single molecule limit Measure of the ability to bind with water surface via hydrogen bonding

7 Experimental check è adsorption (ices) Vola%les : Below 100 K (H 2, CO, CH 4, CO 2 ) E Ads ~ 0.1 ev Weakly bound : Before H 2 O (HCOOCH 3, CH 3 OCH3...) E Ads ~ 0.3 ev Strongly bound : With H 2 O (CH 3 COOH, CH 3 CH 2 OH...). Adapted from M. Lattelais, M. Bertin, et al. A&A, 532, A12 (2011) E Ads ~ 0.6 ev

8 Numerical simulation è adsorption (ices) E (kcal/mol) HOCH 2 CHO 27 [CH 3 COOH] [HCOOCH 3 ] 17 0 HCOOCH 3 CH 3 COOH = 0,01 à 0,1 [CH 3 COOH] [HOCH 2 CHO] = 0,05 E CH3COOH = 17,2 kcal/mol E HOCH2CHO = 11,6 kcal/mol E HCOOCH3 = 7,3 kcal/mol. M. Lattelais, M. Bertin, et al. A&A, 532, A12 (2011)

9 Theoretical approaches for weak interactions with systems of large dimensions Ab initio / DFT molecule molecule ρ 1 ρ molecule support support ρ 2 support «supermolecule» approach: è BSSE artifact Tran et al. J. Phys. Chem. B (2002); Heine et al. PCCP (2004) KSCED approach Tran et al. J. Phys. Chem. B (2002) Periodic approach: plane waves

10 Adsorption on graphite Position of R-CN Orientation of RCN L: middle of a bond X X: to plane C: carbon atom O: center of the ring L O C Z Y Y: to plane Z: to plane

11 Periodic approach Vertical replication Vertical replication vacuum

12 Adsorption on graphene: vertical dimension of the cell vertical Dimension (Ǻ) ΔE (kcal/mol) Test of the adsorption energy of a dipolar system: HCN

13 Nitrile versus Isonitrile on perfect graphite CH 3 CN CH 3 NC E ads (Th) E ads (Exp) = 275 mev (30 mev) 440 ± 25 mev E ads (Th) E ads (Exp) = 255 mev (30 mev) 430 ± 25 mev No significant difference between nitrile and isonitrile on perfect HOPG M. Bertin, M. Doronin, et al; A&A, in press (2017)

14 Nitrile versus Isonitrile on damaged graphite CH 3 CN CH 3 NC E ads (Th) E ads (Exp) = 310 mev (40 mev) 440 ± 25 mev E ads (Th) E ads (Exp) = 300 mev (40 mev) 430 ± 25 mev No significant difference between nitrile and isonitrile on HOPG with 2C hole defect M. Bertin, M. Doronin, et al; A&A, in press (2017)

15 Nitrile versus Isonitrile on damaged graphite CH 3 CN CH 3 NC E ads (Th) E ads (Exp) = 390 mev (50 mev) 440 ± 25 mev E ads (Th) E ads (Exp) = 350 mev (50 mev) 430 ± 15 mev No significant difference between nitrile and isonitrile on HOPG with 2C hole hydrogenated defect M. Bertin, M. Doronin, et al; A&A, in press (2017)

16 Nitrile versus Isonitrile on damaged graphite CH3CN Eads (Th) = 480 mev (0 mev) Eads (Exp) 440 ± 25 mev CH3NC Eads (Th) = 440 mev (0 mev) Eads (Exp) 430 ± 25 mev No significant difference between nitrile and isonitrile on HOPG with hydrogenated step defect M. Bertin, M. Doronin, et al; A&A, in press (2017)

17 Nitrile versus Isonitrile on water ice CH 3 CN CH 3 NC E ads (The) E ads (Exp) = 558 mev 565 ± 25 mev E ads (The) E ads (Exp) = 545 mev 540 ± 15 mev No significant difference between nitrile and isonitrile Similar results on silicates M. Bertin, M. Doronin, et al; A&A, 598, A18 (2017)

18 What to conclude Theory Eads (mev) Perfect HOPG C hole CH hole q No significant difference between nitrile and isonitrile whatever substract and defects (within ~10%) q Systemetic shift of E ads towards lower values for CH 3 NC q CH 3 CN/CH 3 NC not affected by environment TPD Eads (mev) CH3CN CH3NC CH3CN CH3NC Step-H ± ± 25 α-quartz (0001) ± ± 25 Water ice (Ih) ± ± 15

19 The End

20 Adsorption of COMs and simulations Bertin, M., Doronin, M., Fillion, F.-H., Michaut, X.,Philippe, L., Lattelais, M., Markovits, A., Pauzat, F.,Ellinger, Y. & Guillemin, J.-C. 2017, A&A, 598, A18 and 2017, A&A, Part II in press Doronin, M., Bertin, M., Michaut, X., Philippe, P., &Fillion, J.-H. 2015, J. Chem. Phys., 143, Lattelais, M., Pauzat, F., Ellinger, Y., & Ceccarelli, C. 2015, A&A, 578, A62 Pauzat, F., Marloie, G., Markovits, A., & Ellinger, Y., 2015, Int.,J. Astro., 14, 563 Lattelais, M., Bertin, M., Mokrane, H., et al. 2011, A&A, 532, A12 Pauzat, F., Lattelais, M., Ellinger, Y., & Minot, C. 2011, MNRAS, 412, 2729

UV photodesorption of intact molecules and of photofragments from solid formaledhyde and methanol

UV photodesorption of intact molecules and of photofragments from solid formaledhyde and methanol UV photodesorption of intact molecules and of photofragments from solid formaledhyde and methanol Mathieu Bertin, Xavier Michaut, Claire Romanzin, Géraldine Féraud, Pascal Jeseck, Laurent Philippe, Harold

More information

arxiv: v1 [astro-ph.ga] 17 Oct 2016

arxiv: v1 [astro-ph.ga] 17 Oct 2016 Astronomy & Astrophysics manuscript no. 29394 langugage edited 2col c ESO 2016 October 18, 2016 arxiv:1610.05010v1 [astro-ph.ga] 17 Oct 2016 Nitrile versus isonitrile adsorption at interstellar grains

More information

Non-thermal ion desorption from nitrilebearing astrophysical ice analogues studied by electron and heavy ion bombardment

Non-thermal ion desorption from nitrilebearing astrophysical ice analogues studied by electron and heavy ion bombardment Non-thermal ion desorption from nitrilebearing astrophysical ice analogues studied by electron and heavy ion bombardment Fabio Ribeiro, Guilherme C. Almeida, Wania Wolff, Enio Frota da Silveira, Maria

More information

Hydrogenation of solid hydrogen cyanide HCN and methanimine CH 2 NH at low temperature

Hydrogenation of solid hydrogen cyanide HCN and methanimine CH 2 NH at low temperature Hydrogenation of solid hydrogen cyanide HCN and methanimine CH 2 NH at low temperature P. Theule, F. Borget, F. Mispelaer, G. Danger, F. Duvernay, J. C. Guillemin, and T. Chiavassa 5 534,A64 (2011) By

More information

TERAHERTZ SPECTROSCOPY OF DEUTERATED ACETALDEHYDE: CH 2 DCHO

TERAHERTZ SPECTROSCOPY OF DEUTERATED ACETALDEHYDE: CH 2 DCHO TERAHERTZ SPECTROSCOPY OF DEUTERATED ACETALDEHYDE: CH 2 DCHO L. Margulès, R. A. Motiyenko Laboratoire PhLAM, Université de Lille1, France L. H. Coudert LISA, CNRS, Universités Paris Est Créteil et Paris

More information

Université de Cergy-Pontoise, FRANCE

Université de Cergy-Pontoise, FRANCE Water formation through O 2 +D pathway on cold silicate, graphite and amorphous water surfaces of interstellar interest Henda Chaabouni Marco Minissale, François Dulieu LERMA-LAMAp, UMR 82 du CNRS, Observatoire

More information

Chemical modelling of formamide and methyl isocyanate in star-forming regions

Chemical modelling of formamide and methyl isocyanate in star-forming regions Chemical modelling of formamide and methyl isocyanate in star-forming regions David Quénard Post-Doctoral Research Assistant Izaskun Jiménez-Serra (QMUL), Serena Viti (UCL), Jon Holdship (UCL), Audrey

More information

2- The chemistry in the. The formation of water : gas phase and grain surface formation. The present models. Observations of molecules in the ISM.

2- The chemistry in the. The formation of water : gas phase and grain surface formation. The present models. Observations of molecules in the ISM. 2- The chemistry in the ISM. The formation of water : gas phase and grain surface formation. The present models. Observations of molecules in the ISM. 1 Why studying the ISM chemistry? 1- The thermal balance,

More information

The rôle of surfaces in prebiotic chemistry. Piero Ugliengo University of Torino Dip. Chimica Via P. Giuria, 7 - Torino

The rôle of surfaces in prebiotic chemistry. Piero Ugliengo University of Torino Dip. Chimica Via P. Giuria, 7 - Torino The rôle of surfaces in prebiotic chemistry Piero Ugliengo University of Torino Dip. Chimica Via P. Giuria, 7 - Torino 1 A collaborative work Dip. Chimica - NIS Centre Torino University TO BCN Dep. Quimica

More information

Surfaces processes. François Dulieu LERMA. Paris Observatory and Cergy Pontoise University

Surfaces processes. François Dulieu LERMA. Paris Observatory and Cergy Pontoise University Surfaces processes François Dulieu LERMA Paris Observatory and Cergy Pontoise University Cold surfaces and astrophysics Image credit: J. Freitag and S. Messenger Smoky areas = dust grains Cold (10-15 K)

More information

Physical Chemistry Chemical Physics

Physical Chemistry Chemical Physics Physical Chemistry Chemical Physics www.rsc.org/pccp Volume 12 Number 23 21 June 2010 Pages 5929 6292 ISSN 1463-9076 COVER ARTICLE Brown et al. Ice in space: surface science investigations of the thermal

More information

ESO in the 2020s: Astrobiology

ESO in the 2020s: Astrobiology ESO in the 2020s: Astrobiology Izaskun Jimenez-Serra (IIF Marie Curie Fellow, ESO) Leonardo Testi (ESO), Paola Caselli (MPE) & Serena Viti (UCL) 1 From the ISM to the Origin of Life Molecular clouds (Pre-stellar

More information

First-principles Studies of Formaldehyde Molecule Adsorption on Graphene Modified with Vacancy, -OH, -CHO and -COOH Group

First-principles Studies of Formaldehyde Molecule Adsorption on Graphene Modified with Vacancy, -OH, -CHO and -COOH Group 2017 Asia-Pacific Engineering and Technology Conference (APETC 2017) ISBN: 978-1-60595-443-1 First-principles Studies of Formaldehyde Molecule Adsorption on Graphene Modified with Vacancy, -OH, -CHO and

More information

Oxygen Chemistry on Dust Grains

Oxygen Chemistry on Dust Grains Oxygen Chemistry on Dust Grains Gianfranco Vidali and Jiao He, Tyler Hopkins, Jianming Shi Syracuse University Syracuse, NY (USA) Jean Louis Lemaire Paris Observatoire, Paris (France) Michael Kaufman San

More information

atoms H. * Infrared **Optical l - linear c-cyclic

atoms H. * Infrared **Optical l - linear c-cyclic 2 3 4 5 6 7 atoms H *,* 2 C 3 * c-c 3 H C 5 * C 5 H C 6 H AlF C 2 H l-c 3 H C 4 H l-h 2 C 4 CH 2 CHCN AlCl C 2 O C 3 N C 4 Si C 2 H 4 CH 3 C 2 H C 2 ** C 2 S C 3 O l-c 3 H 2 CH 3 CN HC 5 N CH CH 2 C 3

More information

CO and N2 differential depletion in prestellar cores: Experimental study of N2 desorption induced by the CO presence on ices

CO and N2 differential depletion in prestellar cores: Experimental study of N2 desorption induced by the CO presence on ices CO and N2 differential depletion in prestellar cores: Experimental study of N2 desorption induced by the CO presence on ices T.Nguyen, S. Baouche, E.Congiu, H.Chaabouni, L.Pagani, and F.Dulieu LERMA Lamap,

More information

Ortho-para transitions of molecular hydrogen in H + + H 2 collisions. Tomás González Lezana

Ortho-para transitions of molecular hydrogen in H + + H 2 collisions. Tomás González Lezana Ortho-para transitions of molecular hydrogen in H + + H 2 collisions Tomás González Lezana Dep. de Física Atómica, Molecular y de Agregados Instituto de Física Fundamental (CSIC) MADRID (ESPAÑA) Grenoble

More information

Density functional theory with an approximate kinetic energy functional applied to study structure and stability of weak van der Waals complexes

Density functional theory with an approximate kinetic energy functional applied to study structure and stability of weak van der Waals complexes JOURNAL OF CHEMICAL PHYSICS VOLUME 108, NUMBER 15 15 APRIL 1998 Density functional theory with an approximate kinetic energy functional applied to study structure and stability of weak van der Waals complexes

More information

Methyl Formate as a probe of temperature and structure of Orion-KL

Methyl Formate as a probe of temperature and structure of Orion-KL Methyl Formate as a probe of temperature and structure of Orion-KL Cécile Favre Århus University - Institut for Fysik og Astronomy (IFA) N. Brouillet (LAB), D. Despois (LAB), A. Baudry (LAB), A. Wootten

More information

LLNL-PRES W. M. Howard and S. Bastea Extreme Chemistry Group. Lawrence Livermore National Laboratory

LLNL-PRES W. M. Howard and S. Bastea Extreme Chemistry Group. Lawrence Livermore National Laboratory Titan s Interior :(I) A thermo-chemical assessment suggests N 2 is the dominate source of nitrogen near Titan s surface\\ and (II) future studies on the effects of comet impacts on organic and surface

More information

8: Composition and Physical state of Interstellar Dust

8: Composition and Physical state of Interstellar Dust 8: Composition and Physical state of Interstellar Dust James Graham UC, Berkeley 1 Reading Tielens, Interstellar Medium, Ch. 5 Mathis, J. S. 1990, AARA, 28, 37 Draine, B. T., 2003, AARA, 41, 241 2 Nature

More information

Interstellar chemistry. Liv Hornekær

Interstellar chemistry. Liv Hornekær Interstellar chemistry Liv Hornekær Overall structure of the ISM 21 cm 2.6 mm Overview picture 21 cm observations Leiden-Dwingeloo/Argentina/Bonn H atom La: 121.6 nm, 10.2 ev J=L+S F=I+J Relative abundance

More information

Amandeep S. Bolina, Angela J. Wolff, and Wendy A. Brown*

Amandeep S. Bolina, Angela J. Wolff, and Wendy A. Brown* 16836 J. Phys. Chem. B 2005, 109, 16836-16845 Reflection Absorption Infrared Spectroscopy and Temperature-Programmed Desorption Studies of the Adsorption and Desorption of Amorphous and Crystalline Water

More information

Moment equations for chemical reactions on interstellar dust grains. A. Lipshtat and O. Biham

Moment equations for chemical reactions on interstellar dust grains. A. Lipshtat and O. Biham A&A 400, 585 593 (003) DOI: 10.1051/0004-6361:00190 c ESO 003 Astronomy & Astrophysics Moment equations for chemical reactions on interstellar dust grains A. Lipshtat and O. Biham Racah Institute of Physics,

More information

Nucleosynthesis and stellar lifecycles. A. Ruzicka

Nucleosynthesis and stellar lifecycles. A. Ruzicka Nucleosynthesis and stellar lifecycles A. Ruzicka Stellar lifecycles A. Ruzicka Outline: 1. What nucleosynthesis is, and where it occurs 2. Molecular clouds 3. YSO & protoplanetary disk phase 4. Main Sequence

More information

Astrochemistry (2) Interstellar extinction. Measurement of the reddening

Astrochemistry (2) Interstellar extinction. Measurement of the reddening Measurement of the reddening The reddening of stellar colours casts light on the properties of interstellar dust Astrochemistry (2) Planets and Astrobiology (2016-2017) G. Vladilo The reddening is measured

More information

Advanced Electronic Structure Theory Density functional theory. Dr Fred Manby

Advanced Electronic Structure Theory Density functional theory. Dr Fred Manby Advanced Electronic Structure Theory Density functional theory Dr Fred Manby fred.manby@bris.ac.uk http://www.chm.bris.ac.uk/pt/manby/ 6 Strengths of DFT DFT is one of many theories used by (computational)

More information

" There's life Jim...but we don't KNOW it (yet): a journey through the chemically controlled cosmos from star birth to the formation of life"

 There's life Jim...but we don't KNOW it (yet): a journey through the chemically controlled cosmos from star birth to the formation of life " There's life Jim...but we don't KNOW it (yet): a journey through the chemically controlled cosmos from star birth to the formation of life" 30 th May 2007, Stockholm Observatory with support from the

More information

Dissociative recombination reactions. Wolf D. Geppert ISSI workshop, Bern (CH) December 2008

Dissociative recombination reactions. Wolf D. Geppert ISSI workshop, Bern (CH) December 2008 Dissociative recombination reactions Wolf D. Geppert ISSI workshop, Bern (CH) December 2008 Important electron-ion processes A B - Resonant ion pair formation (high energies) AB hν Radiative recombination

More information

Formation of complex molecules after energetic processing of icy grain mantles

Formation of complex molecules after energetic processing of icy grain mantles Formation of complex molecules after energetic processing of icy grain mantles Maria Elisabetta Palumbo INAF Osservatorio Astrofisico di Catania mepalumbo@oact.inaf.it http://www.oact.inaf.it/weblab/ Molecules

More information

E. Rauls. Department of Theoretical Physics, Faculty of Natural Sciences, University of Paderborn, D Paderborn, Germany;

E. Rauls. Department of Theoretical Physics, Faculty of Natural Sciences, University of Paderborn, D Paderborn, Germany; The Astrophysical Journal, 679:531Y536, 2008 May 20 # 2008. The American Astronomical Society. All rights reserved. Printed in U.S.A. A CATALYZED ROUTES TO MOLECULAR HYDROGEN FORMATION AND HYDROGEN ADDITION

More information

Oxidation processes on cold surfaces, diffusion and reactivity

Oxidation processes on cold surfaces, diffusion and reactivity Marco Minissale Université de Cergy-Pontoise and Observatoire de Paris Oxidation processes on cold surfaces, diffusion and reactivity Leiden, 13th March 2013 What we know about oxygenation? Astrophysical

More information

A laboratory study of the OD stretching mode band in H 2 O:HDO ice mixtures.

A laboratory study of the OD stretching mode band in H 2 O:HDO ice mixtures. A laboratory study of the OD stretching mode band in H 2 O:HDO ice mixtures. Preliminary Results R.G. Urso 1,2, C. Scirè 1, G.A. Baratta 1, M.E. Palumbo 1 rurso@oact.inaf.it 1 INAF-Osservatorio Astrofisico

More information

CARBON MONOXIDE ENTRAPMENT IN INTERSTELLAR ICE ANALOGS M. P. Collings, J. W. Dever, H. J. Fraser, 1 M. R. S. McCoustra, and D. A.

CARBON MONOXIDE ENTRAPMENT IN INTERSTELLAR ICE ANALOGS M. P. Collings, J. W. Dever, H. J. Fraser, 1 M. R. S. McCoustra, and D. A. The Astrophysical Journal, 583:1058 1062, 2003 February 1 # 2003. The American Astronomical Society. All rights reserved. Printed in U.S.A. CARBON MONOXIDE ENTRAPMENT IN INTERSTELLAR ICE ANALOGS M. P.

More information

* Corresponding authors:

* Corresponding authors: Mechanism of Olefin Hydrogenation Catalysis Driven by Palladium-Dissolved Hydrogen Satoshi Ohno,*, Markus Wilde,*, Kozo Mukai, Jun Yoshinobu, and Katsuyuki Fukutani Institute of Industrial Science, The

More information

Adsorption on Interstellar Analog Surfaces: from Atoms to Organic Molecules

Adsorption on Interstellar Analog Surfaces: from Atoms to Organic Molecules THÈSE DE DOCTORAT DE L UNIVERSITÉ PIERRE ET MARIE CURIE Spécialité : Physique École doctorale : Physique en Île-de-France réalisée au Laboratoire d Études du Rayonnement et de la Matière en Astrophysique

More information

Reduction of unsaturated compounds under interstellar conditions: chemoselective reduction of C C and C=C bonds over C=O functional group

Reduction of unsaturated compounds under interstellar conditions: chemoselective reduction of C C and C=C bonds over C=O functional group Reduction of unsaturated compounds under interstellar conditions: chemoselective reduction of C C and C=C bonds over C=O functional group Mindaugas Jonusas, Jean-Claude Guillemin, Lahouari Krim To cite

More information

Work hard. Be nice. Name: Period: Date:

Work hard. Be nice. Name: Period: Date: Name: Period: Date: UNIT 6: Organic Chemistry Lesson 2: Isomers and Side Chains By the end of today, you will have an answer to: What happens when two different molecules have the same formula? Do Now:

More information

10 Marking scheme: End-of-chapter test

10 Marking scheme: End-of-chapter test 1 a Element Carbon Hydrogen Oxygen Percentage 62.1 10.3 27.6 Mass in 100 g 62.1 g 10.3 g 27.6 g Number of moles 62.1 10.3 27.6 = 5.18 = 10.3 = Relative number 5.18 10.3 of atoms = 3 = 6 = 1 empirical formula

More information

Astrochemistry Lecture 2 Basic Processes (cont d)

Astrochemistry Lecture 2 Basic Processes (cont d) Astrochemistry Lecture 2 Basic Processes (cont d) Ewine F. van Dishoeck Leiden Observatory Spring 2008 Types of chemical reactions Formation of bonds Radiative association: X + + Y XY + + hν Associative

More information

The structure of water on the (0001) surface of graphite

The structure of water on the (0001) surface of graphite Surface Science 532 535 (2003) 166 172 www.elsevier.com/locate/susc The structure of water on the (0001) surface of graphite P. Cabrera Sanfelix a, S. Holloway a, K.W. Kolasinski b, G.R. Darling a, * a

More information

Protonated Polycyclic Aromatic Hydrocarbons and the Interstellar Medium

Protonated Polycyclic Aromatic Hydrocarbons and the Interstellar Medium 1 Chapter 1 Protonated Polycyclic Aromatic Hydrocarbons and the Interstellar Medium 1.1 Interstellar Molecules Although hydrogen is the most abundant element in the universe, it is other elements that

More information

Supporting information for Polymer interactions with Reduced Graphene Oxide: Van der Waals binding energies of Benzene on defected Graphene

Supporting information for Polymer interactions with Reduced Graphene Oxide: Van der Waals binding energies of Benzene on defected Graphene Supporting information for Polymer interactions with Reduced Graphene Oxide: Van der Waals binding energies of Benzene on defected Graphene Mohamed Hassan, Michael Walter *,,, and Michael Moseler, Freiburg

More information

Lecture 11. IR Theory. Next Class: Lecture Problem 4 due Thin-Layer Chromatography

Lecture 11. IR Theory. Next Class: Lecture Problem 4 due Thin-Layer Chromatography Lecture 11 IR Theory Next Class: Lecture Problem 4 due Thin-Layer Chromatography This Week In Lab: Ch 6: Procedures 2 & 3 Procedure 4 (outside of lab) Next Week in Lab: Ch 7: PreLab Due Quiz 4 Ch 5 Final

More information

9 - The Hot Corinos. Complex organic molecules in the inner 100 AU envelope of Solar type protostars

9 - The Hot Corinos. Complex organic molecules in the inner 100 AU envelope of Solar type protostars 9 - The Hot Corinos Complex organic molecules in the inner 100 AU envelope of Solar type protostars 1 THE COLLAPSING PROTOSTAR PHASE 2 THE INNER ENVELOPES OF LOW MASS PROTOSTARS Direct observations of

More information

EVOLUTION OF MOLECULAR ABUNDANCE IN PROTOPLANETARY DISKS

EVOLUTION OF MOLECULAR ABUNDANCE IN PROTOPLANETARY DISKS EVOLUTION OF MOLECULAR ABUNDANCE IN PROTOPLANETARY DISKS Yuri Aikawa 1 Department of Earth and Planetary Science, University of Tokyo, Bunkyo-ku, Tokyo 113, Japan arxiv:astro-ph/9706204v1 19 Jun 1997 Toyoharu

More information

Title of file for HTML: Supplementary Information Description: Supplementary Figures, Supplementary Tables and Supplementary References

Title of file for HTML: Supplementary Information Description: Supplementary Figures, Supplementary Tables and Supplementary References Title of file for HTML: Supplementary Information Description: Supplementary Figures, Supplementary Tables and Supplementary References Title of file for HTML: Supplementary Movie 1 Description: This movie

More information

Theoretical Electronic and Rovibrational Studies for Anions of Interest to the DIBs

Theoretical Electronic and Rovibrational Studies for Anions of Interest to the DIBs Georgia Southern University From the SelectedWorks of Ryan C. Fortenberry 2013 Theoretical Electronic and Rovibrational Studies for Anions of Interest to the DIBs Ryan C. Fortenberry, Georgia Southern

More information

HYDROGENATION OF CO ON PURE SOLID CO AND CO-H 2 O MIXED ICE

HYDROGENATION OF CO ON PURE SOLID CO AND CO-H 2 O MIXED ICE The Astrophysical Journal, 616:638 642, 2004 November 20 # 2004. The American Astronomical Society. All rights reserved. Printed in U.S.A. HYDROGENATION OF CO ON PURE SOLID CO AND CO-H 2 O MIXED ICE Naoki

More information

Outline. Introduction: graphene. Adsorption on graphene: - Chemisorption - Physisorption. Summary

Outline. Introduction: graphene. Adsorption on graphene: - Chemisorption - Physisorption. Summary Outline Introduction: graphene Adsorption on graphene: - Chemisorption - Physisorption Summary 1 Electronic band structure: Electronic properties K Γ M v F = 10 6 ms -1 = c/300 massless Dirac particles!

More information

Effect of Electric Field on Condensed-Phase Molecular Systems. II. Stark Effect on the Hydroxyl Stretch Vibration of Ice

Effect of Electric Field on Condensed-Phase Molecular Systems. II. Stark Effect on the Hydroxyl Stretch Vibration of Ice Effect of Electric Field on Condensed-Phase Molecular Systems. II. Stark Effect on the Hydroxyl Stretch Vibration of Ice Sunghwan Shin, Hani Kang, Daeheum Cho, Jin Yong Lee, *, and Heon Kang *, Department

More information

Chem. 1C Midterm 1 Practice Test 2

Chem. 1C Midterm 1 Practice Test 2 Chem. 1C Midterm 1 Practice Test 2 First initial of last name Name Student Number All work must be shown on the exam for partial credit. Points will be taken off for incorrect or no units. Calculators

More information

Status of the Diffuse Interstellar Band Problem

Status of the Diffuse Interstellar Band Problem Status of the Diffuse Interstellar Band Problem Ben McCall Department of Chemistry and Department of Astronomy University of Illinois at Urbana-Champaign APO DIB Collaboration: Tom Fishman (Chicago), Scott

More information

Radio astronomy, Lecture 14

Radio astronomy, Lecture 14 Radio astronomy, Lecture 14 1) Molecular clouds 2) Dust 3) ALMA 1937 1 Laboratory tour Helmholtzweg 3 (rotes Haus), Montag 05.02.18 12-00 1937 2 The whole sky (by eyes) Lund observatory 3 The whole sky

More information

GAS PHASE CHEMICAL KINETICS : EXPERIMENTAL ADVANCES AND PROSPECTS

GAS PHASE CHEMICAL KINETICS : EXPERIMENTAL ADVANCES AND PROSPECTS GAS PHASE CHEMICAL KINETICS : EXPERIMENTAL ADVANCES AND PROSPECTS Sébastien Le Picard France Astrophysique de Laboratoire Institut de Physique de Rennes Université de Rennes 1 Gas phase chemistry in the

More information

Astrochimistry Spring 2013

Astrochimistry Spring 2013 Astrochimistry Spring 2013 Lecture 3: H2 Formation NGC 7023 - HST Julien Montillaud 1st February 2013 Outline I. The most abundant molecule in the Universe (6 p.) I.1 Relative abundances I.2 Historical

More information

TPD-MS. Photocatalytic Studies Using Temperature Programmed Desorption Mass Spectrometry (TPD-MS) APPLICATION NOTE NOTE

TPD-MS. Photocatalytic Studies Using Temperature Programmed Desorption Mass Spectrometry (TPD-MS) APPLICATION NOTE NOTE TPD-MS APPLICATION NOTE NOTE Photocatalytic Studies Using Temperature Programmed Desorption Mass Spectrometry (TPD-MS) Thermal analysis consists of many techniques for the exploration of the physical properties

More information

Au-C Au-Au. g(r) r/a. Supplementary Figures

Au-C Au-Au. g(r) r/a. Supplementary Figures g(r) Supplementary Figures 60 50 40 30 20 10 0 Au-C Au-Au 2 4 r/a 6 8 Supplementary Figure 1 Radial bond distributions for Au-C and Au-Au bond. The zero density regime between the first two peaks in g

More information

New Perspective on structure and bonding in water using XAS and XRS

New Perspective on structure and bonding in water using XAS and XRS New Perspective on structure and bonding in water using XAS and XRS Anders Nilsson Stanford Synchrotron Radiation Laboratory (SSRL) and Stockholm University, Sweden R. Ludwig Angew. Chem. 40, 1808 (2001)

More information

Photo-Dissociation Resonances of Jet-Cooled NO 2 by CW-CRDS

Photo-Dissociation Resonances of Jet-Cooled NO 2 by CW-CRDS Photo-Dissociation Resonances of Jet-Cooled NO 2 by CW-CRDS Patrick DUPRÉ Laboratoire de Physico-Chimie de l Atmosphère, Université du Littoral, Côte d Opale Dunkerque, France ISMS 22-26 June 2015 Patrick

More information

Effects of methanol on crystallization of water in the deeply super cooled region

Effects of methanol on crystallization of water in the deeply super cooled region Effects of methanol on crystallization of water in the deeply super cooled region Ryutaro Souda Nanoscale Materials Center National Institute for Materials Science Japan PHYSICAL REVIEW B 75, 184116, 2007

More information

Interstellar dust: The hidden protagonist. Stéphanie Cazaux Marco Spaans Vincent Cobut Paola Caselli Rowin Meijerink

Interstellar dust: The hidden protagonist. Stéphanie Cazaux Marco Spaans Vincent Cobut Paola Caselli Rowin Meijerink Interstellar dust: The hidden protagonist Stéphanie Cazaux Marco Spaans Vincent Cobut Paola Caselli Rowin Meijerink th 15 February 2012 Overview Star form in clouds made of gas + dust Catalyst: Enrich

More information

COMBINED IRAM, Herschel/HIFI and ALMA STUDIES of abundant molecules in ORION KL

COMBINED IRAM, Herschel/HIFI and ALMA STUDIES of abundant molecules in ORION KL COMBINED IRAM, Herschel/HIFI and ALMA STUDIES of abundant molecules in ORION KL Belén Tercero ICMM-CSIC, Madrid, Spain CONTENTS 1. ORION REGION 2. THREE SETS OF DATA 3. STUDIES OF ORION-KL 4. CONCLUSIONS

More information

List of Figures Page Figure No. Figure Caption No. Figure 1.1.

List of Figures Page Figure No. Figure Caption No. Figure 1.1. List of Figures Figure No. Figure Caption Page No. Figure 1.1. Cation- interactions and their modulations. 4 Figure 1.2. Three conformations of benzene dimer, S is not a minimum on the potential energy

More information

Millimeter and submillimeter wave spectra of N-methyl formamide and propionamide

Millimeter and submillimeter wave spectra of N-methyl formamide and propionamide Millimeter and submillimeter wave spectra of N-methyl formamide and propionamide A.A. Mescheryakov, E.A. Alekseev, V.V. Ilyushin Institute of Radio Astronomy, NASU, Kharkov, Ukraine R.A. Motiyenko, L.

More information

Supporting information for Chemical and Electrochemical. Surfaces: Insights into the Mechanism and Selectivity from DFT.

Supporting information for Chemical and Electrochemical. Surfaces: Insights into the Mechanism and Selectivity from DFT. Electronic Supplementary Material (ESI) for RSC Advances. This journal is The Royal Society of Chemistry 2015 Supporting information for Chemical and Electrochemical Hydrogenation of CO 2 to hydrocarbons

More information

Sticking coefficient of hydrogen and deuterium on silicates under interstellar conditions

Sticking coefficient of hydrogen and deuterium on silicates under interstellar conditions Astronomy & Astrophysics ESO 0 Sticking coefficient of hydrogen and deuterium on silicates under interstellar conditions H. Chaabouni, H. Bergeron, S. Baouche, F. Dulieu, E. Matar, E. Congiu, L. Gavilan,

More information

arxiv: v1 [astro-ph] 22 May 2008

arxiv: v1 [astro-ph] 22 May 2008 Structural effects of ice grain surfaces on the hydrogenation of at low temperatures arxiv:0805.3383v1 [astro-ph] 22 May 2008 H. Hidaka a,, N. Miyauchi a, A. Kouchi a, N. Watanabe a a Institute of Low

More information

AP Chemistry Readiness Liquids, Solids, and Solutions Review Page 1 of 16. AP Chemistry Review Session December 10, 2016 UCLA

AP Chemistry Readiness Liquids, Solids, and Solutions Review Page 1 of 16. AP Chemistry Review Session December 10, 2016 UCLA AP Chemistry Readiness Liquids, Solids, and Solutions Review Page 1 of 16 AP Chemistry Review Session December 10, 2016 UCLA Michael A. Morgan mmorgan@lausd.net Richard Erdman xchemteach@yahoo.com Francisco

More information

Carbon Compounds. Chemical Bonding Part 2

Carbon Compounds. Chemical Bonding Part 2 Carbon Compounds Chemical Bonding Part 2 Introduction to Functional Groups: Alkanes! Alkanes Compounds that contain only carbons and hydrogens, with no double or triple bonds.! Alkyl Groups A part of a

More information

CHEM 301: Homework assignment #12

CHEM 301: Homework assignment #12 CHEM 301: Homework assignment #12 Solutions 1. Let s practice converting between wavelengths, frequencies, and wavenumbers. (10%) Express a wavelength of 442 nm as a frequency and as a wavenumber. What

More information

Astrochemistry from a Sub-pc Scale to a kpc Scale. Satoshi Yamamoto Department of Physics and RESCUE The University of Tokyo

Astrochemistry from a Sub-pc Scale to a kpc Scale. Satoshi Yamamoto Department of Physics and RESCUE The University of Tokyo Astrochemistry from a Sub-pc Scale to a kpc Scale Satoshi Yamamoto Department of Physics and RESCUE The University of Tokyo Contents Physical and Chemical Processes in Disk Formation around Solar-type

More information

Introduction. H2 case. The Chemical Desorption. O+O case O2 + H. APiMI meeting Leiden, 13th of march Water form. Others cases.

Introduction. H2 case. The Chemical Desorption. O+O case O2 + H. APiMI meeting Leiden, 13th of march Water form. Others cases. The Chemical Desorption APiMI meeting Leiden, 13th of march 2013 Accretion time H/H2 transition 3 nn==~~1/cm 1/cm3 T= T=1000K 1000K n > 1000/cm3 T= 10 K n = 100/cm3 Tgas= 100 K Tgrains= 20 K CO depletion

More information

arxiv: v1 [astro-ph] 17 Sep 2007

arxiv: v1 [astro-ph] 17 Sep 2007 Astronomy & Astrophysics manuscript no. 8210Hat c ESO 2008 February 1, 2008 H-atom bombardment of CO 2, HCOOH and CH 3 CHO containing ices S. E. Bisschop, G. W. Fuchs, E. F. van Dishoeck, and H. Linnartz

More information

Supporting information for Activity descriptors for CO 2 electroreduction to methane on transition-metal catalysts

Supporting information for Activity descriptors for CO 2 electroreduction to methane on transition-metal catalysts Supporting information for Activity descriptors for CO 2 electroreduction to methane on transition-metal catalysts Andrew A. Peterson 1,3, Jens K. Nørskov 1,2 SUNCAT Center for Interface Science and Catalysis,

More information

THE NITRILES PROJECT: MOLECULE FORMATION IN THE GALACTIC CENTER

THE NITRILES PROJECT: MOLECULE FORMATION IN THE GALACTIC CENTER THE NITRILES PROJECT: MOLECULE FORMATION IN THE GALACTIC CENTER JOANNA CORBY (www.astro.virginia.edu/~jfc9va) University of Virginia, Department of Astronomy Advised by Anthony Remijan, National Radio

More information

The effects of methanol on the trapping of volatile ice components

The effects of methanol on the trapping of volatile ice components doi:10.1093/mnras/stv109 The effects of methanol on the trapping of volatile ice components Daren J. Burke and Wendy A. Brown Division of Chemistry, University of Sussex, Falmer, Brighton, BN1 9QJ, UK

More information

Astronomy. Astrophysics. Formation of methyl formate after cosmic ion irradiation of icy grain mantles. P. Modica and M. E. Palumbo. 1.

Astronomy. Astrophysics. Formation of methyl formate after cosmic ion irradiation of icy grain mantles. P. Modica and M. E. Palumbo. 1. DOI: 10.1051/0004-6361/201014101 c ESO 2010 Astronomy & Astrophysics Formation of methyl formate after cosmic ion irradiation of icy grain mantles P. Modica and M. E. Palumbo INAF Osservatorio Astrofisico

More information

Many-body dispersion interactions between semiconducting wires

Many-body dispersion interactions between semiconducting wires Many-body dispersion interactions between semiconducting wires Alston J. Misquitta TCM Group, Cavendish Laboratory University of Cambridge 26 th July, 2010 Collaborators James Spencer (Imperial College,

More information

Supporting Information for. Dynamics Study"

Supporting Information for. Dynamics Study Supporting Information for "CO 2 Adsorption and Reactivity on Rutile TiO 2 (110) in Water: An Ab Initio Molecular Dynamics Study" Konstantin Klyukin and Vitaly Alexandrov,, Department of Chemical and Biomolecular

More information

Thermal desorption of water ice in the interstellar medium

Thermal desorption of water ice in the interstellar medium Mon. Not. R. Astron. Soc. 327, 1165 1172 (2001) Thermal desorption of water ice in the interstellar medium Helen J. Fraser, 1P Mark P. Collings, 1 Martin R. S. McCoustra 1 and David A. Williams 2 1 School

More information

PCCP Accepted Manuscript

PCCP Accepted Manuscript PCCP Accepted Manuscript This is an Accepted Manuscript, which has been through the Royal Society of Chemistry peer review process and has been accepted for publication. Accepted Manuscripts are published

More information

A Far-ultraviolet Fluorescent Molecular Hydrogen Emission Map of the Milky Way Galaxy

A Far-ultraviolet Fluorescent Molecular Hydrogen Emission Map of the Milky Way Galaxy A Far-ultraviolet Fluorescent Molecular Hydrogen Emission Map of the Milky Way Galaxy (The Astrophysical Journal Supplement Series, 231:21 (16pp), 2017 August) November 14, 2017 Young-Soo Jo Young-Soo

More information

Production of complex organic molecules: H-atom addition versus UV irradiation

Production of complex organic molecules: H-atom addition versus UV irradiation MNRAS 467, 25522565 (2017) Advance Access publication 2017 January 25 doi:10.1093/mnras/stx222 Production of complex organic molecules: H-atom addition versus UV irradiation K.-J. Chuang, 1,2 G. Fedoseev,

More information

Cryochemistry in the inert and interstellar media

Cryochemistry in the inert and interstellar media Cryochemistry in the inert and interstellar media Serge A. Krasnokutski Friedrich Schiller University of Jena, 07740 Jena, Germany MPI for Astronomy, Königstuhl 17,69117 Heidelberg, Germany Holes in heaven

More information

H 2 O and CO Ices in Protostellar Environments Recent Keck Telescope Results. Adwin Boogert California Inst. of Technology. Interstellar Ices-I

H 2 O and CO Ices in Protostellar Environments Recent Keck Telescope Results. Adwin Boogert California Inst. of Technology. Interstellar Ices-I Interstellar Ices-1 H 2 O and CO Ices in Protostellar Environments Recent Keck Telescope Results Adwin Boogert California Inst. of Technology Jan/2005 Interstellar Ices-I Contents Infrared spectra of highly

More information

Interaction between Single-walled Carbon Nanotubes and Water Molecules

Interaction between Single-walled Carbon Nanotubes and Water Molecules Workshop on Molecular Thermal Engineering Univ. of Tokyo 2013. 07. 05 Interaction between Single-walled Carbon Nanotubes and Water Molecules Shohei Chiashi Dept. of Mech. Eng., The Univ. of Tokyo, Japan

More information

Functionalized Carbon Nanotubes a key to nanotechnology?

Functionalized Carbon Nanotubes a key to nanotechnology? 1 27th Max Born Symposium Multiscale Modeling of Real Materials Wroclaw, Sep 19, 2010 Functionalized Carbon Nanotubes a key to nanotechnology? Karolina Milowska, Magda Birowska & Jacek A. Majewski Faculty

More information

Physical Chemistry Chemical Physics

Physical Chemistry Chemical Physics Physical Chemistry Chemical Physics www.rsc.org/pccp Volume 13 Number 23 21 June 2011 Pages 10825 11452 ISSN 1463-9076 COVER ARTICLE Head et al. A computational study on the structures of methylamine carbon

More information

Design of Efficient Catalysts with Double Transition Metal. Atoms on C 2 N Layer

Design of Efficient Catalysts with Double Transition Metal. Atoms on C 2 N Layer Supporting Information Design of Efficient Catalysts with Double Transition Metal Atoms on C 2 N Layer Xiyu Li, 1, Wenhui Zhong, 2, Peng Cui, 1 Jun Li, 1 Jun Jiang 1, * 1 Hefei National Laboratory for

More information

Dust in the Diffuse Universe

Dust in the Diffuse Universe Dust in the Diffuse Universe Obscuring Effects Chemical Effects Thermal Effects Dynamical Effects Diagnostic Power Evidence for Grains: Chemical Effects Catalyzes molecular hydrogen formation. Depletion

More information

Experimental and Quantum Investigation on Ice Surface Structure and Reactivity

Experimental and Quantum Investigation on Ice Surface Structure and Reactivity Experimental and Quantum Investigation on Ice Surface Structure and Reactivity A.Allouche J.P.Aycard F.Borget T.Chiavassa I.Couturier C.Manca F.Marinelli C.Martin S.Raunier P.Roubin Physique des Interactions

More information

Electronic Supplementary Information

Electronic Supplementary Information Electronic Supplementary Material (ESI) for Green Chemistry. This journal is The Royal Society of Chemistry 2016 Electronic Supplementary Information Interfacial acidity in ligand-modified ruthenium nanoparticles

More information

Novel astrochemical aspects of cyanoacetylene-related molecules

Novel astrochemical aspects of cyanoacetylene-related molecules Novel astrochemical aspects of cyanoacetylene-related molecules R. KOŁOS 1,2, M. GRONOWSKI 1 & M. TUROWSKI 1 1) Institute of Physical Chemistry, Polish Academy of Sciences, Warsaw 2) Faculty of Mathematics

More information

Interstellar Dust and Extinction

Interstellar Dust and Extinction University of Oxford, Astrophysics November 12, 2007 Outline Extinction Spectral Features Emission Scattering Polarization Grain Models & Evolution Conclusions What and Why? Dust covers a range of compound

More information

Mechanisms of H- and OH-assisted CO activation as well as C-C coupling on the flat Co(0001) surface Revisited

Mechanisms of H- and OH-assisted CO activation as well as C-C coupling on the flat Co(0001) surface Revisited Electronic Supplementary Material (ESI) for Catalysis Science & Technology. This journal is The Royal Society of Chemistry 2016 Mechanisms of H- and OH-assisted CO activation as well as C-C coupling on

More information

High Resolution Spectroscopy and Astronomical Detection of Molecular Anions

High Resolution Spectroscopy and Astronomical Detection of Molecular Anions High Resolution Spectroscopy and Astronomical Detection of Molecular Anions Sandra Brünken, C. A. Gottlieb, H. Gupta, M. C. McCarthy, and P.Thaddeus Harvard Smithsonian Center for Astrophysics 10th Biennial

More information

Broadband Nitrile Reaction Screening. Kiera Matthews Hanifah Hendricks

Broadband Nitrile Reaction Screening. Kiera Matthews Hanifah Hendricks Broadband Nitrile Reaction Screening Kiera Matthews Hanifah Hendricks Acknowledgements Brooks Pate - University of Virginia Justin Neill University of Virginia Sarah Payne - University of Virginia Michael

More information

Solid-state formation of complex molecules under dense cloud conditions

Solid-state formation of complex molecules under dense cloud conditions Solid-state formation of complex molecules under dense cloud conditions Gleb Fedoseev 1,2 K.-J. Chuang 2,3, S. Ioppolo 4, E. F. van Dishoeck 3, M. E. Palumbo 1 and H. Linnartz 2 1 INAF Osservatorio Astrofisico

More information

Supplementary Figure 1 Morpholigical properties of TiO 2-x SCs. The statistical particle size distribution (a) of the defective {001}-TiO 2-x SCs and

Supplementary Figure 1 Morpholigical properties of TiO 2-x SCs. The statistical particle size distribution (a) of the defective {001}-TiO 2-x SCs and Supplementary Figure 1 Morpholigical properties of TiO 2-x s. The statistical particle size distribution (a) of the defective {1}-TiO 2-x s and their typical TEM images (b, c). Quantity Adsorbed (cm 3

More information