•Interstellar and Circumstellar Chemistries: The Role of Neutral-Neutral Reactions ERIC HERBST DEPARTMENTS OF PHYSICS AND ASTRONOMY THE OHIO STATE UNIVERSITY dense (giant) molecular clouds organic molecules H core 4 -3 n = 10 cm T = 10 K 2 PDR’s embedded stars hot ionized gas HII region protoplanetary disk studied in millimeter-wave and IR GAS PHASE INTERSTELLAR/CIRCUMSTELLAR MOLECULES - HIGH RESOLUTION (9/02) _____________________________________________________________________________________________ H2 KCl HNC C3S C5 C6H HC4CN HCO NH3 CH3 H3O+ CH AlCl CH4 CH3OH AlF HCO+ H2CO SiH4 CH3SH NH PN HOC+ H2CS CH2NH C2H4 OH SiN HN2+ HCCH H2C3(lin) CH3CN C2 SiO HNO HCNH+ c-C3H2 CH3NC C7H, C6H2 C8H HCOOCH3 CH3COOH CH3C2CN H2C6(lin) C6H2 H2COHCHO C2H5OH (CH3)2O CH+ CN SiS HCS+ H2CN CH2CN HC2CHO C2H5CN CO CO+ SO+ C3 C2O CO2 C2S C3H(lin) c-C3H NH2CN CH3C4H CH2CO NH2CHO HC3NH+ HCCN HCOOH C4H2 H2C4(lin) HNCO SiC3 HOCO+ C4H HNCS C2CN C3O NaCN HCCNC HNCCC C4Si H2COH+ CSi + CP H3 CS HF NO CH2 NH2 SiC2 SiCN SO2 NS SO HCl NaCl H2O H2S C2H HCN OCS MgNC MgCN N2O HC2CN C5H C5N CH3NH2 CH2CHOH CH3CCH CH3CHO CH2CHCN c-CH2OCH2 c-CH2SCH2 HC6CN (CH2OH)2 (CH3)2CO CH3C4CN? NH2CH2COOH? HC8CN c-C6H6 HC10CN + ISOTOPOMERS Dust particles contain 1% of interstellar matter. POTENTIAL ENERGY OF REACTION activation energy typical neutral reactions radical-radical reactions A+B ion-molecule reactions k(T) = A(T) exp(-Ea /kT) C+ D Cosmic rays produce ions Radical-Neutral Reactions Radicals: C, CN, CCH 1) Inverse T dependence 2) Large rate coefficients by 10-50 K: k 10(-10) cm3 s-1 (diffusion) FORMATION OF GASEOUS WATER H2 + COSMIC RAYS H2+ + e Elemental abundances: C,O,N = 10(-4); C<O Elemental abundances: C,O,N = 10(-4); C<O H2+ + H2 H3+ + H H3+ + O OH+ + H2 OHn+ + H2 OHn+1+ + H H3O+ + e H2O + H; OH + 2H, etc FORMATION OF O2 ,N2 CO OH + O O2 + H OH + N NO + H NO + N N2 + O CH + O CO + H CO, N2 + He+ C+, N+ +… Precursor to ammonia, hydrocarbons ORGANIC SYNTHESIS CONT. SOME SYNTHETIC REAC TION CLASSES: A. CARBON INSERTION C+ + CH 4 -----> C2H3+ + H ------> C2H2+ + H2 B. CONDENSATION C2H2+ + C2H2 -----> C4H3+ + H C. ATOM IC INSERTION N + C3H3+ -----> HC3NH+ + H D. RADIATIVE ASSOCIATION CH3+ + H2O -----> CH3OH2+ + h E. NEUTRAL-NEUTRAL C + C2H2 C3H + H NEUTRAL-NEUTRAL RX (CONT) CN + C2H2 HCCCN + H CCH + C2H2 C4H2 + H CCH + HCN HCCCN + H YES YES NO O + CCH CO + CH k 1.2 10(-11) cm3 s-1 MAYBE (Ea = 250K?) GAS-PHASE MODELS A+ + B C+ + D k1 C+ + D PRODUCTS k2 d[C+]/dt = k1[A+][B] – k2[C+][D] Constraints: initial concentrations, elemental abundances, density, charge neutrality Steady-state solution: d[C+]/dt = 0 exists for constant density but takes very long (107 yr) to be achieved. CURRENT GAS-PHASE MODEL NETWORKS 4,000 reactions; 10-20% "studied"; 400 species through 13 atoms in size elements: H, He, N, O, C, S, Si, Fe, Na, Mg, P, Cl elemental abundances: “low metal” photodestruction: external, internal (via cosmic rays) Successes for quiescent cores: (1)Reproduces 80% of abundances including ions, radicals, isomers (2)Predicts strong deuterium fractionation CURRENT APPROACH TO NEUTRAL-NEUTRAL RX DO NOT EXTRAPOLATE NEW LOW TEMPERATURE RESULTS UNLESS IN FAMILIES (e.g. C + HCCCN NO) MAINTAIN PAST ESTIMATES UNLESS CONSENSUS THAT THEY ARE INCORRECT. (E.G. O + Cn, CnH) INCLUDES LOW RATE CONSTANT. ESTIMATES IMPROVED WITH IAN; WORK IN PROGRESS IRC10216: An AGB (Old) Star LTE Molecules and dust here C>O N,T similar to cloud CO, C2H2, HCN UV radiation + cosmic rays Actual Distributions GROWTH OF MOLECULES Occurs via neutral and ionic (+ and -) reactions. Modified network necessary to account for acetylenic chemistry. Photochemistry important in the production of radicals such as CN and CCH C2H2 + h CCH + H GROWTH OF MOLECULES. II CCH + C2nH2 C2n+2H2 + H CN + C2nH2 HC2n+1N + H C2nH reactions with hydrocarbons, HCN(?), HNC(?) as well as cyanoacetylenes. Benzene formed via ion-molecule rx. CYANOPOLYYNES in IRC Radius CRL618: A Protoplanetary Nebula Detection of benzene empty 250 K Dense Thin shell Photons, X-rays from central star! 100 x normal ionization rate SUMMARY Thanks to Ian Smith and others (Bertrand Rowe, Ian Sims, David Clary etc.), we now know that neutral-neutral reactions are competitive in both oxygen-rich and carbon-rich chemistries in interstellar and circumstellar sources!!!!! SYNTHESIS OF BENZENE C2H2+ + C2H2 C4H3+ + H C4H3+ + C2H2 c-C6H5+ + h c-C6H5+ + H2 c-C6H7+ + h c-C6H7+ + e c-C6H6 + H INITIAL ABUNDANCES w.r.t. H2 CO C2H2 HCN CH4 NH3 6(-4) 5(-5) 8(-6) 2(-6) 2(-6) ACTUAL CLOUD CORES Model TMC-1 L134N NSM/+grains 80% 80% NNM 50% 70% NOTES: (1) C=0.42 x O (2) N-N reactions involving C and O most important. (3) Larger molecules more strongly affected. TYPES OF SURFACE REACTIONS REACTANTS: MAINLY MOBILE ATOMS AND RADICALS A + B H + AB H H2 association X XH (X = O, C, N, CO, etc.) WHICH CONVERTS H + O OH H2O C CH CH2 CH3 CH4 N NH NH2 NH3 CO HCO H2CO H3CO CH3OH X + Y XY ?????????? H + HX H2 + X abstraction