6
JOURNAL OF RESEAR CH of the Notional Bureau of Standard s - A Ph ysics and Chemist ry Vol. 75A, No. 6, Nove mber-December 1971 The Photochemistry of Propane at High Photon Energies (8.4-21.2 eV) * R. E. Rebbert, S. G. Lias, and P. Ausloos Institute for Materials Research, National Bureau of Standards, Washington, D. C. 20234 (June 28,1971) Neon an d he lium res onan ce l amp s, which deliver photons of 16.7- 16.8 eV and 21.2 eV energy, res p ec ti ve l y, hav e been u sed to photo lyze C:, H H, C:,DH , C:,HW C:,OH (l: 1) mixtur es , and CD"CH,CD" an d the results ob ta in ed at the two energ ies are compared. Ln parti c ul ar , it is no ted th at although the quantum yie ld of ionization in propane is unit y at 16.7- 16 .8 eV. when the e n e rgy is rai se d s till further to 21.2 eV , the probabil it y of ionization appare ntl y dimini shes to 0.93, an obse rvation whieh sugge sts th at at 21.2 eV, s up erexcited s tat es may be re ac hed who se dissociation int o ne utral fragme nt s co mp et es with io ni za ti on. Th e quantum yie ld s of the lower h ydrocarbo n produ cts form ed in the pres ence of a radical sc av- en ge r in C:, HH a nd C:,OH are re ported , an d a re co mp ar ed with quantum yie ld s of produ cts formed in the vac uum ultr aviolet photolysis at lower e nergie s. (Qua ntum yields of produ cts formed at 8.4 eV and 10.0 eV ar e repo rted here fo r the first time.) Acetylene is formed as a produ ct in the d ec o mp osition of th e ne utr al exc it ed propan e mol ec ul e. a nd it s yi e ld increa ses in im po rt an ce with in creas in g energy; at 16.7- 16.8 eV. where a ll produ ct forma ti on can be tr ac e d to ioni c pro cesses . ace tylene is formed in neg li gible yie lds . Lt is concluded that io ni c pro cesses in propa ne do not le ad to the form ation of a ce tylene , a nd the ob se rvation of this product in radio lyti c systems may be a re li able indicator of th e re lativ e importan ce of ne utr a l e xc it ed mol ec ul e dec o mp osition pro cesses . Fro m the results obta in ed with the C:, HH' C:, OH (1: 1) mixtur e, and with CO"C H, CO ", details of the ion-molec ul e r ea c ti on mec han isms and the unim olecul ar d ec o mp osition of the prop ane ion are derived. Key words: Ion-molec ul e rea c ti on; photoionization; propan e; qua ntum yields ; rare-gas res onance radiation ; di ss ocia ti on. 1 . Introduction In th e pa st, mo st photolysis studi es in the vac uum ultraviolet region hav e bee n c arried out at energies be- low 11.8 eV (104.8 nm). Th e lamp s common ly use d in this energy region are r are gas resonance lamp s, which deliv er the resonan ce lin es of xenon (8 .4 eV, 147.0 nm ), kr ypt on (10.0 eV, 123.6 nm ), or argo n (11.6- 11.8 eV, 106.7- 104.8 nm ). Higher energy resonance l amps could not be made beca use of the lack of s uitabl e windows which would tran smit photons above 11.8 eV in energy. R ece ntl y, in this l aboratory, e ncl osed neon a nd helium lamps have b ee n fabric at ed; their opera- tional cha ra ct er is ti cs hav e bee n d esc ribed in detail [1]. t Th ese lamp s, which deliver the neon and helium resonance lin es (16 .7- 16 .8 e V and 21.2 e V, resp ec- tively), are fitted with windows mad e of thin (2 000 - 4000 A) film s of aluminum. Photoly sis studi es in this high energy re gion are, of co ur se , still very rare. Only a few studi es, limited in *Supporlcd in pa rt by the U.S. At o mi c Energy Com mi ssion, Washington, D. C. 20545 I Fi gures in brac kets indi ca te the lit e ratur e referenc es at the end of thi s pap er. scope, of the che mi ca l effects brought about in me th- ane [2 - 4] and in ar go n-propane mi x tur es [5] by helium r eso nan ce radiation have bee n published. On e of th ese studi es [2] wa s carried out with a differentially pump ed windowless helium lamp; under such condition s, the inves tigator is r es tricted to a low pressure ran ge. No studies at press ure s above the millitorr ran ge utilizing neon r eso nan ce radiation have so far appeared in th e lite ratur e. This pap er reports the r esults of a s tudy wher e, for th e first tim e, a co mpound is expo se d to both neon and helium reso nan ce radiation, and the chemic al e ffe cts at th e two energies are co mpar ed. Propan e wa s chosen as the s ubje ct co mp ound beca use the unimol ec ular and bimol ec ular (ionic and fr ee radi cal) processes oc - c urring in this system hav e bee n extensively inv es ti- gated [6] and are well und erstood. In th e high energy region used in this study, c hemi cal effects will be brought about nearly exclusively throu gh ionic pro ces - ses. A comparison of the effec ts brought about by photons of two different energies may highlight subtle differences , and, therefore, incr ease our understanding 607

The photochemistry of propane at high photon …The Photochemistry of Propane at High Photon Energies (8.4-21.2 eV) * R. E. Rebbert, S. G. Lias, and P. Ausloos Institute for Materials

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Page 1: The photochemistry of propane at high photon …The Photochemistry of Propane at High Photon Energies (8.4-21.2 eV) * R. E. Rebbert, S. G. Lias, and P. Ausloos Institute for Materials

--.-~ -- - ----~------------------

JOURNAL OF RESEARCH of the Notional Bureau of Standards - A Physics and Chemist ry Vol. 75A, No. 6, November-December 1971

The Photochemistry of Propane at High Photon Energies (8.4-21.2 eV) *

R. E. Rebbert, S. G. Lias, and P. Ausloos

Institute for Materials Research, National Bureau of Standards, Washington, D.C. 20234

(June 28,1971)

Neon an d helium resonance lamps, whic h delive r photons of 16.7- 16.8 eV and 21.2 eV e ne rgy , resp ecti ve ly, have been used to photo lyze C:, HH, C:,DH, C:,HWC:,OH (l: 1) mixtures , and CD"CH,CD" and the re sult s obta ined at th e two e nergies a re compared . Ln partic ul ar, it is no ted that although the quantum yie ld of ionization in propane is unit y at 16.7- 16.8 e V. when the ene rgy is rai sed s till further to 21.2 eV , the probabil it y of ioniza tion apparentl y dimini shes to 0.93, a n o bservation whie h s uggests that at 21.2 eV, superexc ited s tates may be reached whose di ssoc iation into ne utral frag ments competes with ioni za tion.

The quantum yie ld s of th e lower hydrocarbon produc ts form ed in the prese nce of a radi ca l scav­enge r in C:,HH a nd C:,OH a re reported , and a re co mpared with quantum yie ld s of produ cts formed in the vacuum ultrav iole t photolys is a t lower energies. (Quantum yie lds of produc ts form ed a t 8.4 eV and 10.0 eV are repo rted here fo r th e firs t time. ) Ace tylene is form ed as a produ c t in the decomposition of th e neutra l excit ed propan e mol ecule. and it s yi e ld in creases in im port an ce with increas in g e ne rgy; a t 16.7- 16.8 e V. wh e re a ll produc t forma tion ca n be traced to ioni c processes . ace tylene is formed in ne gli gib le yie lds . Lt is co nc lud ed th at ionic processes in propa ne do not lead to the forma tion o f ace ty lene , and the obse rvatio n of thi s prod uct in radio lyti c s yste ms may be a re li a b le ind icat or of th e relative importance of ne utra l exc it ed mo lecule decompositio n processes .

Fro m the re sults obta in ed with the C:,HH' C:,OH (1: 1) mixture, and with CO"CH,CO", de tai ls of th e ion-molecul e reac tion mechan isms a nd th e unimolec ular decomposition of the propa ne ion a re de rived .

Key word s : Ion-m olecul e reac tio n; photoionization; propan e ; q uantum yields ; ra re-gas reso nance

radiation ; unimo l e~ ul ar dissoc ia ti on .

1 . Introduction

In the past , most photolysis studi es in the vacuum ultraviolet region have been carried out at e nergies be­low 11.8 eV (104.8 nm). The lamps commonly used in this e nergy region are rare gas resonance lamps, which deliver the resonance lines of xenon (8 .4 eV, 147.0 nm), krypton (10.0 eV, 123.6 nm), or a rgo n (11.6- 11.8 eV, 106.7- 104.8 nm). Higher energy resonance lamps could not be made because of the lack of suitable windows which would transmit photon s above 11.8 eV in e nergy. Recentl y, in thi s laboratory, enclosed neon a nd helium lamps h ave been fabri cated; their opera­tional characteristics have been described in detail [1]. t These lamps, whic h deliver the neon and helium resonance lines (16.7- 16.8 e V and 21.2 e V, respec­tively), are fitted with windows made of thin (2000 - 4000 A) film s of aluminum.

Photolysis studies in thi s high energy region are, of course , still very rare. Only a few studies, limited in

*S upporl cd in pa rt by the U.S. At omic Ene rgy Com mission , Washington, D. C. 20545 I Figures in bracke ts indica te the lite rature re fe rences at the end of thi s paper.

scope, of the che mical effects brought about in me th­ane [2- 4] and in argo n-propane mixtures [5] by helium resonan ce radiation have been published. One of th ese studies [2] was carri ed out with a differe ntially pumped windowless helium lamp; under such conditions, the investigator is restricted to a low pressure range. No studies at pressures above the millitorr range utilizing neon resonance radiation have so far appeared in the literature.

This paper re ports the results of a study where, for the first time, a compound is exposed to both neon and helium resonance radiation , and th e che mical effects at the two energies are compared. Propane was c hosen as the subject compound because the unimolecular and bimolecular (ionic and free radi cal) processes oc­c urring in this system have been extensively inves ti­gated [6] and are well und erstood. In the high e nergy region used in this study, chemical effects will be brought about nearly exclusively through ionic proces­ses. A comparison of the effects brought about by photons of two different energies may highlight subtle differences , and, therefore, increase our understanding

607

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of the activation processes in the high energy range. These results should also be of value in interpreting results obtained in systems exposed to high energy radiation (x rays, gamma rays, energetic electrons, etc.) where end product formation is brought about not only through ionic processes similar to those observed here, but also through the unimolecular decomposition of superexcited molecules.

2. Experimental Procedure

The reaction vessel and the resonance lamps used in this study have been described before [lJ. Both the neon and helium resonance lamps were provided with 2000 A aluminum windows which were entirely leak·free, and could withstand a pressure differential between the reaction vessel and the interior of the resonance lamp of 100 torr or more. At the start of the study the photon flux of the helium and neon resonance lamps was, respectively , 5 X 1013 and 7 X 1012 quanta/so It was ascertained that the helium and neon lamps were essentially monochromatic throughout the study by introducing neon and helium, respectively, into the first compartment of a double cell arrangement described before [1]. It was ascer­tained that neon gas placed in the sample cell absorbed the neon resonance radiation and was transparent to the radiation emanating from the helium lamp , while helium was trans parent to the photons from the neon lamp and absorbed those from the helium lamp. In the course of an experiment, either at the neon or the helium line, the decay in the light flux was no more than five percent from beginning to end.

The analytical procedures, as well as the purifica­tion of the materials used in this study, have been described [7J.

In most experiments, quantum yield determinations of the end product were made which were based on saturation ion currents measured periodically during the course of an irradiation [1, 7]. In these experiments, approximately 15 torr of a nonabsorbing inert gas (helium in the neon resonance line experiments, and vice versa) was added; it has been shown that the addition of such an inert will generally improve the definition of the plateau of the saturation ion current [1 , 81, and therefore lead to a more accurate determi­nation of the quantum yields of the end products formed in the photolysis.

Allene and methylacetylene were noted as products at 8.4 to 11.8 e V, but their quantum yields were not determined.

3. Results and Discussion

3 .1. Units

In a photolysis experiment carried out at an energy below the ionization energy of the compound of inter­est, a quantum yield of a given product, <1>, is simply the probability that the particular product will result when an excited molecule undergoes unimolecular de-

608

composition in the system under a particular set of con­ditions. In photoionization experiments, where some quanta produce ions, it has been found convenient in the past [7] to use two systems of units depending on whether a process involving a neutral excited molecule or an ionic process is being considered. Thus, the yields of products resulting fron nonionic processes were expressed in units of M(X)/Nex' or molecules M of product X formed per neutral excited molecule dis­sociating in the system, Nex; for photolysis in the sub­ionization region M(X)/Nex is simply the quantum yield. Ionic product yields, on the other hand, have generally been expressed in ion pair yield units, that is, as M(X)/N + , or molecules M of product X formed per positive ion formed in the system, N + _

Experimentally, an ion-pair yield is easily measured since N+ is directly determined by measuring the saturation ion current:

N+ = 1 X t(s)X6.24xlOI8 ions/C

(where 1 is the saturation ion current in amps and C is coulombs). If the quantum yield of ionization, <1>+, is known, then M(X)/Nex can be determined from the relationship:

The overall quantum yield is thus:

In this paper, we are concerned mainly with results obtained at very high energies where all, or almost all, product formation results from ionic processes; under these conditions the quantum yields and ion pair yields are essentially identical. The products formed at these energies are, however, compared with products observed in the photolysis at lower energies. All product yields are expressed in quantum yield units. Thus, in the 8.4 and 10.0 e V experiments , no ionization occurs, and there is no complication about the yield units. At 11.6-11.8 eV, on the other hand, only 73 percent (table 1) of the quanta absorbed lead to neutral excited molecule formation. Therefore, an

TABLE 1. Ionization quantum yields and extinction coefficients of propane a

Photon energy E cm-1atm - 1 cf>+

11.6-11.8 e V n.d. 16.7-16.8 e V 2950

21.2 eV 2240

" Arg-on lamp : 70 percent 11.6 eV, 30 percent 11.8 eV. b C. E. Kiois . to be published.

0.27 b

1.00 0.93

Page 3: The photochemistry of propane at high photon …The Photochemistry of Propane at High Photon Energies (8.4-21.2 eV) * R. E. Rebbert, S. G. Lias, and P. Ausloos Institute for Materials

estimation of th e probability that the deco mpos ition of the superexcite d propane molecule formed at thi s energy would lead to the form a tion of a given produ ct re quires that th e overall quantum yie lds be divided by 0.73; th e quantum yields can be trans lated into ion pair yie ld s, if the product of inter es t is of ionic origin , b y dividing by 0.27.

3.2. Ionization Quantum Yields

In table 1 are given the extinc tion coe ffi c ie nts and ionization quantum yields of propane at th e argon, neo n , and helium resonan ce lines, 11.6- 11.8 e V (106.7-104.8 nm), 16.7- 16.8 eV (74.4-73.6 nm) and 21.2 eV (58.4 nm), res pective ly [8]. It is noteworth y that wh en the photon ene rgy is inc reased fro m 11.6-11.8 e V to 16.6- 16.7 e V, the quantum yield of ionization increases from 0.27 to a value of unit y, but whe n the photon energy is furth er incre ased to 21.2 e V , the quantum yield of ionization seems to decrease to a valu e lowe r th a n unit y. Th e valu e re ported for 21.2 e V is based on the sa turation ion c urrent meas ure· me nt s show n in fi gure 1. At thi s wavele ngth , hydrogen has an ioniza tion quantum yield of unit y [8- 10]; be· cau se a t the helium r esonance line, hydroge n has a low extinc tion coeffi cie nt [8, 9, 11] (€= 185) , the sat­uration current me asured in hydrogen has a well de· de fin ed plateau extending ove r a ra nge of several hundred volts (fi g. 1). Therefore, the h ydrogen satura­tion ion c urre nt is an ideal standa rd aga ins t whic h to co mpare saturat ion ion curre nts measure d in oth er co mpound s at the sa me light Aux. Und e r press ure con­ditions where all in cide nt photon s a re absorbed , the qu antum yie ld of ioniza tion of the unknown is given simply by the ratio of th e two pl atue u valu es of th e saturation ion c urre nt measure ments . As th e fi gure clearly s hows, the plateau of the satura tion ion c urrent me asured in propane at thi s e ne rgy is not as we ll defined as th a t for hyd rogen , but seems to fall below the plateau meas ured in h ydroge n.

A recent stud y from thi s labora tory [8] re ported that th e ioniza tion quantum yields of C I to C alka nes at the neon resonance lines (16.7-16.8 e V) are a ll unity. The appare nt drop in the importan ce of ioniza­tion in propane as the energy is rai sed to 21.2 ~ V is also observed in these other alkanes [12 , 13J. This

I is an interes ting observation whi ch, if correct , s ugges ts that in alkanes whic h have absorbed a 21.2 eV photon, superexcited s ta tes may be reached which dis sociate so rapidl y tha t decompos ition can co mpete with ioni ­zation. Over all product distributions s uch as th ose show n in the table do not, of co urse, in the mselves give us mu c h inform ation about photolytic mechan­isms. Additional inform ati on, such as that obta ined from de ute rium lab e ling experim e nts is required in order to trace the modes of formation of a give n prod ­uc t. S uc h e xperim e nts have de mon s tra ted [17- 19] that ne utra l excited propane molec ules undergo the followin g pri mary processes:

Cl H ~ --'> Ct HI; + CHt

--'> CH4 + C2H4

(1)

(2)

--'> Hz + CaHli

--'> CRI + C2H~

--'> H+ CaH7

i l--r !Tl llTl"lT

2.0 Hel ium Lamp (584i1)

Amps X 10 8

1.2

40 120 200 280 360 440 520 60 0 VOLTS

(3)

(4)

(5)

F«;U HE 1. Sa tu ra tion ion carrellts 1lIf'!lSI.II·('(1 i ll S torr of h ydrugen Ollrl ill 0 .2 torr ofC, HH ill th e presence 20 torr of helium , irradi!l /ed with th e 21.2 eV heliullI reSOll!ln ce line.

160 EFFECT OF CONVERSION

NEON LAMP 140

" .. '2 120 x Ul 100 w ..J

80 ::J 0 W ..J 60 0 :;;

40

24 32 QUANTA ABSORBED X 10. 15

F IGURE 2. Molecules of etha ne , meth ane, propylene, ond eth yle ll e form.ed in the 16.7- 16.8 eV /Ih otolysis oI (/ Ilropane·oxy{!en-he IiLLIII ( / .0 :0.03:8.3 ) m ixtllre at a total presSlI re oI28/orr, as ofllll ct io/l of th e /lllmber oIquol/to absorbed by th e propane.

3.3. Photolytic Product Yields

Figure 2 shows the number of molec ules of various lower h ydrocarbon products form ed as a fun c tion of th e n umbe r of 16.7- 16.8 e V quant a absor bed in a propane-oxygen-helium (l. 0 :0.03 :8.3) mixture at a propane pressure of 3 torr. Th e amounts of the metha ne, e th a ne, and e th yle ne produ cts form ed increase linearly with the n umber of photons absorbed. Propylene , on the other hand , does not show suc h a linear relationship. This behavior ma y be accounte d for by several fac tors. For instance, it has been s hown before [5] that one precursor of propylene in propane is the propyl ion, and this ion may re act with accumu­lated products at high conversions. Another plausible

609

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TABLE 2. Quantum yields of end products in the photolysis of C3Hs

Photon energy Propane Scavenger Methane Acetylene Ethylene Ethane Propylene

8.4 eV C3H, 0,

10 eV C;jH, 0,

11.6-11.8 eV C3H, 0,

16.7-16.8 eV C3 H, 0, NO

C3 D, 0, NO

21.2eV C:,H, 0, NO

C"D, 0, NO

Press ure = 3.0 torr.

explanation of the fact that the propylene yield drops off at high conversions is that propylene product may be removed by reaction with ions or H atoms in the system. It has been shown [15, 16] that H atoms add to propylene faster than to ethylene or acetylene. Apparently, at the relatively low pressures at which the experiments are carried out, oxygen is not a very effective interceptor of hydrogen atoms.

In table 2, the experiments were carried out under conditions where no more than 3 X 1015 quanta were absorbed by propane at a pressure of 3 torr in the reaction cell. Thus, the yields of propylene shown in table 2 have not been much affected by these second­ary processes.

Table 2 shows the quantum yields of products formed in C3Hs and C3Ds irradiated with 8.4, 10.0, 11.6-11.8, 16.7-16.8, and 21.2 eV photons in the presence of 5 percent O2 or NO added as a radical scavenger. As the photon energy is increased the amount of energy to be distributed among the frag­ments will be larger and secondary decompositions will become more prevalent. For instance the forma­tion of acetylene, whose quantum yield of production is seen to increase with energy from 8.4 to 11.6-11.8 e V, can be attributed to the decomposition of C2H4

and C:JH6 formed in primary processes 2 and 3 respec­tively. It is of interest that at 16.7-16.8 e V, where only ionic processes lead to end product formation, the quantum yield of acetylene is negligible (-0.001). This observation is not unexpected because as shown by Cermak and Herman [20] none of the fragmentation processes of the C4Ht ion formed by collision with metastable neon atoms yields C2H2 as a neutral prod­uct. Furthermore, there are no known ion-molecule reactions involving fragments from C;jHt which would ultimately result in the formation of C2 H2 [21-27].

Thus , the result that acetylene formation from ionic processes (i.e., in the 16.7-16.8 eV photolysis) in propane is negligible, confirms the assumption made earlier [18], that all acetylene formed in the radiolysis of propane has neutral excited propane molecules,

0.040 0.028 0.080 0.015 0.23

.115 .073 .22 .043 .17

.22 .22 .27 .0585 .13

.27 .001 .084 .46 .32

.29 .001 .072 .42 .36

.29 .001 .052 .43 .14

.27 .001 .060 .48 .23

.29 .018 .113 .37 .405

.27 .018 .13 .37 .40

.28 .023 .092 .41 .23

.31 .020 .095 .40 .24

rather than ions, as precursor. The estimate that the ratio of neutral excited molecule formation to ioniza­tion is 0.4 in the radiolysis of propane [18], based on this assumption is, thus, probably approximately correct.

Considering that acetylene formation can apparently all be ascribed to a neutral excited propane precursor, it is interesting that the yield of acetylene increases ten-fold when the photon energy is raised from 16.7-16.8 eV to 21.2 eV (table 3). This is in agreement with the tentative conclusion reached above, that at 21.2 eV as many as 7 percent of the activated species may dissociate as neutral excited molecules before an electron can be ejected.

It is of interest to note that according to the quantum yield data given in table 2, the probability of the elimination of an alkane from neutral excited propane (processes (1) and (2)) increases with the energy of the photon [28]. The increase probably occurs at the expense of the H2 elimination process (3). In a recent study on the far ultraviolet photolysis of ethane [29] a similar trend was seen. In that case, however, all molecular elimination processes decrease at the ex­pense of direct bond cleavage processes as the energy is increased further. Similar trends can be expected for propane. The data given in table 2 do not allow a more detailed analysis of the primary processes occurring in propane in the 8.4-11.8 e V energy range. Quantum yields of all free radicals have to be known as well. A partial analysis of the role of free radicals in the decomposition of neutral excited propane IS

given elsewhere [18,19,30,31].

3.4. Isotopic Labeling Experiments

In table 3 are given the isotopic distributions of the major lower hydrocarbon products formed in the photolysis of a CIHs·C3 DH (1: 1) mixture in the presence of a radical scavenger with 16.7-16.8 and 21.2 e V photons.

The product ethane is known [5, 27, 32] to be formed in the reactions of ethyl ions with propane:

610

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(6)

and in the ethylene ion reaction :

C2 D1 + CIHH ---'> C2 D4 H2 + CIHij. (7)

It can be es timated from the relative amounts of C2D5H and C2 D.,H2 form ed· in these ex perim e nts a t 16.7-16.8 eV, that abou t 75 percent of the ethane res ulted from th e e thyl ion reaction, and a bout 25 percent from the ethylene ion reaction. On thi s basis, since the e th yl ion does not unde rgo any alternate reactions with propane [27J we can estimate roughly that the ion pair yield of the e thyl ion in th e 16.7-16.8 eV photolysis of propane is about 0.32-0.34; the ion pair yield of thi s ion observed in the mass s pec trom etri c study in which propane ions were generated by colli· sion with metastable neon atoms [20] was 0.37. Us ing the same reaso ning, it can be estimated that at 21.2 e V, 89 percent of the ethane originates from the reaction of an ethyl ion precursor. This gives an approximate ion pair yield for the e thyl ion in the photo· lys is at 21.2 eV of - 0. 33; when CaHt ion s are gene rated in a mass spectrometer throu gh colli sion with me tas table helium atoms [20], th e ion pair yield of e thyl ions observed was 0.25.

TABLE 3. Photolysis of C3H8-C3DS (1 :1); isotopic compositions of products

Photon Ethanes Methanes Propyien es Ethyienes Energy

C,D. C, D,H C,D4H, CD"H/CD. C:, D, H/C, D. C,D"H/C, D

16.7·16.8eV l.00 0. 75 0.25 0.057 0.32 0.63

21.2 eV l.00 .95 .1 2 .051 .33 .46

Prescure = 3 tor r. S perc ent O2 added.

The yields of e thanes form ed in reac tions s uc h as 7 from ethyle ne ion precursors do not directly give us the yield of the ethylene ion , s ince thi s ion can also undergo an H- (or D- ) transfer reaction with propane:

(8)

to form an ethyl " radical, which in these experiments will be scave nged. However, in one experiment H2S was added to C lDH irradiated with 21.2 eV photons. In thi s syste m , the d euterated e thyl radical formed in reaction 8 will react with H2S to form CZD5H:

(9)

while all other e thane-forming reactions will give fully deuterated ethane, C2D6 . From the observed yield of C2D5H, it could be deduced that for an ethylene ion r'eacting with propane-ds, the ratio of D- /D2- transfer reactions is 0.9. This value is in reasonably good agree­ment with the results of Sieck and Searles [33], who recently ascribed a value of 0.8 to this ratio on the basis of results obtained in the NBS high pressure photoioni­zation mass spectrometer. (They found that the ratio

of H- /H2- transfer reactions for e thyle ne ions reactin g with C3HS was 1.15.) On thi s basis, we can estimate ion pair yields for the eth yle ne ion genera ted in the 16.7-16.8 eV photolysis or the 21.2 eV photol ysis of propane of about 0.22 and 0.08 , respectively. Th e corres ponding ion pair yields of e thyle ne ions gener· ated in a mass s pec trom ete r by colli sion with meta­;; tahle neon and helium ato ms are 0.20 a nd 0.17.

Because the me th ane formed in the photolysis of C3Hs-ClDs (1:1) mixture contains very little partially deuterated product, it must be formed almost exclu­s ively in the unimolec ular deco mpositions:

(10)

(11 )

Process (11) and/or furth er decomposition of C2H! form ed in process (10) must be of importan ce in vie w of the fact tha t the es timated quantum yields of CzH! are lower th an the quantum yield of molecular methane (table 2).

From studies on CD3CH2CD3 , the fragmentation of the propane ion to form an ethyle ne ion (process 10) is known to occur through two mechanis ms. The lower e nergy process (A.P. = 11.8 eV) [34J is a 1,3 elimination of methane from the propa ne ion:

(12)

and the hi gher energy process (A.P. = 12.2 eV) [34] is a 1,2 elimination:

It is of interes t the n that the observed ratio CD3H/ CD4

(table 4) indeed increases from 0.69 at 16.7-16.8 eV to 0.76 at 21.2 e V. In an earli er s tud y [34] , it was noted that CD3 CH2 CD! ion s generated by charge excha nge with Xe+ ions (12.1-13.4 eV) underwent processes 12 and 13 to gi ve a CD:lH/ CD4 ratio of 0.35.

Because the e thylene and propylene contain large fractions of partially deuterated products (table 3), it is evident th a t an important mode of formation of these products is bimolecular ion-molec ule reactions such as, for in stance:

TABLE 4. Photolysis ofCD3CH2CD:l ; isotopic composition of methane

Photon Energy CD"H/C D,

16.7- 16.8 e V 0.69

21.2 eV .76

Pressure = 3 torr. 5 percent O~ added.

C2D~ + CIHH ---'> C2 D:IH + CIH~

CIDt + CIHH ~ C3DSH + C3H t·

(14)

(15)

611

Page 6: The photochemistry of propane at high photon …The Photochemistry of Propane at High Photon Energies (8.4-21.2 eV) * R. E. Rebbert, S. G. Lias, and P. Ausloos Institute for Materials

Reaction 14 is thought to proceed through formation of a condensation ion , C5D3Ht, which will di ssociate to form other partially de ute rated eth ylenes besides C2D:!H [271. Reaction 15 is a simple hydride transfer reaction.

For a more detail ed discussion on the ne utral end· product res ulting from ion· molecule reactions we refer the read er to earli er studies [5, 18, 27 ,32,35].

4. References

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[31 Je nsen , C. A., and Libby, W. J., J . Che rn. Phys. 9,2831 (1968). [41 Rebbert , R. E. , and Aus loos, P., .J. Am. Che rn . Soc. 90 ,7370

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[1 7] McNesby, ./ . R .. and Okabe. H .. Advan. Photochem. 3, 157 (1964).

[1 8 1 Ausloos, P ., and Li as, S. G., J. Che rn . Phys. 44 ,521 (1966). [1 91 Ausloos, P. , and Lias , S. G., Be r. Bun. Phys ik. Chem. 72, 187

(1968). [201 Cermak , V. a nd Herm an , Z., Coil. Czechoslov. Che rn . Commun.

30,169 (1965). 1211 Ryan, K. R. . and Futre ll , J. H .. J. Che rn . Phys. 42, 819 (1965). [22] P ette rso n, E. , and Lindholm . E .. Arkiv . F ys ik 24, 49 (1963). 123] Munson, M. S. B., F ranklin. J L. , and Field. F. H .. J . Ph ys .

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G. G .. J . Che m. Ph ys. 41 ,2998 (1964). 125] Aquilanti , V . . a nd Volpi . G. C .. .1. Che m. Phys . 44, 2307 (1966). 126] Siec k. L. W .. a nd Futre ll . J H. , J. Che m. Ph ys . 45 ,560 (1 966). 127] Bone . L. I. , and Futrell . J. H. , J. Che m. Ph ys. 46, 4084 (1967). l28] At 11.6- 11.8 eV fragme nt ati on of the C,Ht ion may contribute

to the forma'tion of CHI . However at th e press ures used in thi s study. the llnimolecllia r deco mposition of C,Hii is e ntirely quenched.

129] Li as , S. G., Collin. G. J., Re bbert. R. E., and Aus loos. P ., .J. Che rn. Ph ys . 52 , 1841 (1 970).

[30] Vorache k . ./. H .. and Koob. R. D .. J . Ph ys. C he m. 74,4455 (1970).

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[32] Ausloos, P. , Li as. S. G. , and Sandoval. I. B. . Di sc. Farada y Soc. 36, 66 (1963).

[33] Siec k, L. W., a nd Searl es. S. K. , .1. Am. Che m. Soc. 92, 2937 (1 970).

[34] Futrell. J. H., and Tie rn an. T. 0. , J . Chern. Ph ys. 39, 2539 (1963).

[35] Bone . L. I. , Siec k. L. W .. and Futre ll , J . 1-1. , The Chemis try of Ioni za ti on and Exc itation. G. R. A. Johnson and G. Scholer. Eds .. Taylor and Fran c is Ltd .. London (1967).

(Paper 75A6- 692)

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