Absolute yields of the exciton induced desorption at the surface of solid rare gases

Absolute yields of the photo-induced desorption at the surface of solid rare gases were studied in the excitonic excitation region. Both metastable and total desorption yields depend strongly on excitation energy and film thickness of rare gas solids. The absolute desorption yields and their depende...

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Hauptverfasser: Arakawa, I., Adachi, T., Hirayama, T., Sakurai, M.
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Veröffentlicht: Фізико-технічний інститут низьких температур ім. Б.І. Вєркіна НАН України 2003
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spelling irk-123456789-1288212018-01-15T03:03:59Z Absolute yields of the exciton induced desorption at the surface of solid rare gases Arakawa, I. Adachi, T. Hirayama, T. Sakurai, M. Electronically Induced Phenomena: Low Temperature Aspects Absolute yields of the photo-induced desorption at the surface of solid rare gases were studied in the excitonic excitation region. Both metastable and total desorption yields depend strongly on excitation energy and film thickness of rare gas solids. The absolute desorption yields and their dependence on film thickness were quantitatively reproduced by a simulation based on the diffusion of excitons in the bulk and the kinetic energy release by a cavity ejection mechanism and an excimer dissociation one followed by internal sputtering. 2003 Article Absolute yields of the exciton induced desorption at the surface of solid rare gases / I. Arakawa, T. Adachi, T. Hirayama, M. Sakurai // Физика низких температур. — 2003. — Т. 29, № 3. — С. 342-350. — Бібліогр.: 32 назв. — англ. 0132-6414 PACS: 71.35.-y, 79.20.La http://dspace.nbuv.gov.ua/handle/123456789/128821 en Физика низких температур Фізико-технічний інститут низьких температур ім. Б.І. Вєркіна НАН України
institution Digital Library of Periodicals of National Academy of Sciences of Ukraine
collection DSpace DC
language English
topic Electronically Induced Phenomena: Low Temperature Aspects
Electronically Induced Phenomena: Low Temperature Aspects
spellingShingle Electronically Induced Phenomena: Low Temperature Aspects
Electronically Induced Phenomena: Low Temperature Aspects
Arakawa, I.
Adachi, T.
Hirayama, T.
Sakurai, M.
Absolute yields of the exciton induced desorption at the surface of solid rare gases
Физика низких температур
description Absolute yields of the photo-induced desorption at the surface of solid rare gases were studied in the excitonic excitation region. Both metastable and total desorption yields depend strongly on excitation energy and film thickness of rare gas solids. The absolute desorption yields and their dependence on film thickness were quantitatively reproduced by a simulation based on the diffusion of excitons in the bulk and the kinetic energy release by a cavity ejection mechanism and an excimer dissociation one followed by internal sputtering.
format Article
author Arakawa, I.
Adachi, T.
Hirayama, T.
Sakurai, M.
author_facet Arakawa, I.
Adachi, T.
Hirayama, T.
Sakurai, M.
author_sort Arakawa, I.
title Absolute yields of the exciton induced desorption at the surface of solid rare gases
title_short Absolute yields of the exciton induced desorption at the surface of solid rare gases
title_full Absolute yields of the exciton induced desorption at the surface of solid rare gases
title_fullStr Absolute yields of the exciton induced desorption at the surface of solid rare gases
title_full_unstemmed Absolute yields of the exciton induced desorption at the surface of solid rare gases
title_sort absolute yields of the exciton induced desorption at the surface of solid rare gases
publisher Фізико-технічний інститут низьких температур ім. Б.І. Вєркіна НАН України
publishDate 2003
topic_facet Electronically Induced Phenomena: Low Temperature Aspects
url http://dspace.nbuv.gov.ua/handle/123456789/128821
citation_txt Absolute yields of the exciton induced desorption at the surface of solid rare gases / I. Arakawa, T. Adachi, T. Hirayama, M. Sakurai // Физика низких температур. — 2003. — Т. 29, № 3. — С. 342-350. — Бібліогр.: 32 назв. — англ.
series Физика низких температур
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fulltext Fizika Nizkikh Temperatur, 2003, v. 29, No. 3, p. 342–350 Absolute yields of the exciton induced desorption at the surface of solid rare gases I. Arakawa and T. Adachi Department of Physics, Gakushuin University, Mejiro, Tokyo 171-8588, Japan E-mail: ich.arakawa@gakushuin.ac.jp T. Hirayama Department of Physics, Rikkyo University, Ikebukuro, Tokyo 171-8501, Japan M. Sakurai Department of Physics, Kobe University, Nada, Kobe 657-8501, Japan Received December 10, 2002 Absolute yields of the photo-induced desorption at the surface of solid rare gases were studied in the excitonic excitation region. Both metastable and total desorption yields depend strongly on excitation energy and film thickness of rare gas solids. The absolute desorption yields and their de- pendence on film thickness were quantitatively reproduced by a simulation based on the diffusion of excitons in the bulk and the kinetic energy release by a cavity ejection mechanism and an excimer dissociation one followed by internal sputtering. PACS: 71.35.–y, 79.20.La 1. Introduction When the surface of a solid rare gas is irradiated with vacuum ultraviolet light, it can eject atoms and clusters in ground, electronically and vibrationally excited, or ionized states. A variety of desorption mechanisms have been proposed for each desorbed spe- cies and for the excitation energy region. Two types of mechanisms are known to play an essential role in the desorption induced by the excitonic excitation; a cav- ity ejection (CE) mechanism is due to the repulsive interaction between the excited atom with an inflated electron cloud and the matrix with a negative electron affinity and an excimer dissociation (ED) one is the dissociation of an excimer in the vicinity of the sur- face. The investigation of the desorption phenomena initiated by the excitonic excitation is one of the most powerful tools to reveal the dynamic characters of the exciton in rare gas solids [1]. The desorption of ex- cited neutral particles of Ne and Ar has extensively been investigated for two decades [2]; the close rela- tionship between exciton formation [3] and the detail of the desorption mechanisms [4] has been almost fully elucidated. On the other hand, the desorption mechanism of the ground state neutral, as well as its desorption yield, has not been clarified yet though it can safely be said that they are the main component in the desorbed species. We report the measured results on absolute yields of the metastable desorption and the total one which are induced by the excitonic excitation from the sur- faces of solid Ne, Ar, and Kr. We also show that the experimental results for Ne and Kr are satisfactorily reproduced by the simple model simulation of the desorption process. 2. Desorption mechanism The negative electron affinity of the matrix is known to be essential for the CE process to have a re- pulsive interaction between the excited atom and the surrounding ground state atoms. The metastables desorbed through the CE process were observed for the solid whose electron affinity EA is negative, namely, solid Ne (EA = –1.4 eV) and Ar (–0.4 eV), but not for solid Kr (0.3 eV) and Xe (0.5 eV) [5]. The kinetic energy Ek of the metastable desorbed through © I. Arakawa, T. Adachi, T. Hirayama, and M. Sakurai, 2003 the CE process is originated from the lattice distortion energy around the exciton, which can roughly be esti- mated from the difference between the excitation en- ergy Ex of the exciton and the excitation energy Eg of the corresponding state of an isolated atom in the gas phase [1]. The energy difference, Ex – Eg, is divided among three terms, Ek: the kinetic energy of a de- sorbing particle, Ecoh: the cohesive energy of an atom on the surface, and Elatt: the energy absorbed in the lattice [6]. It has been revealed that 30–70 % of the lattice distortion energy is transferred into the kinetic energy of the desorbing metastable from the surface exciton S1 of Ne and Ar [4]. It has been also experi- mentally studied by the molecular dynamic calcula- tion [7]. In the case of Ne, for example, Ek of the metastable which is desorbed by the first order surface exciton is 0.18 eV at the peak of the distribution, while the excitation energy Ex is (17.17±0.03) eV and Eg of the corresponding 2p53s states are 16.619–16.848 eV [8]. The excitation energy Ex of the bulk exciton B1 of Ne is (17.57±0.03) eV. Con- sidering the low cohesion energy, 0.019 eV, of Ne, the lattice distortion energy, Ex – Eg, of 0.9–0.7 eV is large enough to squeeze the excited atom out of a second or third underlying layer to vacuum. The squeezed excited atom may push overlying atoms for- ward. This internal sputtering process can result in a large total desorption yield of Ne. In solid Ar, though the lattice distortion energy is estimated at about 0.7–0.4 eV, the internal sputtering process must be less efficient because of its larger cohesion energy of 0.068 eV. Dissociative relaxation of a rare gas excimer in the gas phase yields the kinetic energy of about 1 eV [9]. It is known that the ED process in solid produces crys- tal defects [10]. If ED occurs in the surface vicinity of a rare gas solid, a large number of atoms in the surface layer will be released into vacuum by the internal sputtering process. 3. Experimental The experimental apparatus for the photostimu- lated desorption (PSD) study was settled at BL5B beam line in the UVSOR facilities of the Institute for Molecular Science, Okazaki, Japan [11–13]. A solid rare gas film was prepared on a platinum substrate at a temperature of about 6 K which was attached to a liq- uid helium cryostat in an ultra-high vacuum chamber with a base pressure below 10–8 Pa. The amount of the gas condensed on the substrate, the film thickness, was calculated from the exposure, which was the product of the pressure and the duration of deposition, assuming the condensation coefficient to be unity. The wavelength resolution, � ��/ , of the vacuum ultraviolet light source was about 500 ± 200 in the range of � between 20 and 100 nm. The light intensity was monitored by the photoelectron current from a gold plated mesh, through which the light beam was introduced onto the sample surface. We adopted the value of 0.07 electrons/photon as the photoelectron yield at gold surface, which is the average value of the published data by Samson [14] between 52 and 100 nm of wavelength. The intensity of photon flux ranged between 1011 and 1012 photons/s in continu- ous mode and between 105 and 106 photons/pulse in pulse mode within a diameter of 3 mm at the sample. 3.1. Metastable desorption measurement The monochromatized photon beam is pulsed by a mechanical chopper in order to measure the time-of-flight (TOF) spectra of the desorbed metastable atoms. The width and the interval of the pulsed beam are 15 µs and 2.5 ms, respectively. The photon beam is incident at 20 deg of the normal direc- tion of the sample surface. The desorbed metastable atoms are detected by an open electron multiplier tube (EMT, Hamamatsu, R595) with a CuBe dynode as a first electrode. The EMT is fixed at a distance of 360 mm from the sample in the normal direction of the sample. The diameter of the entrance of EMT is 8 mm, which corresponds to the detection solid angle of 3.1·10–5 sr. The lifetimes of the metastable (3P0,2) rare gas atoms are known to be much longer than the flight time of the detected atoms which is less than 1 ms in our experimental sys- tem. The charged particles are rejected by applying suitable voltages to the grid mesh in front of the de- tector and the 1st dynode of EMT. In order to cal- culate the overall metastable yields, which were in- tegrated for all direction in half space, we utilized the angular distribution of the desorbed metastables which have already been reported by our group [15–17]. 3.2. Total desorption measurement The total desorption rate was calculated from the pumping speed and the rise of the partial pressure in the vacuum chamber during irradiation of the sample. The pumping speed of the turbo molecular pump and cold surfaces for desorbed rare gas was determined from the pressure measured by an extractor gauge in- stalled in the chamber and from the flow rate cali- brated volumetrically using a reference volume and a Baratron pressure gauge as a reference. A little rise of the partial pressure during irradiation was detected by a quadrupole mass spectrometer which was calibrated against the extractor gauge. It should be noted that Absolute yields of the exciton induced desorption at the surface of solid rare gases Fizika Nizkikh Temperatur, 2003, v. 29, No. 3 343 the uncertainty of the relative sensitivity of the ex- tractor gauge was cancelled in the present method of determining the desorption rate. 3.3. Accuracy of measurements In the metastable yield determination, the uncer- tainty of the results was estimated to be ± 30% by a quadrature sum of all sources of error; light intensity measurement, detection efficiency of the photomul- tiplier, geometrical configuration, etc. The main part of the error came from the estimation of the amount of higher order light from the monochromator [12,18]. The uncertainty in determining the absolute yield of the total desorption was estimated as large as ±1/3 of the order of magnitude; an error bar ranging from –50% to +100% of the obtained value should be added to the obtained values. In addition to the uncertainty in the intensity measurement of the incident photon, it was caused by difficulties in determining the sensiti- vity of the mass spectrometer and the pumping speed for the desorbed species. Noticeable changes in the desorption yields were observed after a few hours exposure of the sample in the chamber at a pressure of lower 10–8 Pa range, where the main component was a rare gas itself. It was probably due to the adsorption of the common resi- dual gases, H2, H2O, CO, in the UHV system [19,20]. The uncertainty caused by this impurity effect is within the above mentioned error bar in the present experiment. 4. Desorption of Ne 4.1. Experimental results The desorption yields of Ne metastable in the excitonic excitation region is shown in Fig. 1 as a function of incident wavelength. Most of the observed peaks in the figure can be assigned to a series of the bulk (B) and the surface (S) excitons reported by Saile and Koch [21], where S‘ peak is caused by the exciton in the 2p53p state which is allowed at the sur- face because of the reduced symmetry [22]. The four TOF spectra of the Ne metastable in Fig. 2 were ob- tained by the excitations at S1, B1, S’, and B2 excitons. The wavelength dependence of the absolute yield of the total photo-desorption in the range between 52 and 77 nm is shown in Fig. 3 for a film thickness of 73 atomic layers, where the peaks caused by the exciton excitation are also clearly seen. The absolute value of the desorption yield in the figure represents the aver- age number of the Ne atoms desorbed by one incident photon. The large and continuous background was due to the desorption induced by ionization by the second 344 Fizika Nizkikh Temperatur, 2003, v. 29, No. 3 I. Arakawa, T. Adachi, T. Hirayama, and M. Sakurai 7570656055 Wavelength, nm S1 B1 S' B2 Eg N e In te n si ty , ar b . u n its * Fig. 1. The desorption yields of the Ne metastable in the excitonic excitation region as a function of incident wave- length. 8006004002000 Flight time, µs B1 S' B2 Photon B A C D S1 In te n si ty , ar b .u n its Fig. 2. The time-of-flight spectra of the metastable Ne desorbed by the excitation of the four types of excitons. 2.0 1.5 1.0 0.5 0.0D es o rp t i o n y ie ld ,a to m s/ ph ot on 75706560 Wavelength, nm S1 B1 S' B2 B3 73 atomic layers Fig. 3. The absolute yields of the total desorption of the Ne in the excitonic excitation region as a function of incident wavelength. or higher order light from the monochromator. The peaks caused by the bulk excitons, B1 and B2, develop at the film thickness of a few tens atomic layers and the absolute yields seem to be saturated at around 1.6 and 1 atoms/photon, respectively, for the film thicker than 100 atomic layers. The peak heights due to the surface excitons seem to keep constant values of about 0.3 and 0.1 atoms/photon for S1 and S’, respec- tively, over the entire thickness range as expected for the surface excitations. The absolute yields of the metastable and the total desorption by the four differ- ent excitonic excitations are summarized in Table. 4.2. Schematic model of the desorption process The mechanism which works in each desorption process and the branching ratio of the relaxation cas- cade which leads to the desorption can be deduced from a careful examination of the TOF spectra of the metastables and the absolute yields of the metastable and the total desorption. The mechanisms which work in the desorption process are also listed in Table. The higher kinetic energy peak A (Ek = (1.4± ±0.1) eV) [23] in Fig. 2, which is only observed by the excitation of the higher order excitons (S‘ and B2), is caused by the excimer dissociation of the highly excited dimer: Ne2** � Ne + Ne* + Ek. This is also the case for Ar [24]. The lower kinetic energy peak, that is CE one, is obviously composed of two components B (Ek = (0.21±0.02) eV) and C (Ek = = (0.18±0.02) eV) [12]. The metastables which com- pose the peaks B and C are ejected directly from the surface excitons S‘ and S1, respectively [15]. The dif- ference in the kinetic energy is caused by the differ- ence in the magnitude of the repulsive interaction. The low energy tail D is only observed by the bulk ex- citations (B1 and B2) [15] and is likely caused by the bulk exciton trapped in the underlying layer just be- low the surface. They are ejected into the vacuum, loosing their kinetic energy by collision with atoms in the overlayer. These TOF spectra can be used as a fin- gerprint to identify each exciton. These spectra also show clearly the relaxation channel of the excitons Absolute yields of the exciton induced desorption at the surface of solid rare gases Fizika Nizkikh Temperatur, 2003, v. 29, No. 3 345 Table The absolute yields of the metastable and the total desorption from solid Ne, Ar, and Kr Rare gases Initial excitation Desorbed species Yield, atoms/photon Desorption mechanisms Ne S1 metastable (2.3 ± 0.7)·10–3 CE total 0.3 CE + S/CE(?%) + S/ED(?%) S’ metastable (7.8 ± 2.3)·10–4 CE + ED(� 1%) total 0.1 CE + S/CE(?%) + S/ED(?%) B1 metastable (1.4 ± 0.4)·10–3 CE + S/CE(a few %) total 1.6 ± 0.3 S/CE + CE(� 10%) + S/ED(a few %) B2 metastable � 1·10–3 CE + S/CE(a few %) + ED(� 1%) total 1 ± 0.2 S/CE + CE(� 10%) + S/ED(a few %) Ar S1 metastable � 1·10–5 CE total 0.1 CE S2 metastable not determined CE + ED total 0.1 CE B1 metastable not determined CE total 0.23 CE + S/ED B2 metastable not determined CE + ED total 0.16 CE + S/ED Kr S1(3/2) total 0.015 S/ED S1(1/2) total 0.01 S/ED S2(3/2) metastable not determined ED total � 10–3 S/ED B1(3/2) total 0.03 S/ED B1(1/2) total 0.02 S/ED B2(3/2) metastable not determined ED total � 10–3 S/ED from the higher energy state to the lower one; from B1 to S1, from S‘ to S1 and excimer, and from B2 to S’, S1, and excimer. The quantum efficiency of the exciton creation can be estimated from the photo-absorption coefficient of solid Ne at the wavelength corresponding to the bulk exciton (B1) excitation. We assume here that the ex- citation probability of S1 is the same as that of B1 in each layer at their own excitation energy. The estima- tion based on the data by Pudewill et al. [25] leads to the value of 0.1 excitons/photon in each layer. The relaxation cascade of the first order surface exciton S1 of solid Ne is schematically shown in Fig. 4. Incident light of the wavelength of 72.2 nm will excite surface excitons with the probability of 0.1 excitons/photon in the first layer. 90% of the incident photons pass through the solid Ne film and will be scattered or absorbed at the substrate. The surface exciton may decay radiatively or may be desorbed by the CE mechanism as a metastable in 3P2,0 state or as an excited atom in 3P1 or 1P1 state which decay into the ground state with a short lifetime of 1–10 ns. In our study, we have determined the absolute yields of the metastable desorption, 0.0023 Ne*/photon, and of the total desorption, 0.3 Ne/photon. Considering the absolute total desorption yield at S1 excitation of 0.3 atoms/photon, the value, 0.1 excitons/photon, of the initial excitation probability must be underesti- mated since it is likely that a surface exciton can be desorbed only a single excited atom in the CE process. The larger desorption yield may be explained by other desorption processes: the desorption of a dimer by the CE process and the ED process which yields two or more desorbing atoms. However, the branching ra- tio to these two processes must be far smaller than that to the single atom desorption by the CE process. Another possibility is the excitation by the light re- flected at the substrate surface. If this is the case, the initial excitation probability doubles at most. In any case, it can be concluded that almost all the surface excitons yield the desorption of one Ne atom or, in other words, that the desorption probability of the surface excitons S1 is almost unity. The comparison between the metastable desorption yield and the total one shows that about 1% of the desorbed Ne atoms are in the metastable state. The above-mentioned scheme cannot be applied to the analysis of the desorption yield caused by S‘ exci- tation because the quantum efficiency for S’ creation cannot be estimated in the same manner; the excita- tion of 2p53p state is only allowed at the surface of the solid. It can be said from the comparison between the total desorption yields by S‘ and by S1, if we assume that the desorption probability of S‘ exciton is also unity, that the excitation cross section of S‘ is one third of that of S1. The metastable TOF spectrum by S‘ excitation shows that almost two thirds of S‘ exciton decays into S1 state at the surface before the desorption and that a few % of S‘ forms excimers in a higher excited state. It is also worth noting that the ratio of the number of the metastable species to the to- 346 Fizika Nizkikh Temperatur, 2003, v. 29, No. 3 I. Arakawa, T. Adachi, T. Hirayama, and M. Sakurai photon 72.2 nm ~ 0.1 ~ 0.9 S1 exciton radiative decay 3P2,0 3 P1 , 1 P1 Y META � � 0.0023 Ne*/photon Y TOTAL 0.3 Ne/photon Fig. 4. Schematic chart of the relaxation cascade of the first order surface exciton S1 in solid Ne. tal number of desorption events is about 1% also in the case of S‘ excitation. The relaxation cascade of the first order bulk exciton B1 of solid Ne are schematically shown in Fig. 5. When solid Ne is irradiated by 70.5 nm pho- tons, the probability for the bulk exciton creation in the second underlying layer is estimated at 0.1 exci- tons/photon, 0.09 in the third layer, and 0.1(1–0.1)(n–2) in the nth layer. Radiative decay may occur immediately or on the way of migration in the bulk. Some of them may reach the surface and convert into the surface exciton S1, which will follow the scenario in Fig. 4. The experimentally determined value of the meta- stable yield, 0.0014 Ne*/photon, via S1 state sug- gests that the total desorption yields via S1 excitons are about 0.2 atoms/photon considering the ratio of the total yield to the metastable one in the case of S1 excitation. This means that the conversion rate from B1 exciton to S1 exciton is 0.2. The excited atom in the second or third layers can be squeezed out because of the large lattice distortion and can blow a number of atoms in the surface layer away. The desorption of metastable Ne from the underlying layers, which losses the kinetic energy by collisions with neutral at- oms in the overlayers, was experimentally identified in the TOF spectra of Fig. 2 as a tail D. The large de- sorption yields of the order of unity brought by the bulk exciton can be attributed to this internal sputter- ing mechanism by excited atoms in the second and deeper layers beneath the surface [7]. The TOF spectrum of desorbed metastables by the excitation of B2 exciton is quite similar to that by S‘ except the signal caused by a long life time (several hundreds �s) luminescence. The relaxation of B2 into S1, S’, and the excimer is clearly distinguished from the spectrum. Though the total number of excitons ex- cited by B2 excitation is essentially the same to that by B1 excitation, there is an obvious difference be- tween the total desorption yields by B1 and B2 excita- tions. This is probably because of the difference in the distribution of the initial excitation in the Ne film and because of the relaxation channel of B2, which yields the luminescence stated above. 5. Desorption of Kr 5.1. Metastable desorption The desorption of metastable species from solid Kr, which has been observed by electron and high energy Absolute yields of the exciton induced desorption at the surface of solid rare gases Fizika Nizkikh Temperatur, 2003, v. 29, No. 3 347 photon 70.5 nm � 0.1 � 0.1 0.9 � 0.1 0.9 (n –2) radiative decay B1 exciton S1 3P 2,0 3 P2,0 3 P 2,1,0 , 1 P 1 - - - - migration in solid �� Fig. 5. Schematic chart of the relaxation cascade of the first order bulk exciton B1 in solid Ne. ion bombardment, is attributed to the ED mechanism. However, it has been reported that adsorption of a small amount of hydrogen makes it possible to desorb metastables by the CE mechanism by changing the electron affinity into negative [26]. Because of this phenomenon, it is difficult to determine the absolute desorption yields of a metastable via the process in- trinsic of pure solid Kr. This is also the case for solid Xe. 5.2. Total desorption The wavelength dependence of the photo-de- sorption intensities from solid Kr for three different film thicknesses is shown in Fig. 6, where the curves are the direct output from the mass spectrometer with no compensation applied for a higher order light. The arrows show the wavelength corresponding to the ex- citation of the series of excitons in solid Kr. The coin- cidence between the exciton excitation energies and the peaks or the shoulders in the figure clearly shows that the excitons induce the desorption. The de- sorption yields were estimated by the peak height above the continuous background which was due to the bulk ionization caused by the higher order light from the monochromator. The desorption yield at S1(3/2) excitation has apparently no thickness de- pendence and is about 0.015 atoms/photon. The de- sorption by the bulk exciton creation becomes detec- table at a few tens atomic layers in our experimental condition. The desorption yields at B1(3/2) and B1(1/2) excitation increase with the film thickness and reach saturated values, 0.03 and 0.02 atoms/pho- ton, respectively, at a thickness of about 100 atomic layers. The absolute yields of the total desorption by the five different excitonic excitations are summarized in Table. 5.3. Desorption model and simulation of total desorption yields The desorption process caused by excimer dissocia- tion and internal sputtering after the bulk exciton ex- citation is considered as sequential processes as sche- matically shown in Fig. 7: i) creation of a free exciton, ii) migration of the exciton, iii) formation of an excimer, iv) dissociation of the excimer, and v) colli- sion cascade followed by internal sputtering. In order to calculate the desorption yields, each step should quantitatively be evaluated. The detail of the calcula- tion will be published elsewhere [27]. Though the be- havior of the exciton at a vacuum interface and metal substrate is not well understood, the photoemission data of Kr were well described by assuming that the metal surface is a perfect sink and that the vacuum in- terface is a perfect reflector for the exciton [28]. The final process v), which is one of the most important factors to give the theoretical desorption yields, has extensively been studied by a classical molecular dy- namic simulation [7]. A distribution of the initial ex- citation in the process i) and a diffusion length in the migration ii) affect the depth profile of the distribu- tion of the trapped excimer and, therefore, determine the film thickness dependence of the total desorption yield. The initial distribution of the excited bulk excitons is estimated from the photo-absorption coeffi- cient [29]. The only unknown parameter is the diffu- sion length L of the free exciton, which is expected to be highly affected by crystal condition and tempera- ture. As is shown in Fig. 8, both the absolute value and the thickness dependence were satisfactorily re- produced by choosing the parameter L between 5 and 10 nm. This value shows good agreement with the esti- mation between 1 and 10 nm by Schwentner et al. 348 Fizika Nizkikh Temperatur, 2003, v. 29, No. 3 I. Arakawa, T. Adachi, T. Hirayama, and M. Sakurai 125120115110105 Wavelength, nm B2(1/2) B2(3/2) S2(3/2) S1(3/2) 1200 atomic layers 10 atomic layers S1(1/2) B1(1/2) B1(3/2) 150 atomic layers D e so rp tio n yi e ld s, ar b . u n its Fig. 6. The total desorption yields as a function of inci- dent wavelength for three different thicknesses of Kr films. iii) i) iv) v) ii) Fig. 7. The model of sequential steps of the excimer disso- ciation process in solid Kr. from the photoemission study [28]. We have also ap- plied this method of simulation to the ESD case of solid Kr and obtained satisfactory results [27]. Though we assume that the CE mechanism does not work at the surface of solid Kr, the surface exciton ex- citation resulted in significant total desorption. This may be caused by the excimer dissociation on the sur- face. However, we cannot exclude the effect of hydro- gen adsorption which makes the CE process effective. 6. Desorption of Ar The desorption of metastables from solid Ar by both CE and ED mechanisms has been reported by many researchers [24,30,31]. There are some experi- mental difficulties, however, in determining the abso- lute yields of Ar metastable; unknown angular distri- bution of desorbed Ar, low signal intensity, and unstable detection efficiency of a secondary electron multipliers. Nevertheless we have obtained a rough es- timation of the absolute metastable yield of 1·10–5 atoms/photon by S1 excitation [12]. Though the de- termination of the absolute yields of total desorption has already been made in the same way as for Kr (see Table) the comparison between the experimental re- sults and the simulation is not so straightforward as in the Kr case. It is expected for solid Ar that both CE and ED mechanisms contribute to the total desorption in comparable measure. The model calculation of the total yield at B1 excitation, in which only the ED mechanism is assumed under conditions similar to the Kr case, gives a theoretical desorption yield of almost one tenth of the experimental value. This large dis- crepancy is probably because the bulk excitons are ef- ficiently converted to the surface ones at the vacuum interface and they are desorbed by the CE mechanism. The model simulation which takes both CE and ED mechanisms into account is under progress. 7. Summary We have measured the absolute yields of metastable and total desorption at the surface of solid Ne, Ar, and Kr by the photostimulated desorption technique. The experimental results are well ex- plained by the model in which the excitons play a cru- cial role. However the mechanism which leads to the desorption for each rare gas is different. For solid Ne, the predominant mechanism which works for both metastable and total desorptions is the CE one. The large lattice distortion energy makes the internal sput- tering process possible and results in a large total desorption yield of the order of 1 atoms/photon by bulk exciton excitation. For solid Kr, the desorption process can be well described solely with the ED mechanism in which the migration of a free exciton be- fore trapping into the excimer state determines the ab- solute yields and its film thickness dependence. In solid Ar, both CE and ED mechanisms work for the desorption, which make the model calculation of the desorption yield difficult. The mechanism which works in the desorption process from solid Xe must be solely the ED one as is the case for solid Kr. Unfortu- nately, we have not obtained the data on absolute to- tal desorption yields which can be compared with the simulation result. This is because of the experimental difficulty due to the low desorption signal intensity and the limitation of our experimental apparatus. It was demonstrated that the desorption study could reveal the dynamics of excitons in rare gas solids. The promising step in the future study may be a sys- tematic investigation of the temperature dependence of the desorption phenomena on a well defined sample crystal. The desorption study at the surface of a rare gas alloy [32] will also yield interesting information on the dynamics of the exciton in a heterogeneous system. Acknowledgment This work was supported by the Joint Studies Pro- gram of the Institute for Molecular Science and partly by a Grant-in-Aid for Scientific Research from the Ministry of Education, Science, Sports, and Culture, Japan. Absolute yields of the exciton induced desorption at the surface of solid rare gases Fizika Nizkikh Temperatur, 2003, v. 29, No. 3 349 0.08 0.06 0.04 0.02 0.00 10 100 1000 Thickness of Kr film, atomic layers 1nm 5nm 10nm 50nm Diffusion length L A b so lu te d e so rp tio n yi e ld s, at o m s/ p h o to n Fig. 8. Thickness dependence of the total desorption yield of solid Kr; the experimental results (solid square) and the simulated ones (lines) for the diffusion length as a pa- rameter. 1. I. Arakawa, Mol. Cryst. Liq. Cryst. 314, 47 (1998). 2. F. Colletti, J.M. Debever, and G. Zimmerer, J. Phys. Lett. 45, 467 (1984). 3. P. Feulner, T. Muller, A. Puschmann, and D. Menzel, Phys. Rev. Lett. 59, 791 (1987). 4. T. Kloiber and G. Zimmerer, Radiat. Eff. Def. Sol. 109, 219 (1989). 5. N. Scwentner, F.-J. Himpsel, V. Saile, M. Skibowski, W. Steinmann, and E.E. Koch, Phys. Rev. Lett. 34, 528 (1975). 6. D.E. Weibel, A. Hoshino, T. Hirayama, M. Sakurai, and I. Arakawa, in: Desorption Induced by Electronic Transitions DIET V, E.B. Stechel, A. Burns, and D.R. Jennison (eds.), Springer, Berlin (1993), p. 333. 7. S. Cui, R.E. Johnson, and P.T. Cummings, Phys. Rev. B39, 9580 (1989). 8. N.E. Small-Warren and L.-Y. Chow Chiu, Phys. Rev. A11, 1777 (1975). 9. T.R. Connor and M.A. Biondi, Phys. Rev. A140, 778 (1965). 10. I.Ya. Fugol’, O.N. Grigorashchenko, A.N. Ogurtsov, and E.V. Savchenko, J. Luminescence 53, 517 (1992). 11. M. Sakurai, T. Hirayama, and I. Arakawa, Vacuum 41, 217 (1990). 12. T. Hirayama, A. Hayama, T. Koike, T. Kuninobu, I. Arakawa, K. Mitsuke, M. Sakurai, and E.V. Sav- chenko, Surf. Sci. 390, 266 (1997). 13. I. Arakawa, T. Adachi, T. Hirayama, and M. Sakurai, Surf. Sci. 451, 136 (2000). 14. J.A.R. Samson, J. Opt. Soc. Am. 54, 6 (1964). 15. I. Arakawa, D.E. Weibel, T. Nagai, M. Abo, T. Hi- rayama, M. Kanno, K. Mitsuke, and M. Sakurai, Nucl. Instrum. Meth. Phys. Res. B101, 195 (1995). 16. M. Sakurai, T. Nagai, M. Abo, T. Hirayama, and I. Arakawa, J. Vac. Soc. Jpn. 38, 298 (1995). 17. D.E. Weibel, T. Hirayama, and I. Arakawa, Surf. Sci. 283, 204 (1993). 18. M. Sakurai, T. Adachi, T. Hirayama, and I. Arakawa, UVSOR Activity Report 2001, UVSOR-29, 58 (2002). 19. T. Kuninobu, A. Hayama, T. Hirayama, and I. Ara- kawa, Surf. Sci. 390, 272 (1997). 20. A. Hayama, T. Kuninobu, T. Hirayama, and I. Ara- kawa, J. Vac. Sci. Technol. A16, 979 (1998). 21. V. Saile and E. E. Koch, Phys. Rev. B20, 784 (1979). 22. K. Inoue, H. Sakamoto, and H. Kanzaki, Solid State Commun. 49, 191 (1984). 23. T. Hirayama, T. Nagai, M. Abo, I. Arakawa, K. Mit- suke, and M. Sakurai, J. Electr. Spectr. Rel. Phen. 80, 101 (1996). 24. I. Arakawa and M. Sakurai, in: Desorption Induced by Electronic Transitions DIET IV, G. Betz and P. Varga (eds.), Springer, Berlin (1990), p. 246. 25. D. Pudewill, F. Himpsel, V. Saile, N. Schwentner, M. Skibowski, and E.E. Koch, Phys. Status Solidi B74, 485 (1976). 26. Hayama, T. Kuninobu, T. Hirayama, and I. Arakawa, J. Vac. Sci. Technol. A16, 979 (1998). 27. T. Adachi, T. Hirayama, T. Miura, I. Arakawa, and M. Sakurai, Surf. Sci. (to be published). 28. N. Schwentner, G. Martens, and H.W. Rudolf, Phys. Status Solidi B106, 183 (1981). 29. B. Sonntag, in: Rare Gas Solids, vol. II, M.L. Klein and J.A. Venables (eds.), Academic, New York (1977). 30. D.J. O’Shaughnessy, J.W. Boring, S. Cui, and R.E. Johnson, Phys. Rev. Lett. 61, 1635 (1988). 31. I. Arakawa, M. Takahashi, and K. Takeuchi, J. Vac. Sci. Technol. A7, 2090 (1989). 32. D.E. Weibel, T. Nagai, T. Hirayama, I. Arakawa, and M. Sakurai, Langmuir 12, 193 (1996). 350 Fizika Nizkikh Temperatur, 2003, v. 29, No. 3 I. Arakawa, T. Adachi, T. Hirayama, and M. Sakurai