HAL Id: jpa-00221340
https://hal.archives-ouvertes.fr/jpa-00221340
Submitted on 1 Jan 1981
HAL is a multi-disciplinary open access
archive for the deposit and dissemination of
sci-entific research documents, whether they are
pub-lished or not. The documents may come from
teaching and research institutions in France or
abroad, or from public or private research centers.
L’archive ouverte pluridisciplinaire HAL, est
destinée au dépôt et à la diffusion de documents
scientifiques de niveau recherche, publiés ou non,
émanant des établissements d’enseignement et de
recherche français ou étrangers, des laboratoires
publics ou privés.
TIME CONSTANT FOR PHONON INDUCED
DESORPTION OF HELIUM
P. Taborek, M. Sinvani, M. Weimer, D. Goodstein
To cite this version:
JOURNAL DE PHYSIQUE
CoZZoque CF, suppllment au n o 12, Tome 42, dlcembre 1981 page C6-852
P. Taborek, M. Sinvani, M. Weimer and D. Goodstein
California I n s t i t u t e o f Technology, Pasadena, CA 91125, U.S. A .
Abstract.- We have made d i r e c t measurements o f the t i m e constant f o r thermal d e s o r p t i o n o f t h i n helium f i l m s as a f u n c t i o n o f s u b s t r a t e temperature and
f i l m b i n d i n g energy. We f i n d t h a t t h e attempt frequency f o r desorption
T ~ i s several orders o f magnitude l a r g e r than p r e v i o u s l y r e p o r t e d values. - ~
Phonons impinging on a s o l i d s u r f a c e which i s covered w i t h a helium f i l m can
cause some o f t h e atoms t o be e j e c t e d . The physics o f t h i s process i s important f o r an understanding o f the dynamics o f desorption and energy t r a n s p o r t a t s o l i d /
helium i n t e r f a c e s . We have used pulsed phonon techniques t o study t h e r a t e of
d e s o r p t i o n from a nichrome surface. The experimental apparatus c o n s i s t s o f a
r e c t a n g u l a r t h i n f i l m nichrome heater deposited on a sapphire c r y s t a l which forms
the bottom o f a vacuum can (see F i g . 1, i n s e t ) . A superconducting t r a n s i t i o n
bolometer w i t h a thermal response time o f
-
10 nsec i s mounted-
1m
above theheater. By a d m i t t i n g known q u a n t i t i e s o f helium gas, t h e thickness o f the f i l m
which covers a l l t h e surfaces i n t h e c e l l can be c o n t r o l l e d i n t h e range 1-3
l a y e r s . The ambient temperature i s 3.5 K and the pressure i s always s u f f i c i e n t l y
low t h a t t h e atoms t r a v e l b a l l i s t i c a l l y t o the d e t e c t o r . A c u r r e n t p u l s e w i t h a
F i g . 1 : Bolometer s i g n a l as a f u n c t i o n o f time f o r various heater pulse widths. Heater temperature = 6.2 K. The i n s e t shows t h e experimen- t a l geometry. 0 4 6 8 10
TIME
(psec)
'Supported i n p a r t by ONR Contract
#
N00014-80-C-0447I I I I I I I I I I
Pulse W ~ d t h ( p s e c )
I
F i g . 2 : Bolometer s i g n a l as a f u n c t i o n o f t i m e f o r v a r i - ous heater p u l s e widths.
Heater temperature = 8.1 K.
The p u l s e shape i s described
by Eq. 1. No f u r t h e r change
i n t h e s i g n a l i s observed f o r pulses l o n g e r than 1 psec.
known power and d u r a t i o n i s a p p l i e d t o t h e heater, which r a i s e s t h e heater tempera- t u r e and causes d e s o r p t i o n o f t h e f i l m ; t y p i c a l bolometer s i g n a l s a r e shown i n
Figs. 1 and 2. The temperature o f t h e heater f i l m i s a f u n c t i o n o f the power and
can be c a l c u l a t e d from a c o u s t i c mismatch theory(' ) and can a l s o be deduced inde-
pendently from t h e time o f f l i g h t o f the desorbed atoms. The c a l c u l a t e d tempera-
t u r e o f t h e nichrome f i l m and the measured temperature o f the desorbed atoms a r e i n
good agreement. Because t h e heater f i l m i s i n c o n t a c t w i t h a s i n g l e c r y s t a l sub-
s t r a t e , t h e heater temperature can be r a i s e d and lowered w i t h a t i m e constant of
-
10 nsec. When t h e heater temperature i s higher than t h e ambient, the number o fatoms/cm2 i n t h e helium f i l m n ( t ) r e l a x e s t o a new steady s t a t e value nss i n a c h a r a c t e r i s t i c time T.
For heater pulse widths .s T , t h e d e s o r p t i o n s i g n a l i s a s e n s i t i v e f u n c t i o n of t h e pulse width, b u t f o r l o n g pulses, t h e s i g n a l saturates. By s l o w l y i n c r e a s i n g t h e p u l s e w i d t h from a minimum o f 30 nsec, the p u l s e w i d t h which causes s a t u r a t i o n
i s e a s i l y observed. We have used t h i s technique t o measure T as a f u n c t i o n o f
f i l m thickness and heater temperature. T y p i c a l data shown i n Figs. 1 and 2 g i v e
T
-
1 usec f o r Theater = 6.2 X and T-
.2 usec f o r Theater = 8.1 X.Theories f o r the d e s o r p t i o n time T can be q u i t e complicated,(') b u t t h e
r e s u l t s can be described using a simple thermal a c t i v a t i o n model(3) T = T 0 eEbIT
where T~ i s a c h a r a c t e r i s t i c attempt frequency and Eb i s t h e b i n d i n g ener3y of
t h e atom t o t h e s u b s t r a t e . I n order t o comnare our r e s u l t s w i t h previous i n d i r e c t
experimental
measurement^(^)
and t h e o r e t i c a l c a l c u l a t i o n s ( ' ) i t i s necessary t omeasure an average Eb f o r t h e desorbed f i l m s . We have estimated Eb i n two inde-
C6-854 JOURNAL DE PHYSIQUE
temperature o f t h e s u b s t r a t e and t h e atoms desorb w i t h a Maxwellian d i s t r i b u t i o n . The expected bolometer s i g n a l has t h e form
w i t h v = E / t where
L
i s t h e d i s t a n c e t o t h e d e t e c t o r . Eb may a l s o be deduced from t h e chemical p o t e n t i a l o f t h e gas, which can be determined by measuring P and T. Using these methods we f i n d t h a t Eb 2 3 5 K f o r t h e data shown i n Figs. 1 and 2.From
r
= ro eEb/T, we f i n d ro<
5 xl o - '
sec, a t l e a s t two orders o f magnitudesmaller than t h e value deduced i n r e f e r e n c e (4) and explained i n reference (2). The technique used i n t h a t experiment i s very i n s e n s i t i v e t o t h e small t i m e
constants which a r e observed f o r heater temperatures above 6 K. Our measurements
are c o n s i s t e n t w i t h t h e i r data, b u t y i e l d much more p r e c i s e values of T i n t h i s
regime.
Keterences: 1. 0. Weis, Z. Ang. Phy.
26,
325, 1969.2. Z. W. Gortel, H. J. Kreuzer, and D. Spaner, J. Chem. Phys.
72,
234, 1980.
3. J. Frenkel, K i n e t i c Theory o f L i q u i d s , Dover, New York, 1946.