• Keine Ergebnisse gefunden

2 Task Elektronenspektroskopie

N/A
N/A
Protected

Academic year: 2022

Aktie "2 Task Elektronenspektroskopie"

Copied!
3
0
0

Wird geladen.... (Jetzt Volltext ansehen)

Volltext

(1)

Heiko Dumlich April 4, 2008

2 Task Elektronenspektroskopie

2.1 (Film thickness)

This task is about a thin metal film on a substarte.

a)

We are meant to determine the film thickness, from the measured intensities of If andIs. Therefore we first have to determine the intensities. We start withIs, which is given with:

Is=Is0 Z

0

eΛzssdz e

d Λf f

while Is0 ∝nsσs, Λss = Λs(Es) and Λf f = Λf(Ef). We use the substitutiony = Λx ⇔dx= Λdy therefore we get:

Is∝nsσse

d Λf fΛss

Z

0

dy e−y

The integration is simple and only gives a 1:

Is∝nsσse

d Λf fΛss

Now we can have a look atIf, while this one is given with

If ∝nfσf

Z d

0

e

z Λf f

which leads to:

If ∝nfσfΛf f

1−e

d Λf f

Now we can get the quotient of the intensities to find d:

If

Is

=

nfσfΛf f

1−e

d Λf f

nsσse

d Λf fΛss

which can be rearranged to:

d = Λf fln

1 + nsσsΛssIf

nfσfΛf fIs

dtherefore depends only on known quantities.

1

(2)

b)

To simplify this expression we assume, that the mean free path will be much bigger than the film thickness, meaning Λ≫d. We can simplify the expression, starting withIs

Is∝nsσse

d Λf fΛss

while we now haved≪Λf f we can expand to first order:

Is∝nsσsΛss

and forIf

If ∝nfσfΛf f

1−e

d Λf f

whiled≪Λf f, we can expand the exponential function (to second order, while first order would cancel the whole term):

e

d

Λf f ≈1− d Λf f

+O d

Λf f

2!

which leads to:

If ∝nfσfd

Now we can get the quotient of the intensities again in the simplified form to findd: If

Is

= nfσfd nsσsΛss

which can again be rearranged to:

d= Ifnsσs

Isnfσf

Λss

2.2 (Yield of photoelectrons in the high kinetic energy regime)

The law for the yield of photoelectrons in the high kinetic energy regime Ekin ≈~ω is given withY ∝(~ω)α. We are meant to determine the exponentα. We know that

Y ∝

Z z

0

dz I

∝ Λ∝E12

∝ σ∝E−3

this means

Y ∝E−3+12 ∝E52 or

Y ∝σ·Λ

We have a look at the figure called “Cross sections vs energy” in the lecture notes. We have three lines there, we will get an average value therefore:

2

(3)

line σe

c1s −(2.9±0.05) n1s −(3.0±0.05) o1s −(2.95±0.05) average −(2.95±0.03)

Therefore we were able to determine the exponent with σe=−(2.95±0.03). This first value seems to fit the expectation of−3 quite well, now the second graph leads to Λe = 0.5, which also fulfills our expectation.

We therefore find:

Y ∝(~ω)α∝(~ω)σee≈(~ω)52

3

Referenzen

ÄHNLICHE DOKUMENTE

Organizarea contabilităţii de gestiune şi calculaţiei costurilor pe baze ştiinţifice în întreprinderile din industria fierului şi oţelului asigură premisele pentru

12.— The redshift-space power spectrum recovered from the combined SDSS main galaxy and LRG sample, optimally weighted for both density changes and luminosity dependent bias

The results show that with regard to the overall carbon footprint we need to focus on an intelligent mix of powertrains that meets indi- vidual requirements and includes

Impact of the Economic Cycle on Gender Differences in Unemployment Rates As the previous discussion suggests, women’s higher unemployment rate may be related to economic

In particular, the Bernardian lesson, which Cziko develops into a cybernetic framework explaining aspects of behavior, is the strength of this book.. Cognition is no longer the

 We are sorry to note that the goods (ordered) have not arrived yet..  We are

• The quality of the data allows for analysing highly deformed structures, as found in the shear margins of ice streams. • The 3D horizons illustrate how the ice stream

Hammerschmidt (Hrsg.): Proceedings of the XXXII Intemational Congress for Asian and North African Studies, Hamburg, 25th-30th Augusl 1986 (ZDMG-Suppl.. century locally