Download A Simple Model for Interpreting the Basics of Time Dependent Fluorescence Spectroscopy | PHYS 552 and more Study Guides, Projects, Research Optics in PDF only on Docsity! A simple model for interpreting the basics of time dependent fluorescence anisotropy Athanasius Kircher
Athanasius Kircher
(1602-1680) beschreibt in
seinem Buch »Ars Magna
Lucis et Umbme* die
Wirkung eines Holz
extrakts von Lignum ne-
phriticum in Wasser und
endrtert die Nutzung von
Glidhwitemchen als Haws
belewchrung.
Johann Wilhelm Ritter
(1776-1810) entdeckte
bein Experimentionn mit
Silberchloridan der
Universitit Jena 1801 das
ultraviolette Ende des
Spektrums,
Johann Wilhelm Ritter
Inseiner »Farberlehre®
beschreit auch Johann
von Goethe
(1749-1832) die fluoreszie-
renden Lichterscheinungen.
Er fordert die Laser auf»...
tauche ein frisches Stiick
Baumirinde der Rosskasta-
nie in ein Glas mit Wasser,
sofort erscheint eine rein
himmelblaue Fare.”
Johann Wolfgang v. Goethe
1602-1680 1776-1810 1749-1832
Der Erfinder des Kaleido-
shops, Sir David Brewster
(1781-1868), beschreibt
1833 die rote Strahlung
von Chlorophyll.
Sir David Brewster
1781-1868
1845 entdeckte Sir
John Frederick William
Herschel (1792-1871)
eee
Fluoreszenz in einer
Chininlisung.
Sir John Frederick William Herschel
1792-1871
Sir George Gabriel Stokes
Sir George Gabriel Stokes
(1819-1903) bezeichnet
1852 die Leuchterschei-
nung des Minerals Fluss-
spat (Calciumfluorid) als
Fluoreszenz,
1819 -1903
Max Haitinger
Max Haitinger
(1868-1946) priigte 1911
den Begriff Fluorochrom
und gilt als Begyiimder
der modermen Pluores-
zenzinikroskopie und der
Flucrochromierungs-
technik,
1868-1946
Alexander Jablonski
(1898-1980) stellt 1935
sein Modell zur Erkiérung
der Fluoveszenz vor:
Ein Fluorochrom besitzt
unterschiedliche enengeti-
sche Formen, sogenanate
Singuleit-Zusttinde
(SO, S1, S2...).
Alexander Jablonski
1898-1980
Albert Hewett Coons
Albert Hewett Coons
(1912-1978) und Melvin
Kaplan entwickeln ab 1950
dic Immunfluoreszenz-
techuik, die im den Natur-
wissenschaften zu Auf-
sehen erregenden Ergeb=
nnissen auf dem Gebiet der
Zellforschung filrte.
1912-1978
General solution for all weird bodies A Wigner Rotation Matrix here, a Spherical Harmonic there, and a Legendre Polynomial everywhere, and you have the answer. Got it? Integrate a bit, expand in these lovely functions, orthogonalize everything, and so on. It’s easy – no sweat. A theoretician solving for the rotational anisotropy of a completely anisotropic body PHYSICAL REVIEW VOLUME 107, NUMBER 1 JULY 1, 1957
Isotropic Rotational Brownian Motion
W. H. Forey
Lyman Laboratory of Physics, Harvard University, Cambridge, Massachusetts
. (Received March 8, 1957)
The Brownian motion of the orientation of any rigid body (sphere, set of rectangular axes, etc.) is calcu-
lated for the case of individual random infinitesimal rotations whose probabilities are independent of the
direction of the axis of rotation (isotropic case). The calculations are carried out by means of quaternions;
the more important formulas are also given in terms of the rotation angle and axis direction. The unit solu-
tion, or distribution of orientations arising from a specified initial orientation, is found as a series converging
rapidly for not-too-small times. Tr turns out to be expressible in terms of a theta function, and thus there is
also available a series converging rapidly for small times. The use of the unit solution as a propagation func-
tion is discussed briefly, and is illustrated by verification of the iteration property of the unit solution,
PHYSICAL REVIEW VOLUME 119, NUMBER 1 JULY 1, 1960
Theory of the Rotational Brownian Motion of a Free Rigid Body*
L, Dare Fayrot
Department of Physics, Harvard University, Cambridge, Massachuselts
(Received February 10, 1960)
The orientation of a rigid body is specified by the Cayley-Klein parameters. A system af such bodies
subject to small random changes in orientation but not subject to any externally applied torque is then
considered in some detail. A diffusion equation is derived with certain linear combinations of the Cayley-
Klein parameters as independent variables. This equation is expressed in terms of quantum-mechanical
angular momentum operators and a Green's function for the equation is obtained as an expansion in angular
momentum eigenfunctions. This expansion can be used to calculate averages of various physical quantities
in a nonequilibrium distribution of orientations. It may also be used to calculate the spectral density of
fluctuating quantities in an equilibrium distribution. Illustrative examples of both of these applications
are given.
anisotropic rotational diffusion is given by Favro." He
showed that the diffusion equation can be given by
af(Q, t) /at= — Hf(Q, 1), (1)
where /(Q, ¢) is the probability that the vector of a
molecular dipole transition is oriented in the angle
(Q) at time / and the Hamiltonian is given by
H=Q LDisL;,
tea
where L is the quantum mechanical angular momentum
operator and Dy; is the component of the diffusion
tensor. If one is able to find a coordinate system that
diagonalizes the diffusion tensor,” then the Hamil-
tonian becomes
H=E D;L2. (2)
It is immediately evident that Eq. (1) is analogous to
the Schridinger equation for an asymmetric rigid rotor.
It is further shown by Favro that the diffusion Eq. (1)
may be solved by the Green’s function method, namely
f(,1)= J {O)G(O4|0,4M, (3)
where f({p) is the initial probability that the dipole
vector is oriented in @) at f=0 and G(Qp| Q, 1) is the
Green’s function that describes the rotation of the
dipole vector from Q» at =O into Q at time /. The
function G(Q)|Q,/) can be expanded in terms of
asymmetric rotor wavefunctions.
G(Q5 | @, 1) =E WV." (5) ¥a(Q) exp(— Ext), (4)
THE JOURNAL OF CHEMICAL PHYSICS VOLUME 57, NUMBER 12
Theory of Fluorescence Depolarization by Anisotropic Rotational Diffusion
T. J. Cuvans ano K. B. Eisuxruat
IBM Research Laborsory, San Jose, Calijornic 95114
(Received 28 February 1972)
with the initial condition
G(Qp | 2, 0) = 8(Mo, Q) = Hn* (Qo) Fn (Q),
where ¥,(@) and E, are the stationary state eigen-
function and eigenvalue for the asymmetric rigid rotor
with the substitution #?/2/; by D;. The wavefunction
¥,(Q) may be expanded in terms of symmetric rotor
wavefunctions ym“! (@)"
¥,(Q) =F, (Q) = zy Anji? Bim (Q). (5)
i=]
The coefficients 4,,.9 and eigenvalues E,{ are tabu-
lated by Favro and Huntress! for /<2.
15 DECEMBER 1972
Zi (t) = PO) (o-+ (4/15) geguvery exp[—3(D.+ D)1]
+ (4/15) qaersy: expl—3(Ds+D)t]
+(4/15) q.qe¥ evs exp[—3(D,+ D)t]
+ (1/15) (8+a) exp[—(6D+24)¢]
4 + (1/15) (@—e) exp[—(6D—2a)s]}, (12a)
am
hO=sPO-Ai, (12b)
where
B=aeye+qiy tqere— (1/3),
a= (Do! A) (artery egy t+ y+ 92")
+(D,/A) (g2y2+ 92 — Igy 3 +yi+4")
+ (D./A) (qaPy2? tay — gry e+ ae)
—(2D/A),
D=4(De+D,+D,),
A= (D2+D,-++ D2—D,D,—D,D,—D,D,) "2.
The constant D is the average of the three principal
diffusion constants and A is related to the anisotropy
of the diffusion. The fluorescence polarization anisot-
ropy, defined as R(f) = (7) () —fa() /H +20]
can be obtained from Eqs. (12a) and (12b), Similarly,
the steady-state fluorescence polarization, P, given by
P= (K-Ex)/U4Ey), (13)
can also be obtained by time averaging over the emis-
sion decay. For an exponential decay of the emission
= 1 Sauda a¥y
Pie =—
3 ae (D,+D)
Aqugevy¥s +
* i¢3(D-4D)r
we find
Completely anisotropic rotator
From Eqs. (12a) and (12b), we see that in general,
aside from P(t), the polarized components of the
fluorescence and its anisotropy R(é) have five exponen-
tials in their decay. This is expected since both the
probability functions of excitation and emission trans-
form as the second rank of the rotation matrices which
have 2/-+1=5 dimensionality. Only eigenfunctions and
eigenvalues for the rigid rotor with /=2 are therefore
involved in the evaluation of J)\(¢) and Ji(¢), Hence
for a given molecular system, one can see clearly how
many exponentials and what type of exponents one
would expect to obtain by examining the transforma-
tion properties of the asymmetric rotor wavefunctions.
Tn(tde, (14a)
iu=r f°
o
her f ” ra(Ddt, (14b)
o
and 7
Aq.daVe¥2
1+3(D,+D)r
B+o + a- )
+(6D+2A)r © 14+(6D—2A)z/"
(15)
Ellipsoid
For symmetric-top molecules, one would generally ex-
pect three exponential decay terms, aside from P(1),
because there is a twofold degeneracy of eigenvalues in
the components of the angular momentum along the
symmetric axis for this type of system. The eigen-
functions Vim (Q) and Wiam®(Q), and Wen (Q)
and W_2.m(@) are degenerate when D.= Dy¥D,. In
this case Eq. (12a) is reduced to
T(t) = ($+ (1/15) [2 (geet aus)? (1-92) (1-2) ]
X exp[—(2D,+-4D,)t}+ (4/15) geye(gevet ayy)
X exp[— (5D,+D,)fJ+ (1/15) (39.21) (y2—4)
x exp(—6D2)}P(). (17)
This corresponds to the rotation of an ellipsoid. prolate
or oblate in shape.
Sphere
. As for the case of isotropic diffusion,
only one constant, namely 6D, can characterize the
decay in polarization since rotation along any axis has
the same diffusion constant, From Egs. (12a) and
(12b) we have
T(t) = { (1/9) + (2/45) exp(—6D%) (3 cos*’— 1) } P(t),
(18a)
Fi(t)={ (1/9) — (1/45) exp(—6Dzé) (3 cos*s—1)} P(A),
(18b)
and
R(t) =4(3 cos*k—1) exp(—6Di), (19)
Po i= (P—}) (14+-6Dr), (20)
where .
Po— 4= (10/3) (3 cos®’&— 1), (21)
and ) is the angle between the absorption and emission
dipoles. We recognize that Eq. (20) is just the expres-
sion for steady-state volarization given bv Perrin for
spherical molecules."
Volume 14, number 5 CHEMICAL PHYSICS LETTERS 1 July 1972
POLARIZED FLUORESCENCE AND ROTATIONAL BROWNIAN MOTION
M. EHRENBERG and R. RIGLER
institute for Cell Research, Medicinska Nabelinstitutet, Karolinska Mnstitatet, Stackholm, Sweden
Received 27 March 1972
b
ON
Fig. i.
The transformation of vectorial components from.
one system to the other is achieved with the aid of a
matrix M [10].
ix, fo %e\ {cos #3 sin ay
1X4
t a
j ty |
| ¥, =MiC}, ly l= ual sing, sind |, (4.1)
poet ye} ie] \ Z }
ls} \f -/ \
\2a/ \L \z0/ cosa
with
/[ cosy, sin? sing, cosy, sin 2,
re i j |
sing, cos 0, cosy, sing, sin ca i,
Qo cos By {
!
\csind
Why does a cylinder with rotational diffusion about only its cylinder axis show two correlation times of anisotropy decay? We give up!! WHY? It’s simple – just sines, cosines, and a bit of trigonometry =molecular rotation
axis
A
n
<N —
( ) ( ) 2 2D , ,t tt ∂ ∂ ∂∂Φ Ρ Φ = Ρ Φ Φ r D kT fφ = ( ) ( )( ) 2Dcos sin k tk ka k b k e−Φ + Φ ( ) ( )( ) ( )( ) 20 1, cos sin k Dtk kkt a a k b k e ∞ − = Ρ Φ = + Φ + Φ∑ ( ) ( )( ) ( )( )0 1,0 cos sink kka a k b k ∞ = Ρ Φ = + Φ + Φ∑ Ρ Φ,0( ) = an cos nΦ( )+ am cos mΦ( ) Ρ Φ, t( ) = an cos nΦ( )e −n2 Dt + am cos mΦ( )e −m 2Dt ( ) ( ) ( ) ( ) ( ) 0 1 ,0 2 1 ,0 cos 1 ,0 sin k k a d a k d b k d π π π π π π π π π − − − ⎛ ⎞= Ρ Φ Φ⎜ ⎟ ⎝ ⎠ ⎛ ⎞= Ρ Φ Φ Φ⎜ ⎟ ⎝ ⎠ ⎛ ⎞= Ρ Φ Φ Φ⎜ ⎟ ⎝ ⎠ ∫ ∫ ∫ If: Then: The diffusion equation about the cylinder rotation axis (the only free parameter) Specific solution: General solution: t=0 initial distribution Example of initial and time dependent solutions. x2 = 2Dt Just like Einstein told us: Initial angular distribution of an ensemble (from photoselection). Both distribution shapes remain constant with time. Only the amplitudes decrease with their time constants. ( ) 41 2 0 Remember: D t D tr t A e A e A− −= + + ( ) ( ) ( ) 2 2 2 0 0 0 ˆˆThe vertical signal is , , sine et z e d d d π π π ϕ ϕ ϕ θ φ= Ρ Φ ⋅ ⋅∫ ∫ ∫ ( ) ( ) ( ) 2 2 2 0 0 0 ˆ ˆThe horizontal signal is , , sine et x e d d d π π π ϕ ϕ ϕ θ φ= Ρ Φ ⋅ ⋅∫ ∫ ∫ ( ) ( ) ( )ˆ ˆ ˆ ˆ ˆ ˆ ˆ ˆ ˆ ˆ ˆ ˆ ˆ ˆsin cos cos cos ˆ ˆ ˆ ˆcos sin sin ˆ ˆ ˆ ˆsin cos sin e e e e e e n e n x e x y e y x n x x n e y e x e x y ϕ θ θ ϕ θ θ φ θ φ θ Φ Φ Φ Φ Φ Φ Φ Φ = ⋅ + ⋅ + ⋅ ⋅ = ⋅ = − ⋅ = ⋅ = ⋅ = ⋅ = Now we have to observe the anisotropy ( ) ( ) ˆ ˆ cos sin cos sin cos cos cos sin sin sin cos cos sin sin cos cos sin sin sin e e e e e e e e e e x e θ ϕ θ θ φ θ ϕ θ φ θ θ θ ϕ θ φ ϕ θ φ θ ⋅ = − + = − + Project the distribution of the emission dipole onto the x- and z-axes and integrate over the distribution. Then form the anisotropy expression. ( ) ( )( ) ( ) ( )( ) ( )( ) ( )( ) 2 2 2 2 2 2 2 2 D 2 2 2 4D 4 2sin sin cos15 15 vert. sig. 4 62cos sin cos15 15 32 cos sin cos sin cos15 8 sin sin cos 215 e a a e a a t e e a a e a t e e e a e e θ θ θ π θ θ θ π θ θ θ θ φ π θ θ φ − − ⎛ ⎞+⎜ ⎟ = ⎜ ⎟ + +⎜ ⎟ ⎝ ⎠ + + ( ) ( )( ) ( ) ( )( ) ( )( ) ( )( ) 2 2 2 2 2 2 2 2 D 2 2 2 4D 6 8sin sin cos15 15 horiz. sig. 2 8 4cos sin cos15 15 16 cos sin cos sin cos15 4 sin sin cos 215 e a a e a a t e e a a e a t e e e a e e θ θ θ π θ θ θ π θ θ θ θ φ π θ θ φ − − ⎛ ⎞+⎜ ⎟ = ⎜ ⎟ + +⎜ ⎟ ⎝ ⎠ − + ( )( )( ) ( )( ) ( )( ) 2 2 D 2 2 4D 1 3cos 1 3cos 110 6 cos sin cos sin cos5 3 sin sin cos 210 a e t e e a a e a t a e e a r e e θ θ θ θ θ θ φ θ θ φ − − = − − + + ( )( )( ) ( )( ) ( ) ( )( ) 2 2 D 2 2 2 2 4D 1 3cos 1 3cos 110 3 sin 2 sin 2 cos10 3 sin sin cos sin10 a e t e a e a t a e ea ea r e e θ θ θ θ φ θ θ φ φ − − = − − + + − Sometimes given as: ( ) ( )( ) ( ) ( ) 2 2 2 2, sin sin , , ,sin r r D D f t f t f t f t t θ θ θ θθ φ ⎡ ⎤∂ ∂ ∂ ∂ ∇ Ω = Ω + Ω = Ω⎢ ⎥∂ ∂ ∂∂⎣ ⎦ 3 , 8r sphereD kT aπη= ( ) ( ) ( ) ( ) ( )( ) ( ) ( ) ( ) ( ) 2 2 2 2 2 2 , , , , ,11 cos 2 cos 1 2 coscos r f t f t f t f t f t u u D t uu θ θ θθ ∂ Ω ∂ Ω ∂ Ω ∂ Ω ∂ Ω − − = = − − ∂ ∂ ∂∂∂ ( ) ( ) ( )0, n nnf t P u a t ∞ = Ω =∑ ( ) ( ) ( ) ( )0 0( 1)r n n n nn n dD n n P u a t P u a t dt ∞ ∞ = = − + =∑ ∑ ( ) ( ) ( ) ( )( 1)r n n n n dD n n P u a t P u a t dt − + = ( ) ( ) ( )0 exp ( 1)n n ra t a n n D t= − + ( ) ( ) ( ) ( )0, cos 0 exp ( 1)n n rnf t P a n n D tθ ∞ = Ω = − +∑ ( )( )2 2cos 1 3 2 cos 1Pθ θ= + ( )1 6spherer rDτ = Rotation of a Sphere ( ) ( ) ( ) ( ) 2 2 21 2 ( 1) n n n P u P u u u n n P u uu ∂ ∂ − − = − + ∂∂ Then photoselection