Introduction
Solvent paramagnetic relaxation enhancement (sPRE) has been used to study protein solvent
accessibility,1-7 to refine NMR protein structures,8-10 to investigate protein-cosolute interactions,11-
14 and to characterize the electrostatic potential on small molecules and proteins.15-26
In m any sPRE applications, the transverse sPRE rate G2 is directly used to quantify
electrostatics20-25 and for structure refinement ,8-10 based on the Otting-LeMasterβs empirical
analysis,3, 4 which correlates G2 with the average interspin distance β©π!"βͺ#$%& . This empirical
approach has demonstrated excellent correlation with the Poisson-Boltzmann based theoretical
electrostatic near -surface potentials (ENS) and the experimental ENS. However, d espite its
apparent success, a fully satisfactory theoretical explanation for why this approach works has yet
to be established.
In previous work, we hypothesized that G2 is proportional to β©π!'βͺ#$%& and demonstrated its
validity using a simple hard-sphere square potential model.13 Here, we present a comprehensive
theoretical framework that establishes G2 as being proportional to β©π!'βͺ#$%& rather than β©π!"βͺ#$%&.
Our derivation is broadly applicable to various types of intermolecular potential, including those
in confined environement, such as reverse micelle systems. While this work focuses on sPRE, the
analysis is equally applicable to a wide range of intermolecular spin relaxation by translational
diffusion in liquids.
Theory
The dipole-dipole correlation function in an isotropic liquid is given by:27, 28
πΆ(π‘) = π! β©"!#$Μ(')β$Μ(*)+
$"(')$"(*) βͺ (1)
where r and πΜ are the lengths and orientation of the interspin vector πβ; P2(x) is the Legendre
polynomial of degree 2; and NS is the number of paramagnetic cosolute molecules in the system.
The number density of the cosolute π( is related to NS and the volume of the system V by
,#
- .
The subscript o denotes the quantity at t = 0.
The spectral density J(w) is given by the cosine transform of C(t):
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π½(π) = β« ππ‘
β
0 πΆ(π‘) cos(ππ‘) (2)
where w is the angular frequency in radians.s-1, and is related to the spectrometer frequency (n) in
Hz) by π = 2ππ.
The transverse ( G2) sPREs are defined as the difference in the transverse relaxation rates,
respectively, of a protein nuclear spin (generally a proton) in the presence and absence of the
paramagnetic cosolute.29 At high external magnetic field limit, G2 is related to the spectral density
function J(w) by:30-32
Ξ) =
*
+ -
,!
'π.
)
β) πΎ-
) πΎ.) 2π½(0) +
/
' π½(π-)5 (3)
where gH and ge are the gyromagnetic ratios of the proton and electron, respectively; Β΅o is the
vacuum permittivity constant; is Planckβs constant divided by 2 p; wH is the angular frequency
of the proton. In many instances, π½(0) β« π½(π-) thus Eq.(3) can be approximated as
Ξ) β
*
+ -
,!
'π.
)
β) πΎ-
) πΎ.
) π½(0) (4)
Consequently, the insights we can gain about the cosolute-protein interactions from the transverse
sPRE relaxation rate is contained primarily in the details of the spectral densities J(0).
To relate experimentally observable sPRE relaxation rates to physical quantities, we
introduced the concepts of the concentration normalized average interspin distances11, 13, 14
β©π!) 0βͺ#$%& = 4π β« ππ
β
1 π!) (03*)π!56(7) (5)
where π(π) is the potential of the mean force ; b is the thermodynamic beta; and l is 2, 3, or 4. It
should be emphasized that Eq.(5) is defined for any arbitrary shapes of the protein and cosolute
and for arbitrary interactions between them.
If J(w) can be measured across a wide range of the spectrometer fields, β©π!"βͺ#$%& can be
calculated by taking the integration the spectral density function.11 It has also been shown that the
high-frequency limit of the w2J(w) is directly related to β©π!8βͺ#$%&.13
!
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In the previous work,13 we hypothesized that J(0) is related to β©π!'βͺ#$%& by
β©π!'βͺ#$%& β
)9 :"#$%&
';'
π½(0) (6)
We demonstrated that Eq.(6) provide reasonable approximat ions for simple models involving
spherically symmetric square -well and Coulombic potentials. We have also compared
experimental ENS and Poisson -Boltzmann-based ENS , implemented with β©π!'βͺ#$%&
interpretation, on ubiquitin and drkN SH3. For both systems, excellent agreements are achieved
between calculated and experimental ENS similar to or slightly better than the conventionally used
β©π!"βͺ#$%& interpretations.
Despite the apparent success of the Eq.(6), its applicability for arbitrary potentials with
varying interaction strengths remained unclear. In this work, we establish a rigorous theoretical
foundation of the validity of Eq.(6) and demonstrate that it applies across a wide range of
systems, including those in confined environments.
In this work, we consider the simplest case where the protein and cosolutes are modeled
as hardspheres, with the nuclear and electron spins located at their respective centers. The
interspin vector πβ is specified by three coordinates in spherical coordinates πβ = (π
, π, π). The
cosolute and protein are assumed to be diffuse under the influence of the spherically symmetric
potential characterized by the potential of the mean force U(R), which only depends on the
center-to-center distance R. The cosolute is allowed to diffuse within the volume V specified by
the contact distance π
< and the outer boundary π
= such that π
< β€ |πβ| β€ π
=. To simplify and
clarify our discussion, many of the technical details of the derivations of the equations described
below are provided in the Supporting Information.
Under the assumption that cosolute-protein pair is described by the Smoluchowski formalism
(see Supporting Information for detail), it can be shown13 that the J(0) is given by
π½(0) =
('>)(
+ π( β« ππ
?
@)
@*
.+,-(/)
@!
π?(π
?) (7)
where π?(π
?) is the solution to the equation,
β
A
A@!
Fπ!56(@!)π
?
) A
A@!
π?(π
?)G + 6π!56(@!)π?(π
?) =
+.+,-(/!)
'>:"#$%&@!
(8)
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subjected to the reflective boundary conditions
AB!
A@!
I
@!C@*
=
AB!
A@!
I
@!C@)
= 0 (9)
Therefore, J(0) can be calculated once π? is known. In practice, π? can be solved analytically
only for few special cases such as force-free hardsphere (FFHS) model where U(R)=0 or when
the potential of the mean force is modelled as a square-well potential.
In the case of the FFHS model, J(0) is given by
π½(0) = π(
>(*!D)E/) 3D(*3D)F/93D(+3/) D)GH
+'@*(*3D3D( 3D13D2) (10)
where π¦ = π
;'
)9 :"#$%&@*
=
';'
)9 :"#$%&
β©π!'βͺ#$%& (11)
It should be pointed out that for the FFHS model with infinite volume, Eq.(11) implies that
Eq.(6) is exact; however, as seen from Eq.(10), π½(0) is not strictly equal to
';'
)9 :"#$%&
β©π!'βͺ#$%&
when finite volume is considered.
Lower and Upper Bounds of J(0)
Since the analytical form of π? for an arbitrary potential is not known, we approximate J(0) by
evaluating its lower and upper bounds using the complementary variational principle.33-36
For rigorous explanations the technique employed in this work, see refer to Ref.33, 37, 38.
Let us introduce new functions π, π€, π given by
π(π
?) = π!56(@!)π
?
)
π€(π
?) = 6π!56(@!)
π(π
?) = 5π!56(@!)
4ππ·J%K#Lπ
?
(12)
It is important to note that π, π€, π are nonnegative functions.
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Using these new functions, Eq.(8) can be written in the form of Sturm-Liouville equation
β
A
A@!
-π
AB!
A@!
. + π€π? = π (13)
Let us introduce a functional πΌ[π] given by
πΌ[π] = β« ππ
?
@)
@*
Yβπ -
AB
A@!
.
)
β π€π) + 2ππ[ (14)
where the admissible functions of this functional are the set of all functions π that have well
defined first- and second derivatives and also satisfy the boundary conditions Eq.(9).
When π = π?,
πΌ[π?] = \ ππ
?
@)
@*
]βπ 2ππ?
ππ
?
5
)
β π€π?
) + 2ππ?^ = \ ππ
?
@)
@*
{ππ?} = 25
(4π)/
π½(0)
π·J%K#Lπ(
(15)
If π is a function that deviates from the π? by a small amount
π(π
?) = π?(π
?) + ππ(π
?) (16)
where π is some small number and π is some arbitrary admissible function. Substituting Eq.(16)
in Eq.(14), we get
πΌ[π] = \ ππ
?
@)
@*
]βπ 2 ππ
ππ
?
5
)
β π€π) + 2ππ^
= \ ππ
?
@)
@*
]βπ 2ππ? + ππ
ππ
?
5
)
β π€(π? + ππ)) + 2π(π? + ππ)^
= πΌ[π?]β π) \ ππ
?
@)
@*
]π 2 ππ
ππ
?
5
)
+ π€π) ^
(17)
The first variation πΏπΌ (the term linear to π) is given by
πΏπΌ = 0 (18)
and the second variation πΏ) πΌ (the term linear to π) ) is given by
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πΏ) πΌ = βπ) β« ππ
?
@)
@*
Yπ -
AM
A@!
.
)
+ π€π) [ β€ 0 (19)
Since πΌ[π?] has the first variation zero and second variation negative (concave down), Eq.(18)
and (19) imply that πΌ[π?] is the global maximum value that can attained by any admissible π.33
To obtain the upper bound, define another function
π’?(π
?) = π(π
?) A
A@!
π?(π
?) (20)
Note that π’? satisfies π’?(π
<) = π’?(π
=) = 0.
Then the Eq.(13) can be rewritten as
β
AN!
A@!
+ π€π? = π (21)
Let us introduce another functional πΊ[π’] given by
πΊ[π’] = β« ππ
?
@)
@*
Y
*
O π) +
*
P -
A,
A@!
+ π.
)
[ (22)
where the admissible functions is the set of all functions that have well-defined first derivative
and satisfies the boundary conditions
π’(π
)1
R(1)
:"#$%&;'
(24)
Similar to the lower bound case, we calculate the first- and second variations of πΊ[π’] by
considering small deviations to π’?. Consider the function π’ given by
π’(π
?) = π’?(π
?) + ππS(π
?) (25)
where πS is some admissible function.
When Eq.(25) is substituted in Eq.(22), we get
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πΊ[π’] = \ ππ
?
@)
@*
]1
π π’) + 1
π€ 2 ππ’
ππ
?
+ π5
)
^ = \ ππ
?
@)
@*
h1
π (π’? + ππS)) + 1
π€ Fππ’? + ππS
ππ
?
+ πG
)
i
= πΊ[π’?]+ π) \ ππ
?
@)
@*
hπ F ππS
ππ
?
G
)
+ π€πS) i
(26)
Eq.(26) implies that
πΏπΊ = 0 (27)
πΏ) πΊ = 2 β« ππ
?
@)
@*
Yπ -
AM3
A@!
.
)
+ π€πS) [ β₯ 0 (28)
Having first variation zero and second-variation nonnegative (concave up), Eqs.(27) and (28)
implies that πΊ[π’?] is the global minimum value attainable by any admissible function.33
To summarize our finding, we derived the following relation
πΌ[π] β€ πΌ[π?] =
)+
('>)1
R(1)
:"#$%&;'
= πΊ[π’?] β€ πΊ[π’] (29)
Eq.(29) provides the useful estimation of J(0) by choosing proper choice of the trial functions π
and u.
Here, the FFHS model (U(R)=0) was used as the trial function by setting π = πT--( to obtain
the lower bound. Similarly, upper bound were found by substituting trivial function u = 0 into
Eq.(22). After some rearrangement of the equation, we obtained the main finding of this work
0.9375β©π!'βͺ#$%& β€
)9 :"#$%&R(1)
';'
β€ 1.125β©π!'βͺ#$%& (30)
Eq.(30) suggest that
)9 :"#$%&R(1)
';'
β β©π!'βͺ#$%& with the error up to 12.5 %. Consequently, once
π·J%K#L is acquired, a reasonable estimate of β©π!'βͺ#$%& can be determined without any adjustable
parameters. It should be emphasized that Eq.(30) holds true for arbitrary potential of any
interaction strength. Furthermore, Eq.(30) does not depend on the value of π
= (see Supporting
Information and Fig.S1), making it applicable to confined environments, such as reverse-
micelles, under assumption that the diffusive motion of the cosolute is described by
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Smoluchowski equation Eq.(S2). As a result, Eq.(30) provides the rigorous interpretation of J(0)
for wide variety of systems. To illustrate this, we simulated the spectral densities using Lennard-
Jones and Coulombic potentials and demonstrated that the inequality Eq.(30) indeed holds valid
(Figure 1).
Interestingly, the upper bound found in Eq.(30) combined with the continuity of the first
derivative of π? implies that
AB!
A@!
is always less than or equal to zero. That is, π?(π
?) is a
monotonically decreasing function, which may not be intuitively obvious.
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13
Figures
Figure 1. Illustration of the validity of Eq.(30).
(A) The examples of the potentials used to simulate β©π45βͺ6789 and the approximate β©π45βͺ6789
:;;87< = 27π·transπ½(0)
4πS
.
The Lennard-Jones potential of the form π½π(π
C) = 4π , -
D!
D"
.
EF
β -
D!
D"
.
G
0 was used to generates the points on the
left panel. The potential is minimum at 2
#
$π
H. The Coulomb potential of the form π½π(π
C) = βπ
D%I&'("
D"
where π
is
the inverse of the Debye length was used to simulate the points on the right panel. For both potentials, π is the
parameter used to modulate the strengths of protein-cosolute interaction. (B) The comparison between exact and
approximate β©π45βͺ6789. The exact β©π45βͺ6789 were calculated from numerically evaluating the integral Eq.(5). The
approximate β©π45βͺ6789 were calculated using Eq.(6). The corresponding β©π45βͺ6789
:;;87< are numerically calculated by
finite-difference method explained in details in the Supporting Information of the Ref. 13. The relevant parameters
used for the finite-difference methods are : βπ
= 104EF m, π = 120, π = 500 and π = 1.01. The values for the
other parameters used in the simulations are: π
J = 1 nm, π
K = 5.8 nm, π
H = 1.15 nm and the Debye lengths
1/π
= 25 nm. It should be pointed out that the numerical values of π( and π·L8:6M do not affect our results.
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