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. 2011 Nov 2;101(9):2232–2241. doi: 10.1016/j.bpj.2011.09.053

Size Distribution of Amyloid Nanofibrils

Raffaela Cabriolu †, Dimo Kashchiev ‡, Stefan Auer †,∗
PMCID: PMC3207154  PMID: 22067163

Abstract

We consider the size distribution of amyloid nanofibrils (protofilaments) in nucleating protein solutions when the nucleation process occurs by the mechanism of direct polymerization of β-strands (extended peptides or protein segments) into β-sheets. Employing the atomistic nucleation theory, we derive a general expression for the stationary size distribution of amyloid nanofibrils constituted of successively layered β-sheets. The application of this expression to amyloid β1-40 (Aβ40) fibrils allows us to determine the nanofibril size distribution as a function of the protein concentration and temperature. The distribution is most remarkable with its exhibiting a series of peaks positioned at “magic” nanofibril sizes (or lengths), which are due to deep local minima in the work for fibril formation. This finding of magic sizes or lengths is consistent with experimental results for the size distribution of aggregates in solutions of Aβ40 proteins. Also, our approach makes it possible to gain insight into the effect of point mutations on the nanofibril size distribution, an effect that may play a role in experimentally observed substantial differences in the fibrillation lag-time of wild-type and point-mutated amyloid-β proteins.

Introduction

The assembly of proteins into amyloid fibrils is an important phenomenon with wide implications ranging from human disease to nanoscience. Amyloid fibril formation is associated with a growing number of neurological and systemic diseases (1) including Alzheimer's and Parkinson's diseases, and the application of amyloid fibrils as molecular building blocks in biosensors, tissue engineering, and antibacterial agents has been demonstrated (2). The main insight into the structures formed by proteins comes from structural biology experiments. Such experiments are very challenging for protein aggregates because of the aggregate transient nature and structural heterogeneity (1). An essential point in our current understanding is that peptides and proteins unrelated in sequence and structure have been shown to convert into large fibrillar aggregates including amyloid fibrils (1). These aggregates share a common cross-β structure formed by intertwined layers of β-sheets extending in a direction parallel to the fibril elongation axis (3–8). Oligomeric aggregates are often found as precursors of amyloid fibrils (9–11) and their structure can vary from that of highly disordered aggregates that are composed of unstructured proteins to that of nativelike aggregates in which the proteins retain their native state.

It is now well established (9,10,12–30) that fibrillar protein aggregates can form by a nucleation mechanism. Time-resolved optical experiments that measure the fluorescence signal arising from a dye-binding molecule such as thioflavin-T bound to the protein aggregate have been used to determine the lag time, during which no aggregates are detected, and the maximal rate of conversion of protein monomers into aggregates. Experiments (28,31–41) have been performed to reveal the relationship between the physicochemical properties of the natural amino acids and the kinetics of amyloid formation. These experiments have in turn been used to substantiate phenomenological models (42–46) able to predict changes in the propensity of proteins to aggregate upon mutation as well as to identify amino-acid sequences of proteins that are likely to belong to the fibril core. To gain more insight into the nucleation mechanism and to determine important nucleation parameters such as the fibril nucleus size and nucleation rate, it is necessary to monitor the time evolution of the aggregates formed in a nucleating protein solution. Recently, small-angle x-ray scattering (47,48) and fluorescence correlation spectroscopy experiments (29,49) have been used to monitor the population, structural changes, and size of protein aggregates in the solution. Understanding and interpreting such experiments requires developing a theoretical framework describing amyloid fibril nucleation.

In previous studies, we used concepts from the theory of overall crystallization to describe the kinetics of overall protein aggregation (50), and applied the classical and atomistic nucleation theories (CNT and ANT, respectively) to treat the nucleation of amyloid fibrils when the process takes place by the mechanism of direct polymerization of single β-strands (extended peptides or protein segments) into β-sheets (51,52). In this, our treatment differed from that of Schmit et al. (53), who considered the case of amyloid fibril nucleation in two steps: single β-strands assemble into disordered oligomers, which then transform into β-sheets. The application of ANT has been demonstrated by correlating theoretical fibril nucleation rates with experimental lag times in the fibrillation kinetics of β2-microglobulin and amyloid β1-40 (Aβ40) proteins (54). The objective of this study is to employ nucleation theory for determination of the size distribution of amyloid nanofibrils (protofilaments) in protein solutions when fibril nucleation occurs in one step by polymerization of β-strands from the solution directly into β-sheets. We derive a general expression for the stationary size distribution of amyloid nanofibrils constituted of successively layered β-sheets and illustrate how this expression can be applied to the smallest Aβ40 protofilaments. The results obtained are applicable to homogeneous nucleation that takes place when the protein solution is sufficiently pure and/or strongly supersaturated.

Theory

Modeling the amyloid nanofibril

Nucleation of nanosized amyloid fibrils by direct polymerization of β-strands into β-sheets is operative when no fibril precursors such as dropletlike oligomers are formed as a first step in the fibril nucleation process. Fig. 1 defines the nanofibril and illustrates our model (52,54). The model is based on reported structural and morphological results for amyloid fibrils and microcrystals (3–8). Due to their strong hydrogen bonds, the virtually fully extended protein β-strands can arrange themselves into β-sheets that stretch forth along the fibril lengthening axis (the m axis in Fig. 1). The much weaker hydrophobicity-mediated interstrand bonds cause the β-strands to assemble along the fibril thickening axis (the i axis in Fig. 1) in such a way that a nanosized amyloid fibril composed of successively layered β-sheets can form. Because the fibril width is fixed and equal to the β-strand length, the fibril can be considered as a two-dimensional aggregate in the m,i plane, with building blocks (the β-strands) arranged in a two-dimensional lattice with simple rectangular symmetry (Fig. 1). Inasmuch as these blocks play the role of the atoms in the original ANT, with the term “atomistic” referring to the β-strands, this theory is readily applicable to our nanofibril model.

Figure 1.

Figure 1

Schematic of nanosized fibril with thickness of two differently long β-sheets. The first and the second β-sheets are with length of 14 and 7 β-strands, respectively. Each of the 21 β-strands of the fibril is composed of 19 amino acids. The 19 red and 19 blue lines shown for the rightmost β-strand of the second β-sheet visualize the amino-acid strong and weak broken bonds that are in direction of the fibril lengthening and thickening (m and i) axes, respectively.

Sequence-specific binding energies

In the atomistic approach to nucleation of amyloid fibrils (52,54,55), important parameters are the binding energies of the β-strands within the fibril. We denote by E (J) and Eh (J) the binding energies between two nearest-neighbor β-strands along the m and i axes in Fig. 1, respectively. The excess energy of any n-sized nanofibril equals the fibril total surface energy (51) that, according to ANT (52,55), is given by the total energy lnE/2 + lh,nEh/2 of the nearest-neighbor broken-bonds at the periphery of the fibril cross section in the m,i plane. In the above sum, n is the number of β-strands in the fibril, and ln or lh,n is the number of all nearest-neighbor broken bonds that are parallel to the fibril m axis or i axis, respectively.

To calculate E and Eh, we assume that each amino acid in a β-strand (19 such amino acids are illustrated in Fig. 1 by the prisms in the rightmost β-strand of the shorter β-sheet) forms hydrogen bonds solely along the m axis, and that hydrophobicity-mediated bonds can be formed along both the m and i axes. Assuming further that bonds can only be formed between nearest-neighbor amino acids, the interstrand binding energies E and Eh are obtained by summation of the bond energies of such amino acids over all amino-acid pairs in neighboring β-strands:

E=∑p[εjq(p)+εh,jq(p)], (1)
Eh=∑phεh,jq(ph). (2)

In Eq. 1, the summation goes over all amino-acid pairs p in two nearest-neighbor β-strands of a β-sheet, and in Eq. 2 it goes over all amino-acid pairs ph in two nearest-neighbor β-strands of two successive β-sheets. The energies of a nearest-neighbor hydrogen amino-acid bond and a nearest-neighbor, hydrophobicity-mediated amino-acid bond between amino acids j and q are denoted by εjq (J) and εh,jq (J), respectively (εjq ≫ εh,jq, because the hydrogen bond is much stronger than the hydrophobicity-mediated one).

The assignment of amino-acid, sequence-specific values to the binding energies εjq and εh,jq allows application of our nanofibril model to concrete protein systems. In this study, the sequence-specific hydrogen-bond energies used are based on a statistical analysis (45) of the frequency that two residue types are found paired in neighboring β-strands within β-sheets in globular proteins. The pairing energy depends on the orientation (parallel or antiparallel) of the β-strands. We denote by εPjq and εAjq the dimensionless pairing energies for the parallel and antiparallel orientation, respectively, and employ the εPjq and εAjq values from Table 1 of Trovato et al. (45) to modulate the basic unit ε (J) of the hydrogen bond energy in such a way that the values of the binding energy εjq lie in the interval [0, 2ε]:

εjq=2(εPRO,ASPA−εjqP(A))(εPRO,ASPA−εCYS,CYSA)ε. (3)

Here εACYS,CYS = −2.57 and εAPRO,ASP = 3.55 are, respectively, the dimensionless energies of a CYS-CYS pair and a PRO-ASP pair in an antiparallel β-sheet, and εjqP(A) equals εPjq or εAjq for the parallel or antiparallel orientation. For the basic unit of the hydrogen bond we use ε = 6.95 × 10−21 J (1 kcal/mol), a value in the range of the hydrogen-bond energies measured experimentally (56).

Nanofibril evolution mechanism

The determination of the nanofibril size distribution requires specification of the sequence of shapes that the fibril takes during its evolution from the monomer size n = 1 to the considered size n > 1. In reality, there are many such sequences, but we choose a sequence of shapes that have the fibril equilibrium shape as a reference low-energy shape, because the latter corresponds to the minimal fibril total surface energy (51).

In this shape sequence (Fig. 2), the fibril initially evolves as a single β-sheet and its transition from one-dimensional to two-dimensional aggregate occurs at transition size nt that is assumed to be given by the CNT formula (51) nt = E/Eh. This size is an important parameter, because it characterizes the fibril equilibrium shape, i.e., the fibril thermodynamically favored aspect (length/thickness) ratio. Thus, the (nt + 1)-sized fibril (the one with n = 15 in Fig. 2) has the shape of 1β-sheet of length nt with one protein monomer (β-strand) adsorbed on the sheet surface. This monomer gives birth of the fibril second β-sheet and creates two kink sites at the fibril surface (marked by plus signs in Fig. 2). As shown in Cabriolu et al. (52), in a certain supersaturation range the (nt + 1)-sized fibril requires maximum work for its formation and is therefore the so-called nucleus. Further monomer attachment to a kink site does not increase the fibril total surface energy, because the fibrils of size n = nt + 1, nt + 2,…, 2nt have the same total number of broken bonds (see the fibrils with n = 15, 16, and 28 in Fig. 2).

Figure 2.

Figure 2

Sequence of nanofibril shapes corresponding to minimum total surface energy, which depicts the fibril evolution when the transition from one-dimensional to two-dimensional aggregate is at size nt = E/Eh = 14. The first three nanofibrils of size n′j (pink) and n″j (blue) are shown. (Hatched) First three fibril nuclei. (Pluses) Kink sites at which β-strand attachment occurs at no surface-energy cost.

Because from n = 2nt to n = 2 × 2nt the CNT equilibrium shape requires fibril thickness between one and two β-sheets, the attachment of the next protein monomer to the 2nt-sized fibril can be assumed to occur at one of the two fibril ends. This lengthwise monomer attachment creates a kink site at the end of the fibril of size n = 2nt + 1 (the fibril with n = 29 in Fig. 2) and the next monomer is attached to this site with no surface-energy cost. Thus, further fibril growth occurs by alternating creation and annihilation of kink sites at the fibril ends until the fibril reaches the size n = 2 × 2nt (see the fibril with n = 56 in Fig. 2). At this size, the attachment of the next protein monomer can be assumed to occur again to the surface of one of the fibril two β-sheets, because the CNT equilibrium shape requires fibril thickness between two and three β-sheets for fibril sizes from n = 2 × 2nt + 1 to n = 3 × 3nt. The fibril of size 2 × 2nt + 1 (the one with n = 57 in Fig. 2) will therefore have the shape of a double β-sheet, i.e., a 2β-sheet, of length 2nt with one protein monomer adsorbed on the 2β-sheet surface rather than attached to one of the 2β-sheet ends. The (2 × 2nt + 1)-sized fibril is also remarkable, because it is the nucleus in a corresponding supersaturation range (52). The first monomer on the 2β-sheet triggers the growth of the fibril third β-sheet, because it generates two kink sites at which subsequent monomers can attach themselves without changing the total number of the fibril broken bonds. In Fig. 2, the fibrils with n = 57 and 58 illustrate this situation.

When the third β-sheet is completed at size 3 × 2nt, the fibril growth continues by lengthwise attachment of the next protein monomer (see the fibrils with n = 84 and 85 in Fig. 2). Subsequent lengthwise attachment of monomers to the fibril is thermodynamically favored only up to size n = 3 × 3nt (that of the fibril with n = 126 in Fig. 2), because between this size and the size n = 4 × 4nt, to keep its shape close to the CNT equilibrium shape, the fibril has to increase its thickness by one more β-sheet. Thus, it can again be assumed that the fibril of size n = 3 × 3nt + 1 (which is the nucleus size in a respective supersaturation range (52)) will have the shape of a triple β-sheet, i.e., a 3β-sheet, of length 3nt with one monomer adsorbed on the surface of the fibril outer β-sheets (see the fibril with n = 127 in Fig. 2). Further growth of the fibril can be expected to occur in the above manner provided it is not disturbed by other processes, e.g., fibril flocculation.

Nanofibril size distribution

As known from nucleation theory (e.g., Kashchiev (57)), the stationary size distribution of the aggregates of a nucleating single-component phase can be presented exactly as (n = 1,2,3,…)

Xn=Cn∑k=nM−1(1fkCk)∑k=1M−1(1fkCk), (4)

when nucleation takes place by the Szilard-Farkas mechanism, according to which the aggregates change size by random attachment and detachment solely of monomeric building units. Here n (or k) is the number of building units in an aggregate, Xn (m−3) is the stationary concentration of n-sized aggregates, Cn (m−3) is the respective equilibrium concentration of such aggregates, M is the number of building units in a large enough supernucleus aggregate, and fn (s−1) is the frequency of building-unit attachment to an n-sized aggregate.

Equation 4 is readily applicable to nucleation of amyloid fibrils in the case when the process occurs by the mechanism of direct polymerization of β-strands into β-sheets. Then n is the number of β-strands in an n-sized amyloid nanofibril and, according to ANT, Cn and fn are of the form (52)

Cn=C1exp[(n−1)s−(ln−2)ψ−(lh,n−2)ψh], (5)
fn=12f1ln, (6)

when only the nearest-neighbor interactions between the β-strands are taken into account.

In Eqs. 5 and 6, C1 (m−3) is the actual concentration of single β-strands in the protein solution, and f1 (s−1) is the frequency of attachment of a single β-strand to another single β-strand. Physically, the sum in the exponent of Eq. 5, taken with minus sign, is the ratio between the work Wn to form a fibril of size n and the thermal energy kBT (kB is the Boltzmann constant, T is the absolute temperature). For sufficiently dilute solutions, the dimensionless supersaturation s is given by

s=lnC1Ce, (7)

where Ce (m−3) is the equilibrium concentration of single β-strands in the solution (Ce is also known as the protein solubility). The dimensionless energies ψ and ψh per strong (mainly hydrogen) and weak (hydrophobicity-mediated) broken bond are defined by

ψ=E2kBT, (8)
ψh=Eh2kBT. (9)

Equations 4 and 5 show that both the equilibrium and the stationary concentrations Cn and Xn of amyloid nanofibrils of a given size n increase strongly with increasing the solution supersaturation s, i.e., with a rise of the actual β-strand concentration C1 and/or a fall of the protein solubility Ce. As to Eq. 6, in it the proportionality of fn to ln reflects the fact that the β-strands are attached predominantly to the ends of the fibril β-sheets (the fibril strong broken bonds are namely at these ends), and the divisor 2 takes into account that a single β-strand has l1 = 2 strong broken bonds.

Combining Eqs. 4–9, we find that when only the nearest-neighbor β-strand interactions are accounted for, the sought stationary fibril size distribution Xn is given by the general ANT formula (n = 1,2,3,…) as

Xn=Cn∑k=nM−1(1lk)(CeC1)kexp(lkψ+lh,kψh)∑k=1M−1(1lk)(CeC1)kexp(lkψ+lh,kψh), (10)

in which

Cn=Ce(C1Ce)nexp[(2−ln)ψ+(2−lh,n)ψh] (11)

is the respective equilibrium fibril size distribution.

Equation 10 is a central result of this study. We emphasize that it is highly reliable, because it is based on the exact Eq. 4 and because in it the ratio of the two sums is practically unaffected by the approximate character of Eq. 6 for fn. Importantly, Eq. 11 is in conformity with the law of mass action because of the proportionality of Cn to C1n. Also, as a single β-strand has l1 = 2 strong and lh,1 = 2 weak broken bonds, Eq. 11 is self-consistent in the sense that at n = 1 it returns the identity C1 = C1.

It should be borne in mind that Eq. 10 is applicable solely to a supersaturated protein solution (i.e., when C1 > Ce), because the stationary size distribution Xn can exist in such a solution only. As then the solution is metastable with respect to fibril nucleation and growth, Xn replaces the equilibrium size distribution Cn that, albeit mathematically well defined, has no physical reality because of the solution metastability. When C1 = Ce or C1 < Ce, however, the solution is saturated or undersaturated, respectively, and neither nucleation nor growth are possible, for then the solution is thermodynamically stable with respect to these processes. In such a solution, it is the stationary size distribution Xn that is physically irrelevant and the fibril population is described by the equilibrium size distribution Cn from Eq. 5 or Eq. 11.

Changes in fibril solubility due to point mutations

The integrated van' t Hoff equation

Ce=Crexp(−LkBT), (12)

in which Cr (m−3) is a reference protein concentration, relates the equilibrium concentration Ce to the latent heat or enthalpy L (J) (per β-strand) of protein aggregation (e.g., Kashchiev and Auer (51) and Auer and Kashchiev (58)). As found elsewhere (58), in line with the Haas-Drenth lattice model of protein crystals (59), L is approximately given by half of the average binding energy 〈Eb〉 of a β-strand within the bulk fibrillar phase, i.e., L ≈ 〈Eb〉/2. For the fibril model considered here, we have 〈Eb〉 = 2(E + Eh) = 4(ψ + ψh)kBT, where E, Eh, ψ, and ψh are given by Eqs. 1, 2, 8, and 9. Hence, approximately,

L=E+Eh=2(ψ+ψh)kBT. (13)

If sW and sM are the supersaturations for a wild-type and a point-mutated protein, respectively, employing Eqs. 7 and 12, we find that the change Δs ≡ sM − sW in the supersaturation upon a point mutation of the wild-type protein at the same temperature T and monomer concentration C1 is of the form

Δs=LM−LWkBT. (14)

The latent heat LW or LM (per β-strand) of the wild-type protein or the mutant can be calculated from Eq. 13 when the corresponding binding energies E and Eh are known. Also, if Ce,W and Ce,M are the solubilities of the wild-type and the point-mutated protein, respectively, the mutation-affected change in the protein solubility at the same temperature can be characterized by the ratio

Ce,MCe,W=exp(LW−LMkBT). (15)

This formula follows from Eq. 12 provided the point mutation has practically no effect on Cr.

Results and Discussion

Application to Aβ40 nanofibrils

Our considerations pertain to that molecular structure proposed by Sachse et al. (60) for Aβ40 fibrils, in which the β-strand is formed by a long amino-acid stretch at the C-terminal tail of the protein monomer. As in our previous study (54), we rely on theoretical models (44,45) that identify the most aggregation-prone amino acids in proteins. The theoretical algorithm by Trovato et al. (45) predicts that amino acids 12–20 (VHHQKLVFF) and 31–40 (IIGLMVGGVV) are the most aggregation-prone ones (V = Valine, H = Histidine, Q = Glutamine, K = Lysine, L = Leucine, F = Phenylalanine, I = Isoleucine, G = Glycine, M = Methionine). Joint together, these 19 amino acids form a sequence that defines the β-strand in our nanofibril model (Fig. 1). The sequence-specific energy εjq of the hydrogen bond between amino acids j and q can vary in the interval [0, 2ε], depending on the frequency with which two residue types are found paired in neighboring β-strands within a β-sheet in globular proteins (see Eq. 3). For simplicity, we assume that the energy εh,jq of a hydrophobicity-mediated bond is the same for all amino-acid pairs, so that εh,jq = εh, and we set εh = ε/10.

With this set of parameter values, the interstrand binding energies E and Eh for the β-strands (VHHQKLVFFIIGLMVGGVV) arranged parallel within wild-type Aβ40 fibrils can be calculated from Eqs. 1–3, and are E = 25.4ε and Eh = 1.9ε (see also Table 1). Accordingly, the rounded-up ratio between the β-strand strong and weak binding energies is E/Eh = 14, and the fibril transition size is thus nt = 14 (Table 1) because of our assumption that it is given by the CNT formula (51) nt = E/Eh, which characterizes the fibril equilibrium shape. We note, however, that during nucleation the fibrils are under nonequilibrium conditions: on average, they grow and thus assume a kinetically determined growth shape that may differ considerably from the equilibrium one. Computer simulation data (see Fig. 2 in Zhang and Muthukumar (30)) indicate that the fibril kinetic aspect (length/thickness) ratio that quantifies the fibril growth shape can be several times greater than the thermodynamic aspect ratio E/Eh, i.e., that the fibrils can grow longer than it is thermodynamically expected. It should be kept in mind therefore that, actually, the fibril transition size nt may have values considerably greater than the value of E/Eh assumed in our analysis.

Table 1.

Parameter values related to the size distribution of nanosized fibrils of wild-type and point-mutated Aβ40 at T = 300 K; the corresponding basic hydrogen-bond energy is ε = 6.95 × 10−21 J

Aβ40 Wild-type V18N V18R V18P
E (J) 1.76 × 10−19 1.72 × 10−19 1.68 × 10−19 1.65 × 10−19
Eh (J) 1.32 × 10−20 1.32 × 10−20 1.32 × 10−20 1.32 × 10−20
ψ 21.3 20.8 20.3 19.9
ψh 1.59 1.59 1.59 1.59
nt 14 14 13 13
Ce (μM) 3.9 10.6 28.8 64.1

Aβ40 nanofibril size distribution: supersaturation dependence

The nanofibril size distribution for wild-type Aβ40 solution at T = 300 K and supersaturations s/ψh = 0.9, 1, 1.2, 2, and 2.5 are displayed in Fig. 3 by lines 0.9, 1, 1.2, 2, and 2.5, respectively. The lines are obtained from Eq. 10 by setting M = 300 (as in Cabriolu et al. (52)) and by using the ln and lh,n values from Table S1 in the Supporting Material and the ψ- and ψh-values following from Eqs. 8 and 9 and given in Table 1. According to Eq. 7, with ψh from Table 1, the above supersaturations correspond to supersaturation ratios C1/Ce = 4.20, 4.90, 6.78, 24.0, and 53.3, respectively.

Figure 3.

Figure 3

Stationary nanofibril size distribution Xn on (a) Xn1/5 and (b) log Xn scale according to Eq. 10 at T = 300 K and supersaturations s/ψh = 0.9, 1, 1.2, 2, and 2.5 (as indicated) for wild-type Aβ40.

As seen in Fig. 3, Eq. 10 predicts a series of peaks, each of them being at a certain fixed fibril size for high enough supersaturations and at a smaller, but again fixed, size for sufficiently low supersaturations. The first peak is positioned either at fibril size n′1 or at fibril size n″1 > n′1 that, due to our choice of the nanofibril evolution mechanism illustrated in Fig. 2, are given by n′1 = 1 (for 0 < s < 2ψh) and by n″1 = nt (for s > 2ψh), where nt = 14 and 2ψh = 3.18 because of the ψ- and ψh-values used in our calculation of Xn in Fig. 3. At s = 2ψh (line 2), the peak is plateaulike, extending from n = n′1 to n = n″1, i.e., from the monomer size to the fibril size nt for transition of the fibril from one-dimensional to two-dimensional aggregate.

Similarly, the fibril sizes n′j and n″j at which the second, third, etc. peaks are positioned at low or high supersaturations, respectively, are obtainable from the relations (j = 2,3,4,…),

nj′=j(j−1)nt (16)

(for 0 < s < 2ψh/j) and

nj″=j2nt (17)

(for s > 2ψh/j). At s = 2ψh/j, the jth peak is a plateau (jagged for j = 2,3,4,…) that extends from n = n′j to n = n″j. In Fig. 2, the first three nanofibrils of size n′j and of size n″j are colored pink and blue, respectively.

Fig. 2 and Eqs. 16 and 17 show that both the n′j-sized and the n″j-sized fibrils are constituted of j β-sheets, but their lengths m′j and m″j, respectively, are multiples of nt (except m′1 = 1):

mj′=(j−1)nt, (18)
mj″=jnt. (19)

Equations 16 and 17 show also that for s > 2ψh, i.e., for high enough supersaturations, all peaks (including the first one) remain fixed at characteristic or “magic” fibril sizes n″j given by Eq. 17. The n″j-sized fibril itself is j β-sheets thick and jnt β-strands long (see the blue fibrils in Fig. 2), i.e., its length m″j is determined by Eq. 19. This equation implies that when s > 2ψh, if plotted as a function of the nanofibril length m, the stationary size distribution of the nanofibrils will be multipeaked at magic lengths m″j, the peaks being at the same distance nt from their nearest neighbors on the m axis. We note, however, that this result about equidistanced peaks in the nanofibril length distribution characterizes the nanofibril shape sequence illustrated in Fig. 2. Deviations from this sequence, in particular regarding the length at which the nanofibril acquires the energetically very costly β-strand that gives birth of its subsequent β-sheet, could lead to different interpeak distances on the nanofibril length axis.

Combining Eq. 17 with the formula n∗j = j2nt + 1 for the successive nucleus sizes n∗j (52), we arrive at the equation (j = 1,2,3,4,…)

nj∗=nj″+1, (20)

which says that the jth fibril nucleus is just one β-strand bigger than the fibril corresponding to the jth peak at high enough supersaturations (see Fig. 2 in which the first three fibril nuclei are hatched, and the n″j-sized fibrils are blue). Equation 20 is of particular interest, for it seems to be a result of general validity when amyloid fibrils are nucleated by the mechanism of direct polymerization of β-strands and when s > 2ψh. According to this equation, with a negligible difference of one β-strand, the positions n″j of the peaks in a nanofibril size distribution that is obtained in a real or computer experiment at a high enough supersaturation s merely represent the sizes n∗j of the successive fibril nuclei.

Table S2 lists the first three values of n′j, m′j, n″j, and m″j in the respective s ranges. To get a feel of these values for the Aβ40 protein, we recall that the molecular mass of the protein monomer is 4.3 kDa (61), and that the distance between β-strands in the Aβ40 fibril is ∼0.47 nm (62). Hence, from Eqs. 17 and 19 with nt = 14, the first three peaks of the nanofibril mass or length distribution are at magic masses 4.3 n″j of 60.2, 241, and 542 kDa or lengths 0.47 m″j of 6.58, 13.2, and 19.7 nm provided the solution is at supersaturation s > 2ψh = 3.18.

The physical reason for which the size distribution Xn of nanosized fibrils is peaked at magic sizes n′j or n″j is the presence of deep local minima of the work Wn to form a fibril of n β-strands (see Fig. 3b of Cabriolu et al. (52)). The attachment of a β-strand to the end of an n′j-sized fibril or to the surface of an n″j-sized fibril requires considerable work so that the n′j- or n″j-sized fibrils become the most numerous in the solution and thus give rise to peaks in the nanofibril size distribution. As to the s value at which the jth peak is plateaulike, it coincides with that at which, according to CNT (Kashchiev and Auer (51), Eq. 13), a jβ-sheet is in thermodynamic equilibrium with the solution, i.e., it neither grows nor dissolves. We note as well that, regardless of the s value, a given peak concentration Xp,j is always higher than the subsequent concentration Xp,j+1, i.e., the peak concentrations of the nanofibrils obey the order Xp,1 ≥ Xp,2 ≥ Xp,3 ≥ ….

Clearly, Xn will be closer to a monotonically decreasing function of n when the work (−s + 2ψ)kBT (Kashchiev and Auer (51)) of thicknesswise β-strand attachment to the kinkless surface of any of the n″j-sized fibrils (Fig. 2) is sufficiently smaller than the thermal energy kBT. Thus, the condition for relatively low peaks in the stationary nanofibril size distribution reads

2ψ<1+s. (21)

This condition shows that, as usually ψ > 1, well-pronounced peaks at magic sizes (or lengths) are to be expected in the stationary size (or length) distributions of most amyloid nanofibrils (the effect of the supersaturation is quite small, because amyloid fibril nucleation occurs at s values considerably smaller than those of ψ (51,52)). For nanofibrils of shorter β-strands the peaks will be less pronounced, because ψ diminishes with decreasing β-strand length. In principle, any biophysicochemical factor that lessens the ψ-value will also contribute to the suppression of the Xn peaks and, hence, to the possible disappearance of the magic nanofibril sizes or lengths.

Preferred sizes, lengths, or thicknesses of Aβ oligomers or fibrils have been recorded in many experiments (e.g., (29,61–65)). In this respect, our finding of magic sizes is in qualitative agreement with experiment. No experimental data we are aware of, however, allows us using it for a quantitative verification of this finding. Reported histograms of the fibril mass-per-length ratio (60,61,63–69) exhibit one or more peaks, but pertain to portions of rather long fibrils and show that these usually contain an integer number of β-sheets. To reliably quantify the magic nanofibril sizes, we need histograms of the masses of entire fibrils with nanoscale lengths. To the best of our knowledge, only Goldsbury et al. (61) have obtained such a histogram (Fig. 4D in their article), but it is for pseudospherical rather than fibrillar Aβ40 aggregates and the authors could fit it by two Gaussian curves with maxima at masses of 311 and 554 kDa corresponding to 72 and 128 protein molecules. The experimental size distributions of Garai et al. (29) for solutions of Aβ40 also exhibit peaks at magic sizes represented by the aggregate hydrodynamic radii. Again, a quantitative comparison between our theory and the experiment of Garai et al. (29) is not possible. The reported size distributions are not stationary, the aggregate morphology is unknown, and the second peak of the size distributions is at radius of ∼50 nm. This radius corresponds to the rather large number of 1.2 × 105 protein molecules if, as in Garai et al. (29), one uses 4.3 nm3 for the Aβ40 molecular volume and assumes that the aggregates are spherical.

Figure 4.

Figure 4

Stationary nanofibril size distribution on (a) Xn1/5 and (b) log Xn scale according to Eq. 10 at T = 300 K and monomer concentration C1 = 120 μM for wild-type Aβ40 and its mutants V18N, V18R, and V18P: (black) line WT, wild-type; (red) line N, V18N; (green) line R, V18R; and (blue) line P, V18P.

Very interesting are as well the experimental data of Kellermayer et al. (62), which support our finding of magic nanofibril lengths. These authors have presented a histogram of most frequently observed increments of the lengths of epitaxially growing individual Aβ25-35 fibrils (the inset in Fig. 2a of Kellermayer et al. (62)). The histogram exhibits five successive peaks at 6.5, 13.3, 23.2, 32.5, and 40 nm. As noted by Kellermayer et al. (62), the nearly 7-nm interpeak distance “corresponds to a stretch of fibril containing ≈15 peptides along its length.” This is in close quantitative agreement with our finding for peaks in the Aβ40 nanofibril length distribution, which are equidistanced at 14 β-strands or, equivalently, 6.6 nm. However, this agreement is very likely to be fortuitous, because whereas the fibrils of Kellermayer et al. (62) elongate at a practically constant thickness, according to our model (Fig. 2) every subsequent fibril lengthening of nt β-strands is preceded by fibril thickening of one β-sheet.

Aβ40 nanofibril size distribution: effect of mutations

The presented theoretical framework enables us also to study the effect of point mutations on the nanofibril size distribution. In particular, at fixed T and C1, we examine how Xn is affected by the point mutations of residue 18 (V) with amino acids Asparagine (N), Arginine (R), and Proline (P), because the effect of these mutations of Aβ40 on the fibrillation kinetics has been investigated experimentally (35).

To be able to calculate Xn from Eq. 10 for each mutant, we need to know the corresponding fibril solubility Ce and energy parameters ψ and ψh that have different values for each mutant, because the binding energies E and Eh of the β-strands within the fibrils are different (see Table 1). For the wild-type Aβ40, we employ the experimentally obtained Ce = 3.9 μM at T = 300 K (29). As Ce has not been determined experimentally for any of the mutants, we find it theoretically by making use of Eqs. 13 and 15 and the ψ- and ψh-values from Table 1. The Ce values computed in this way for fibrils with point mutations V18N, V18R, and V18P are given in Table 1. Using the procedure outlined above for the wild-type Aβ40, from Eq. 10 we calculate Xn for each mutant by setting M = 300 (as in Cabriolu et al. (52)) and by using the ψ- and ψh-values from Table 1 and the ln and lh,n values from Table S1 and Table S3. For mutations V18N, V18R, and V18P the transition size nt = E/Eh has the values 14, 13, and 13, respectively, and is equal or nearly equal to the transition size nt = 14 for the wild-type protein (Table 1).

The nanofibril size distributions obtained at T = 300 K and C1 = 120 μM are shown in Fig. 4. At this concentration, the supersaturation for the wild-type protein and the three mutants V18N, V18R, and V18P can be calculated from Eq. 7 and is s = 3.43, 2.43, 1.43, and 0.63, respectively. As can be seen in Fig. 4, the main effect of the mutations is that the peaks for all magic nanofibril sizes n′j or n″j lose height. This is so because by considerably increasing the fibril solubility, the mutations lower the solution supersaturation, which leads to a strong decrease in the entire fibril population and, accordingly, in the peak heights. In contrast, the effect of the mutations on n′j or n″j is minor (because nt changes only from 14 to 13 for two of the mutants) and, as a result, the peak positions remain essentially the same. For mutant V18R, the second peak is at n′2 = 26, because the Ce value for this mutant is so great that the corresponding supersaturation ratio C1/Ce is too low for the peak to be at n″2 = 52.

The effect of mutations on the fibril population could be exemplified by considering the number of nanofibrils of 13 β-strands in a solution of volume V = 100 mL typically used in experiments. From Eq. 10 (see also Fig. 4) we calculate that whereas the number X13V of wild-type fibrils of size n = 13 is 1020, the V18N and V18R fibrils of the same size are much less numerous: the V18N ones are 9 × 1014, and the V18R ones are 1010. Remarkably, the fibrils of the same size for mutant V18P are practically absent from the solution, because their number is 4 × 105. It is worth noting also that the decrease of the peak heights for the different mutants that is seen in Fig. 4 is consistent with experiments on protein fibrillation kinetics (35), which reveal that the lag time before detectable fibrillation is longer for the mutants V18N and V18R than for the wild-type Aβ40; and that the mutant V19P is not detectable at all. This consistency is in support of the correlation reported earlier (54) between ANT nucleation rates of amyloid fibrils and experimentally measured fibrillation lag-times of wild-type and point-mutated Aβ proteins.

Conclusion

The analysis made illustrates the ability of the nucleation theory to describe the size distribution of amyloid nanofibrils in protein solutions when nucleation occurs by the mechanism of direct polymerization of β-strands into β-sheets. The atomistic modeling of the nanofibrils of successively layered β-sheets leads to a general formula (Eq. 10) for the stationary size distribution as a function of the protein concentration and of the temperature (via Ce, ψ, and ψh that, given the nanofibril shape sequence, are the only three theoretical parameters). Application of this formula to Aβ40 nanofibrils reveals the existence of a series of characteristic peaks in the size distribution, which are positioned at magic nanofibril sizes (or lengths) and which are due to the sufficiently deep local minima in the work for fibril formation. This finding of magic sizes or lengths is consistent with experimental results for the size distribution of aggregates in solutions of Aβ40 proteins.

We believe our analysis provides a new opportunity to obtain information about the sizes of the successive fibril nuclei, because according to Eq. 20, these sizes are practically equal to the magic sizes at which the nanofibril size distribution is peaked when the solution supersaturation is sufficiently high. Also, we believe our atomistic approach makes it possible to gain novel insight into the effect of point mutations on the size distribution of amyloid nanofibrils, an effect that may play a role in experimentally observed substantial differences in the fibrillation lag-times of wild-type and point-mutated Aβ proteins.

The results obtained remain without quantitative verification because of the lack of suitable experimental or simulation data for the size distribution of amyloid nanofibrils. It is hoped that our study will inspire new real and computer experiments especially aimed at investigating this distribution and/or the magic nanofibril sizes or lengths.

Acknowledgments

This work was supported by Engineering and Physical Science Research Council grant No. EP/G026165/1.

Supporting Material

Document S1. Three tables
mmc1.pdf (49.7KB, pdf)

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Associated Data

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Supplementary Materials

Document S1. Three tables
mmc1.pdf (49.7KB, pdf)

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