On the temperature dependence of amide I intensities of peptides in solution

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Abstract

Temperature dependence of the amide I/I′ spectral intensities is investigated for N-methylacetamide (NMA) as a model compound for the peptide bond in D2O and three organic solvents with different polarities (dimethyl sulfoxide (DMSO), acetonitrile and 1,4-dioxane). The total amide I/I′ intensity (dipole strength) systematically decreases in less polar solvents as well as with the increasing temperature. Decreased solvent polarity results in the narrowing of the amide I bandwidths, while increasing temperature predominantly reduces the peak absorbance, with only a small effect on the spectral width. In D2O, the NMA amide I′ dipole strength decreases by 1.7 × 10−4 Debye2/deg, in DMSO, acetonitrile and 1,4-dioxane by 1.0 × 10−4 Debye2/deg. The amide I/I′ intensity variations in the non-protic solvents rule out hydrogen bonding as the sole source of these effects. The experimental NMA amide I dipole strengths in the organic solvents are accurately described by a simple theory based on the Onsager reaction field with temperature-dependent solvent dielectric constant, refractive index and the solute molecular cavity, which can be approximated using NMA density. Experimental results are compared to density functional theory (DFT) BPW91/cc-pVDZ/Onsager calculations. The computations significantly overestimate the absolute experimental amide I intensities, but comparison of the relative values underscores the importance of the temperature-dependent molecular cavity dimension (density) as well as the frequency-dependent response of the reaction field (index of refraction) for describing the amide I spectral intensities in polar solvents. Correlations between temperature-dependent amide I frequencies and intensities, and their possible utility for analyses of the temperature-dependent peptide and protein infrared spectroscopy (IR) spectra are discussed.

Introduction

Infrared spectroscopy (IR) is frequently used for studies of peptide and protein structures and dynamics of the structural transitions during protein folding or function [1]. Several advantages of the IR, such as higher resolution compared to the electronic spectroscopies, and fast intrinsic time-scale compared to the NMR, have made IR spectroscopy a technique of choice, for example, for numerous dynamic studies of peptide and protein folding [2], [3], [4], [5]. On the other hand, one of the disadvantages for investigations of protein structural properties is that most commonly used denaturants absorb strongly in the IR, interfering with the structurally sensitive protein signals. As a consequence, temperature is most often used to induce protein unfolding in the IR spectroscopic studies. The temperature-dependent IR spectra can, however, be complicated by the temperature-dependent changes unrelated to the peptide or protein structural properties. Such temperature effects must be well understood for the IR spectroscopy to provide accurate and reliable information about peptide and protein structure.

The majority of peptide and protein IR studies focus on the amide I band (predominantly amide Cdouble bondO bond stretching, often measured in D2O as amide I′ for N-deuterated peptides) since its conformational sensitivity has been best established [1], [6], [7]. Most frequently, amide I/I′ frequencies are the basis for structural assignments and the amide I/I′ frequency shifts for the interpretation of structural changes. In the recent study, we have investigated the temperature dependence of the peptide amide I/I′ vibrational frequencies in solution [8]. We found that an α-helical oligopeptide, random coil poly-l-lysine and a simple amide N-methylacetamide (NMA) exhibit the same amide I′ frequency shifts with temperature in D2O. To understand the origin of these effects, we measured the amide I frequencies of NMA as a function of temperature in organic solvents of different polarities: dimethyl sulfoxide (DMSO), acetonitrile and 1,4-dioxane. Similar temperature dependence of the amide I vibrational frequencies in all these solvents demonstrated that the dominant cause for the spectral shifts is not hydrogen bonding (to the amide Cdouble bondO), which is the most common interpretation. The frequency shifts in the organic solvents can be quantitatively explained by Buckingham theory [9] based on a simple, continuum model for the solvent, which takes into account the temperature dependence of the dielectric constant, index of refraction and density.

In this report we focus on the amide I/I′ intensities and their changes with temperature. Overall, spectral intensities have received much less attention than the vibrational frequencies, even though the intensities are equally important in determining the appearance of the experimental amide I spectral contours. While in the gas phase the IR absorption intensities are temperature independent, at least in the harmonic approximation [10], the amide I intensity, along with its frequency, is highly sensitive to the solvent environment. For example, the amide I dipole strength of NMA has been shown to more than double between acetonitrile and aqueous solution [11]. This effect could be, again, expected to arise primarily from hydrogen bonding, as suggested by studies on NMA association in CH3Cl [12] and of NMA and isotopically labeled peptides in D2O at cryogenic temperatures [13]. However, bulk solvent electrostatics may play an important, or even dominant role, as in the case of the vibrational frequency shifts [8], [11], and as also suggested by theoretical simulations of the NMA spectra with explicit and implicit solvent models [11]. Since the dielectric properties of the solvents are temperature dependent, so will be the solvent-induced effects on the spectral intensities [14].

It is perhaps well appreciated that the spectral intensities inherently depend on temperature, but the IR studies of peptide or protein thermal denaturation seldom account for any intrinsic temperature dependence of the spectra. In order to reliably extract the structural information, it is necessary to separate the temperature dependence of the spectral changes arising from structural transitions from those due to the solvent and other structure unrelated effects. To date, and to our best knowledge, no systematic study of the amide infrared intensities as a function of solvent and temperature has been reported. We again use NMA as a model for the amide bond to eliminate all possible effects from the conformational equilibria, the Buckingham theory [9] and density functional theory (DFT) calculations to quantitatively model the temperature-dependent amide I spectral intensities under different solvent conditions.

Section snippets

Experimental

All solvents used in this study were of analytical or better grade. Acetonitrile and 1,4-dioxane were used without further purification. DMSO was found to contain a significant amount of water and therefore was dehydrated over activated molecular sieves; the dryness was evidenced by a complete absence of the water infrared (IR) absorption bands. NMA was purchased from Sigma–Aldrich and D2O was from Cambridge Isotope Laboratories.

To obtain accurate absolute intensities, repeated IR spectral

Results and discussion

Experimental NMA amide I′ spectra in D2O and amide I in DMSO, acetonitrile and 1,4-dioxane are shown in Fig. 1. For all studied solvents, nearly symmetric absorption bands with slight inhomogeneous broadening toward the lower frequencies are observed. Symmetric profiles imply monomeric NMA, as can be expected at relatively low concentrations [15]. Although the inhomogeneous broadening could be caused by intermolecular association, this would result in concentration and, most likely,

Conclusion

We have investigated the intrinsic temperature dependence of the amide I IR intensities in solution, using NMA as a model system. The NMA amide I intensity depends significantly on the solvent as well as on temperature. Interestingly, the solvent polarity seems to affect predominantly the bandwidths, while the increase in temperature is manifested by decrease in the peak absorption, but without significant broadening. A simple theory based on the Onsager reaction field was used to

Acknowledgements

This work was supported by the Faculty Grant-in-Aid and Basic Research Grant programs of the University of Wyoming. The computations were made possible by the National Science Foundation under the following NSF programs: Partnerships for Advanced Computational Infrastructure, Distributed Terascale Facility (DTF) and Terascale Extensions: Enhancements to the Extensible Terascale Facility. Loren Ackels was supported in part by the University of Wyoming EPSCoR undergraduate research fellowship.

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