The isotopic resonance hypothesis postulates that certain isotopic compositions of chemical elements affect kinetics of chemical reactions involving molecules built of these elements. The isotopic compositions for which this effect is predicted are called resonance isotopic compositions. Fundamentally, the IsoRes hypothesis relies on a postulate that less complex systems exhibit faster kinetics than equivalent but more complex systems. Furthermore, system’s complexity is affected by its symmetry, and symmetry of reactants may be affected by their isotopic composition. The term “resonance” relates to the use of this term in nuclear physics, where peaks in the dependence of a reaction cross section upon energy are called “resonances”. Similarly, a sharp increase in the reaction kinetics as a function of the average isotopic mass of a certain element is called here a resonance.
History of formulation
The concept of isotopes developed from radioactivity. The pioneering work on radioactivity by Henri Becquerel, Marie Curie and Pierre Curie was awarded the . Later Frederick Soddy would take radioactivity from physics to chemistry and shed light on the nature of isotopes, something with rendered him the . The question of stable, non-radioactive isotopes was more difficult and required the development by Francis Aston of a high-resolution mass spectrograph, which allowed the separation of different stable isotopes of one and the same element. Francis Aston was awarded the for this achievement. With his enunciation of the whole-number rule, Aston solved a problem that had riddled chemistry for a hundred years. The understanding was that different isotopes of a given element would be chemically identical. It was discovered in the 1930s by Harold Urey in 1932. It was early on found that the deuterium content had a profound effect on chemistry and biochemistry. In the linear approximation, the effect of isotopic substitution is proportional to the mass ratio of the heavy and light isotope. Thus chemical and biological effects of heavier isotopes of the “biological” atoms C, N and O are expected to be much smaller since the mass ratios for the normal to heavier isotopes are much closer to unity than the factor two for hydrogen to deuterium. However, it has been reported in 1930s, and then again in 1970s and 1990s, as well as recently, that relatively small changes in the content of the heavy isotope of hydrogen, deuterium, has profound effects on biological systems. These strong nonlinear effects could not be fully rationalized based on the known concepts of the isotopic effects. These and other observations make it possible that isotopes have a much more profound importance than could ever have been imagined by the pioneers. In 2011 formulated the isotope resonance hypothesis. It originated in the following, unexpected observation. Define ΔMm = Mmono - Mnom, where Mmono is the monoisotopic mass and Mnom is the nominal mass, i.e., the number of nucleons. ΔMm is a constant in the whole Universe. Define ΔMis = Mav - Mmono, where Mav is the average isotopic mass. Obviously ΔMis depends on the precise isotopic composition for a given molecule. Finally define NMD = 1000ΔMm/Mnom and NIS = 1000ΔMis/Mnom, where NMD and NIS are the normalized isotopic defect and shift, respectively. If NIS is plotted as a function of NMD for a large number of terrestrial peptides, one would anticipate a homogenous distribution of data points. This is not what was found by Zubarev’s team, instead they found band gap in the distribution with a narrow line in the middle. This serendipitous discovery led Zubarev to formulate the isotope resonance hypothesis.
Analogues in science
As an example of isotopic symmetry affecting the kinetics of physic-chemical processes, see mass independent isotope fractionation in ozone O3.
According to the IsoRes hypothesis, there are certain resonance isotopic compositions at which terrestrial organisms thrive best. Curiously, average terrestrial isotopic compositions are very close to a resonance affecting a large class of amino acids and polypeptides, the molecules of outmost importance for life. Thus, the IsoRes hypothesis suggests that early life on Earth was aided, perhaps critically, by the proximity to an IsoRes. In contrast, there is no strong resonance for then atmosphere of Mars, which led to a prediction that life could not have originated on Mars and that the planet is probably sterile.
Other nontrivial predictions
One would expect that enrichment of heavy isotopes leads to progressively slower reactions, but the IsoRes hypothesis suggests that there exist certain resonance compositions for which kinetics increases even for higher abundances of heavy stable isotopes. For example, at 9.5% 13C, 10.9% 15N and 6.6% 18O and normal deuterium composition, a very strong resonance is predicted. Yet another nontrivial prediction of the IsoRes hypothesis is that at ≈250-350 ppm deuterium content, the terrestrial resonance becomes “perfect”, and the rates of biochemical reactions and growth of terrestrial organisms further increase. This prediction seems to be matched by at least some experimental observations.
Experimental verification
The IsoRes hypothesis has been tested experimentally by means of growth of E. coli and found to be supported by extremely strong statistics. Particular strong evidence of faster growth was found for the “super-resonance”. Fig. 1. 2D plot of molecular masses of 3000 E. coli tryptic peptides. A – terrestrial isotopic compositions ; B – 18O abundance is increased by 20%, which destroyed the terrestrial resonance; C – isotopic compositions of the “super-resonance”, where all dots are perfectly aligned. Adapted from ref. 4.
