| Literature DB >> 35482933 |
Colin Olito1, Suvi Ponnikas1,2, Bengt Hansson1, Jessica K Abbott1.
Abstract
The evolution of suppressed recombination between sex chromosomes is widely hypothesized to be driven by sexually antagonistic selection (SA), where tighter linkage between the sex-determining gene(s) and nearby SA loci is favored when it couples male-beneficial alleles to the proto-Y chromosome, and female-beneficial alleles to the proto-X. Despite limited empirical evidence, the SA selection hypothesis overshadows several alternatives, including an incomplete but often-repeated "sheltering hypothesis" that suggests that expansion of the sex-linked region (SLR) reduces homozygous expression of partially recessive deleterious mutations at selected loci. Here, we use population genetic models to evaluate the consequences of deleterious mutational variation for the evolution of neutral chromosomal inversions expanding the SLR on proto-Y chromosomes. We find that SLR-expanding inversions face a race against time: lightly loaded inversions are initially beneficial, but eventually become deleterious as they accumulate new mutations, and must fix before this window of opportunity closes. The outcome of this race is strongly influenced by inversion size, the mutation rate, and the dominance coefficient of deleterious mutations. Yet, small inversions have elevated fixation probabilities relative to neutral expectations for biologically plausible parameter values. Our results demonstrate that deleterious genetic variation can plausibly drive recombination suppression in small steps and would be most consistent with empirical patterns of small evolutionary strata or gradual recombination arrest.Entities:
Keywords: Chromosomal inversion; indirect selection; mutation; recombination suppression; sex chromosomes
Mesh:
Year: 2022 PMID: 35482933 PMCID: PMC9324078 DOI: 10.1111/evo.14496
Source DB: PubMed Journal: Evolution ISSN: 0014-3820 Impact factor: 4.171
Figure 1Illustration of deterministic fitness and frequency dynamics for inversions initially loaded with different numbers of deleterious alleles. Results are shown for inversions of length three different dominance scenarios ( corresponding to each column of panels, left to right). Panels (a)–(c) show the fitness of SLR‐expanding inversions on a Y chromosome relative to the average fitness of all Y chromosomes (color coded lines). Points indicate when the corresponding inversions dropped below a frequency of 10−5, where they became effectively extinct, while stars indicate when an inversion reached a frequency of (), at which point they were considered to have fixed. Panels (d)–(f) show the inversion frequency dynamics (color coded lines) and illustrate that despite being initially beneficial, lightly loaded inversions (i) are not expected to deterministically rise to high frequencies unless deleterious mutations are strongly recessive; and (ii) will eventually become deleterious and crash to extinction (see also Figs. S1–S3 in Appendix C). Panels (f)–(i) illustrate the deleterious allele frequency dynamics at W loci on the inversion (; red line), and both W and D loci on X chromosomes in ovules/eggs ( and ; black solid and dotted lines, respectively) for the representative case of inversions initially loaded with relatively few deleterious alleles ( for G,H; for I). Results were generated using the following parameter values: , , , .
Figure 2Fixation probabilities estimated from Wright–Fisher simulations plotted as a function of inversion length for Autosomal (panels a and b) and SLR‐expanding (panels c and d) inversions on Y chromosomes. Point shapes indicate different chromosome‐arm wide mutation rates relative to selection (i.e., different values of U), which influence the average numbers of deleterious mutations carried by a standard‐arrangement chromosome (). Dashed horizontal lines indicate the corresponding expected fixation probability for a neutral allele for the same population size, and hence correspond to values of for autosomal inversions, and for Y‐linked inversions. Other parameter values were set to: , , .