We analyse the evolution of postponed seed germination in temporally and spatially homogeneous habitats under the assumption that sibling seedlings compete because of clumped seed dispersal. The seed germination trait is assumed to be affected by two sets of autosomal genes. One set controls a germi
Evolution of Seed Dormancy Due to Sib Competition: Effect of Dispersal and Inbreeding
β Scribed by YUTAKA KOBAYASHI; NORIO YAMAMURA
- Publisher
- Elsevier Science
- Year
- 2000
- Tongue
- English
- Weight
- 213 KB
- Volume
- 202
- Category
- Article
- ISSN
- 0022-5193
No coin nor oath required. For personal study only.
β¦ Synopsis
The e!ect of dispersal and inbreeding on the evolution of seed dormancy to avoid sib competition is theoretically investigated, using a model which assumes a plant population with patchy spatial structure in a constant environment. Applying the inclusive "tness method, the evolutionarily stable dormancy rates are analytically derived for three cases: (a) an asexual haploid population, (b) a diploid-hermaphrodite population in which the dormancy rate is controlled by seeds, and (c) a diploid-hermaphrodite population in which the dormancy rate is controlled by mother plants. The evolutionarily stable dormancy rates decrease in the order of case (c), case (a), and case (b). In all the cases, the evolutionarily stable dormancy rates increase with decreasing the dispersal rate. Although inbreeding generally increases the evolutionarily stable dormancy rates, inbreeding due to sel"ng reduces the rate exceptionally in case (c).
π SIMILAR VOLUMES
Dispersal is often presented as a mechanism to avoid competition among relatives and inbreeding depression. However, the formal analysis of the e!ects of both these factors on the evolution of dispersal has only been conducted in few studies with strong restrictive assumptions. In this paper, I "rst
We study the evolution and equilibrium values of velocity dispersions of particles in a circumplanetary disk, taking into account both inelastic collisions and gravitational interactions between particles. For a disk of particles with a Rayleigh distribution of orbital eccentricities and inclination