Divergence and correlated evolution of male wing spot and courtship display between Drosophila nepalensis and D.trilutea

Male-specific wing spots are usually associated with wing displays in the courtship behavior of Drosophila and may play important roles in sexual selection.Two closely related species,D.nepalensis and D.trilutea,differ in wing spots and scissoring behavior.Here,we compare male morphological characters,pigmentation intensity of male wing spots,wing-scissoring behavior,courtship songs,and reproductive isolation between 2 species.F1 fertile females and sterile males result from the cross between females of D.nepalensis and males of D.trilutea.The pigmentation of wing spots is significantly weaker in D.trilutea than in D.nepalensis and the F1 hybrid.Males scissor both wings in front of the female during courtship,with a posture spreading wings more widely,and at a faster frequency in D.nepalensis than in D.trilutea and the F1s.Males of D.trilutea vibrate wings to produce 2 types(A and B)of pulse songs,whereas D.nepalensis and the F1s sing only type B songs.The incidence of wing vibration and scissoring during courtship suggests that wing vibration is essential but scissoring is a facultative courtship element for successful mating in both species.The association between the darker wing spots with more elaborate scissoring might be the consequence of correlated evolution of these traits in D.nepalensis;however,D.trilutea retains wing scissoring during courtship despite having weaker pigmentation of wing spots.The genetic architecture of 2 traits differs in the F1s,consistent with maternal or sex-linked effects for spots but nonadditive effects for scissoring.

Correlations of the Evolution of a CCOPE Squall Line with Surface Thermodynamics and Kinematic Fields

A midlatitude squall line passed over the array of the Cooperative Convective Precipitation Experiment (CCOPE) on 1 August 1981. The structure and evolution of the squall line, and the correlations of the storm with surface thermodynamics and kinematic fields are investigated, mainly by using radar and surface mesonet data in CCOPE. The storm-wide precipitation efficiency is also estimated.The squall line was of an obvious process of metabolism. Thirty-four cells formed successively in front of the primary storm and eventually merged into it during the period 1700-2010 MDT. The newest cells formed near surface equivalent potential temperature maxima, and near surface moisture flux convergence zones or / and the 'temperature break lines'. The thunderstorm rainfall, with the precipitation efficiency of 54%, lags 25-30 min behind the moisture flux convergence on the average.

Quantum Correlations Evolution Asymmetry in Quantum Channels

It was demonstrated that the entanglement evolution of a specially designed quantum state in the bistochastic channel is asymmetric. In this work, we generalize the study of the quantum correlations, including entanglement and quantum discord, evolution asymmetry to various quantum channels. We found that the asymmetry of entanglement and quantum discord only occurs in some special quantum channels, and the behavior of the entanglement evolution may be quite different from the behavior of the quantum discord evolution. To quantum entanglement, in some channels it decreases monotonously with the increase of the quantum channel intensity. In some other channels, when we increase the intensity of the quantum channel, it decreases at first, then keeps zero for some time, and then rises up. To quantum discord, the evolution becomes more complex and you may find that it evolutes unsmoothly at some points. These results illustrate the strong dependence of the quantum correlations evolution on the property of the quantum channels.

Pseudorapidity dependence of short-range correlations from a multi-phase transport model

Using a multi-phase transport model（AMPT） that includes both initial partonic and hadronic interactions, we study neighboring bin multiplicity correlations as a function of pseudorapidity in Au＋Au collisions at √sNN= 7.7- 62.4 GeV.It is observed that for √sNN〈19.6 GeV Au＋Au collisions, the short-range correlations of final particles have a trough at central pseudorapidity, while for √sNN 〉19.6 GeV AuAu collisions,the short-range correlations of final particles have a peak at central pseudorapidity. Our findings indicate that the pseudorapidity dependence of short-range correlations should contain some new physical information, and are not a simple result of the pseudorapidity distribution of final particles. The AMPT results with and without hadronic scattering are compared. It is found that hadron scattering can only increase the short-range correlations to some level, but is not responsible for the different correlation shapes for different energies. Further study shows that the different pseudorapidity dependence of short-range correlations are mainly due to partonic evolution and the following hadronization scheme.