13,644 research outputs found
Sympathy and Punishment: Evolution of Cooperation in Public Goods Game
An important way to maintain human cooperation is punishing defection. However, since punishment is costly, how can it arise and evolve given that individuals who contribute but do not punish fare better than the punishers? This leads to a violation of causality, since the evolution of punishment is prior to the one of cooperation behaviour in evolutionary dynamics. Our public goods game computer simulations based on generalized Moran Process, show that, if there exists a \'behaviour-based sympathy\' that compensates those who punish at a personal cost, the way for the emergence and establishment of punishing behaviour is paved. In this way, the causality violation dissipates. Among humans sympathy can be expressed in many ways such as care, praise, solace, ethical support, admiration, and sometimes even adoration; in our computer simulations, we use a small amount of transfer payment to express \'behaviour-based sympathy\'. Our conclusions indicate that, there exists co-evolution of sympathy, punishment and cooperation. According to classical philosophy literature, sympathy is a key factor in morality and justice is embodied by punishment; in modern societies, both the moral norms and the judicial system, the representations of sympathy and punishment, play an essential role in stable social cooperation.Public Goods Game, Cooperation, Social Dilemma, Co-Evolution, Sympathy, Punishment
Asteroid (3200) Phaethon: colors, phase curve, limits on cometary activity and fragmentation
We report on a multi-observatory campaign to examine asteroid 3200 Phaethon
during its December 2017 close approach to Earth, in order to improve our
measurements of its fundamental parameters, and to search for surface
variations, cometary activity and fragmentation. The mean colors of Phaethon
are B-V = 0.702 +/- 0.004, V-R = 0.309 +/- 0.003, R-I = 0.266 +/- 0.004,
neutral to slightly blue, consistent with previous classifications of Phaethon
as a F-type or B-type asteroid. Variations in Phaethon's B-V colors (but not
V-R or R-I) with observer sub-latitude are seen and may be associated with
craters observed by the Arecibo radar. High cadence photometry over phases from
20 to 100 degrees allows a fit to the values of the HG photometric parameters;
H = 14.57 +/- 0.02, 13.63 +/- 0.02, 13.28 +/- 0.02, 13.07 +/- 0.02; G = 0.00
+/- 0.01, -0.09 +/- 0.01, -0.10 +/- 0.01, -0.08 +/- 0.01 in the BVRI filters
respectively; the negative G values are consistent with other observations of F
type asteroids. Light curve variations were seen that are also consistent with
concavities reported by Arecibo, indicative of large craters on Phaethon's
surface whose ejecta may be the source of the Geminid meteoroid stream. A
search for gas/dust production set an upper limit of 0.06 +/- 0.02 kg/s when
Phaethon was 1.449 AU from the Sun, and 0.2 +/- 0.1 kg/s at 1.067 AU. A search
for meter-class fragments accompanying Phaethon did not find any whose on-sky
motion was not also consistent with background main belt asteroids.Comment: Accepted by the Astronomical Journal, 15 pages, 8 figures, 1 animated
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