| Records |
| Author |
Hochart, A. |
| Title |
Unique Ergodicity of Deterministic Zero-Sum Differential Games |
Type |
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| Year |
2021 |
Publication |
Dynamic Games And Applications |
Abbreviated Journal |
Dyn. Games Appl. |
| Volume |
11 |
Issue |
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Pages |
109-136 |
| Keywords |
Differential games; Hamilton-Jacobi equations; Viscosity solutions; Ergodicity; Limit value |
| Abstract |
We study the ergodicity of deterministic two-person zero-sum differential games. This property is defined by the uniform convergence to a constant of either the infinite-horizon discounted value as the discount factor tends to zero, or equivalently, the averaged finite-horizon value as the time goes to infinity. We provide necessary and sufficient conditions for the unique ergodicity of a game. This notion extends the classical one for dynamical systems, namely when ergodicity holds with any (suitable) perturbation of the running payoff function. Our main condition is symmetric between the two players and involve dominions, i.e., subsets of states that one player can make approximately invariant. |
| Address |
[Hochart, Antoine] Univ Adolfo Ibanez, Fac Ingn & Ciencia, Diagonal Las Torres 2640, Santiago, Chile, Email: antoine.hochart@gmail.com |
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Thesis |
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| Publisher |
Springer Birkhauser |
Place of Publication |
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Editor |
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| Language |
English |
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Edition |
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| ISSN |
2153-0785 |
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| Notes |
WOS:000527444200001 |
Approved |
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| Call Number |
UAI @ eduardo.moreno @ |
Serial |
1148 |
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| Author |
Dempsey, A.M.; Munoz, D.J.; Lithwick, Y. |
| Title |
Outward Migration of Super-Jupiters |
Type |
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| Year |
2021 |
Publication |
Astrophysical Journal Letters |
Abbreviated Journal |
Astrophys. J. Lett. |
| Volume |
918 |
Issue |
2 |
Pages |
L36 |
| Keywords |
GIANT PLANETS; ECCENTRIC MODES; DENSITY WAVES; DISK; ACCRETION; EVOLUTION; SATELLITES; VISCOSITY; GAPS |
| Abstract |
Recent simulations show that giant planets of about 1 M (J) migrate inward at a rate that differs from the type II prediction. Here we show that at higher masses, planets migrate outward. Our result differs from previous ones because of our longer simulation times, lower viscosity, and boundary conditions that allow the disk to reach a viscous steady state. We show that, for planets on circular orbits, the transition from inward to outward migration coincides with the known transition from circular to eccentric disks that occurs for planets more massive than a few Jupiters. In an eccentric disk, the torque on the outer disk weakens due to two effects: the planet launches weaker waves, and those waves travel further before damping. As a result, the torque on the inner disk dominates, and the planet pushes itself outward. Our results suggest that the many super-Jupiters observed by direct imaging at large distances from the star may have gotten there by outward migration. |
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| ISSN |
2041-8205 |
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| Notes |
WOS:000696692000001 |
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| Call Number |
UAI @ alexi.delcanto @ |
Serial |
1469 |
| Permanent link to this record |
