Categories Astroparticle Physics 4PN conservative dynamics in the EFT approach

4PN conservative dynamics in the EFT approach

  • 12 views

  • 0 favorites

  • uploaded March 1, 2022

Stefano Foffa (Université de Genève),

Kolleg Mathematik Physik Berlin, 2019

Tags:
Categories: Astroparticle Physics
Date of recording: 2019-11-20
Presenter: Stefano Foffa

More Media in "Astroparticle Physics"

Observational cosmology - Dr. Jochen Liske
Observational cosmology - Dr. Jochen Liske
Multi messenger Astroparticle physics - Dr. Francesca Calore
Multi messenger Astroparticle physics - Dr. Francesca Calore
APPEC Town Meeting Berlin 2022 - Part 3
APPEC Town Meeting Berlin 2022 - Part 3
APPEC Town Meeting Berlin 2022 - Part 2
APPEC Town Meeting Berlin 2022 - Part 2
APPEC Town Meeting Berlin 2022 - Part 1
APPEC Town Meeting Berlin 2022 - Part 1
Laying of the foundation stone | New building CTA SDMC and canteen
Laying of the foundation stone | New building CTA SDMC and canteen
Grundsteinlegung | Neubau CTA SDMC und Kantine
Grundsteinlegung | Neubau CTA SDMC und Kantine
Analytic Integration Methods for Master Integrals in QFT
Analytic Integration Methods for Master Integrals in QFT
Gravitational scattering and radiation in the eikonal approach
Gravitational scattering and radiation in the eikonal approach
Spinning black holes versus quantum higher-spin particles
Spinning black holes versus quantum higher-spin particles
Feynman integrals: from collisions to intersections
Feynman integrals: from collisions to intersections
Binary Black Holes and Gluon Scattering Amplitudes
Binary Black Holes and Gluon Scattering Amplitudes
Gravitational scattering/radiation in/from transplanckian-energy collisions
Gravitational scattering/radiation in/from transplanckian-energy collisions
Field theory for gravity at all scales
Field theory for gravity at all scales
Approaches to classical spins and their gravitomagnetic interaction
Approaches to classical spins and their gravitomagnetic interaction
Amplitudes for Classical Solutions
Amplitudes for Classical Solutions
Simplifying PerturbativeGravity
Simplifying PerturbativeGravity
From theory to astrophysics: Observing the first colliding compact objects
From theory to astrophysics: Observing the first colliding compact objects
Numerical-relativity simulations of compact object binaries
Numerical-relativity simulations of compact object binaries
Applications of the ADM formalism to the relativistic two-body problem
Applications of the ADM formalism to the relativistic two-body problem
Classical effective action of dilaton gravity and the double copy
Classical effective action of dilaton gravity and the double copy
POST-NEWTONIAN MOTION AND RADIATIONOF COMPACT BINARY SYSTEMS
POST-NEWTONIAN MOTION AND RADIATIONOF COMPACT BINARY SYSTEMS
PN, PM, MPM, EOB, SF, EFT, ACV, BCJ, BCRSSZ and All That
PN, PM, MPM, EOB, SF, EFT, ACV, BCJ, BCRSSZ and All That
Spin holonomy and scattering angle in a PM approximation
Spin holonomy and scattering angle in a PM approximation
4PN conservative dynamics in the EFT approach
4PN conservative dynamics in the EFT approach
From Boundary Data to Bound States
From Boundary Data to Bound States
Towards 5PN accuracy in Non Relativistic General Relativity
Towards 5PN accuracy in Non Relativistic General Relativity
The interaction potential between point masses at the fifth Post-Newtonian order
The interaction potential between point masses at the fifth Post-Newtonian order
Abenteuer Astroteilchenphysik - Energiereiche Teilchen aus dem Kosmos
Abenteuer Astroteilchenphysik - Energiereiche Teilchen aus dem Kosmos
PeV Cosmic Ray Acceleration in the Supernova Post Breakout Expansion Phase: Kinetic-magnetohydrodynamic Simulations
PeV Cosmic Ray Acceleration in the Supernova Post Breakout Expansion Phase: Kinetic-magnetohydrodynamic Simulations