Generation, evolution, and observations of cosmological magnetic fields

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Sessions*

Course "Simulations of Early Universe Magnetohydrodynamics" day 4

Course "Simulations of Early Universe Magnetohydrodynamics" day 3

Course "Simulations of Early Universe Magnetohydrodynamics" day 2

Course "Simulations of Early Universe Magnetohydrodynamics" day 1

Preparation session for course "Simulations of Early Universe Magnetohydrodynamics"

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Contributions*

Backreaction from magnetic fields generated during inflation

Challenges in understanding primordial magnetic fields and its evolution (remote)

Charge transfer induced by chiral plasma instability

CMB spectral distortions meet PMFs

Connecting the observed and simulated cosmic web to primordial magnetism

Constraining inflationary magnetogenesis and reheating via GWs in light of PTA data

Constraints on extragalactic magnetic fields from ultra-high-energy cosmic rays

Cosmic magnetic field probes with electromagnetic cascades and cosmic rays

Cosmic Recombination in the Presence of Primordial Magnetic Fields (remote)

Cosmological Seed Magnetic Field from Inflation

Cosmological simulations including magnetic fields and realistic feedback from galaxies

Cosmological-scale magnetic fields from galactic outflows

CR propagation in intermittent magnetic fields

CRPropa 3.2 - a public framework for high-energy astroparticle simulations

Dark matter minihalos from primordial magnetic fields

Efficient subsonic turbulent dynamo during cosmic RD era

Evolution of Cosmological Magnetic Fields from Early to Late Times

Exploring the PMF imprints through rotation measure in the rarified cosmic regions

Fluid and Magnetic Spectra in First-Order Phase Transitions

General Relativistic Entropic Acceleration (GREA): Dark Energy from First Principles

Gravitational Waves from Chiral Plasma Instability in Standard Cosmology

Hints of magnetic helicity in the gamma-ray background?

How's Schwinger effect affect primordial Magnetogenesis?

IceCube/CTAO

Imprints of primordial curvature perturbations on inflationary magnetic fields

Introduction (in session "Course "Simulations of Early Universe Magnetohydrodynamics" day 1")

Lattice Simulations of Axion-U(1) Inflation

Lecture 5. Cosmology (in session "Course "Simulations of Early Universe Magnetohydrodynamics" day 3")

Lecture 6a. MHD in an expanding universe (in session "Course "Simulations of Early Universe Magnetohydrodynamics" day 3")

Lecture 6b. MHD in an expanding universe (in session "Course "Simulations of Early Universe Magnetohydrodynamics" day 3")

Lecture 7. Magnetic chiral dynamo (in session "Course "Simulations of Early Universe Magnetohydrodynamics" day 4")

Lecture 8. Gravitational waves (in session "Course "Simulations of Early Universe Magnetohydrodynamics" day 4")

Magnetic dynamo in SWIFT simulations

Magnetic field seeds from black holes accretion disks

Magnetic fields effects on particle interactions strength in the early universe

Magnetic fields in galaxy clusters

Magnetic reconnection in the early Universe

Magnetism footprints in cosmological envirnments

Magnetogenesis and baryogenesis in pseudoscalar inflation

Magnetogenesis form axion-U(1) preheating

Magnetogenesis from axion-SU(2) inflation

Magnetogenesis from vorticity in the primordial universe

Modeling the galactic dynamo in the cosmological context

Multi-messenger signatures of cosmological magnetic fields

Multimessenger constraints on intergalactic magnetic fields: quo vadis?

New Models of the Coherent Galactic Magnetic Field

Numerical simulations from reheating to turbulent MHD

Observations of Magnetic Fields in the Large Scale Structure of the Universe (remote)

On adiabatic renormalization and Gauge invariant backreaction in U(1)-axion inflation

Particle production by axion-like particles

Pencil Code office hours (in session "Course "Simulations of Early Universe Magnetohydrodynamics" day 3")

PMFs and their density perturbations through recombination

PMFs from Double Inflation

Practice session 1. Sound waves (in session "Course "Simulations of Early Universe Magnetohydrodynamics" day 1")

Practice session 2a. MHD waves (in session "Course "Simulations of Early Universe Magnetohydrodynamics" day 2")

Practice session 2b. MHD waves (in session "Course "Simulations of Early Universe Magnetohydrodynamics" day 2")

Practice session 3. Driven turbulence (in session "Course "Simulations of Early Universe Magnetohydrodynamics" day 2")

Practice session 4. MHD decaying turbulence (in session "Course "Simulations of Early Universe Magnetohydrodynamics" day 3")

Practice session 5. Chiral dynamo (in session "Course "Simulations of Early Universe Magnetohydrodynamics" day 4")

Practice session 5. Chiral dynamo (in session "Course "Simulations of Early Universe Magnetohydrodynamics" day 4")

Practice session 6. Gravitational waves (in session "Course "Simulations of Early Universe Magnetohydrodynamics" day 4")

Primordial Magnetic Fields from Preheating at the Electroweak Scale

Primordial Magnetic Fields, CMB and the Hubble tension

Primordial magnetogenesis from electroweak dumbbells

Probing high-frequency gravitational waves in cosmic magnetic fields

Probing primordial magnetic fields with 21 cm line observations

Probing the intergalactic magnetic field through gamma-ray observations

Production of chiral anomaly, dynamo instabilities and generation of turbulence

Rethinking Recombination: Primordial Magnetic Fields and the Hubble tension

Role of space plasma instabilities in blazar probes of the intergalactic magnetic field

Scalar perturbations from inflationary magnetogenesis

Scenarios of inflationary magnetogenesis

Searching for Primordial Magnetism in the Cosmic Microwave Background with LiteBIRD (remote)

Simulating the Early Universe

Small scale baryons fluctuations from causal primordial magnetic fields

Statistical Mechanics of the Universe

Sterile Neutrino Dark Matter and Magnetic Fields

Stochastic effects and Primordial magnetogenesis

Structure Formation with Primordial Magnetic Fields: enhancing baryon fraction in halos

Symmetry breaking and magnetic fields

The Non-linear early Universe

Theory lecture 1a. Fluid dynamics (in session "Course "Simulations of Early Universe Magnetohydrodynamics" day 1")

Theory lecture 1b. Fluid dynamics (in session "Course "Simulations of Early Universe Magnetohydrodynamics" day 1")

Theory lecture 2. MHD (in session "Course "Simulations of Early Universe Magnetohydrodynamics" day 2")

Theory lecture 3. Turbulence (in session "Course "Simulations of Early Universe Magnetohydrodynamics" day 2")

Vacuum Energy of the Universe, Large scale magnetic field and nontrivial topology in QCD.

Very large magnetohydrodynamical simulations of structure formation with the cosmological code SWIFT

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