TeV Particle Astrophysics 2026

Asia/Tokyo
Description

TeV Particle Astrophysics (TeVPA) is a leading international conference focused on recent developments in astroparticle physics. The 2026 edition will be held in Tendo, Japan, bringing together researchers to present and discuss the latest findings.

๐Ÿ•’ Schedule

  • August 30, 2026 (Afternoon):
    Pre-conference Workshop: MMA-CADO
  • August 31 โ€“ September 4, 2026:
    Main Conference (TeVPA 2026)

Pre-conference Workshop

A dedicated workshop, "Multi-messenger Astrophysics through Collaboration Among Different Observatories (MMA-CADO)", will be held prior to the main program. All TeVPA participants are welcome to attend with no additional fee.

This session highlights international collaboration and recent developments in multi-messenger fields, offering excellent networking opportunities.

Explore Workshop Scope & Details โ†’

Scientific Program

Plenary and parallel sessions will cover the following topics:

โ€ข Cosmic ray physics
โ€ข Gamma-ray & Neutrino astronomy
โ€ข Cosmology
โ€ข Dark matter searches (both direct and indirect)
โ€ข Gravitational waves
โ€ข Particle physics connections

List of Plenary Speakers

Name Affiliation Topic
Sylvia Biscoveanu Princeton University gravitational-wave astronomy
Teresa Bister Radboud University Nijmegen probe UHECR origin with B-field configuration
Antonella Castellina INFN, Torino Measurements of UHECRs and their multimessenger aspects
Shion Chen Kyoto University Quantum Sensor Development and Wave-like Dark Matter Detection
Motoko Fujiwara University of Toyama The standard WIMP and that go beyond the standard WIMP paradigm
Diego Gotz CEA Paris-Saclay SVOM mission, GRB and rapid follow-up of gravitational wave and neutrino
Gonzalo Herrera Harvard University & MIT Cosmic-ray+neutrino+Dark Matter (multimessenger modeling, observation)
Alexander Kusenko UCLA Primordial black holes
Bing Liu Purple Mountain Observatory, CAS LHASSO result oriented Galactic gamma-ray emission
Ruoyu Liu Nanjing University Galactic Sources of High-Energy Messengers (modeling)
Yuan Liu National Astronomical Observatories, CAS Multimessenger transient with X-ray
Lu Lu University of Wisconsin-Madison An overview of the field of neutrino astrophysics and its role in multi-messenger astrophysics
Maria Petropoulou National & Kapodistrian University of Athens Theoretical modeling of high-energy sources, blazar/GRB emission, AGN jets
Elena Pinetti Flatiron Institute Phenomenological interpretation of DM (IceCube, JWST, Fermi)
Tina Pollman University of Amsterdam (GRAPPA) Direct DM detection
Katherine Rawlins University of Alaska Anchorage Galactic CR - measurements and interpretation around knee
Fuminobu Takahashi Tohoku University Axion cosmology, inflation
Tomislav Terzic University of Rijeka VHE Gamma-ray astrophysics
John Tomsick UC Berkeley Mission oriented future overview of MeV astronomy
Naomi Tsuji ICRR, The University of Tokyo Multiwavelength campaigns targeting Galactic PeVatron candidates
Tejaswi Venumadhav UC Santa Barbara Gravitational wave independent of LIGO
Angela Zegarelli Ruhr-University Bochum multimessenger phenomenology for SNe
ICEHAP Multimessenger KAKENHI