activity
20242026
collaborators

12 papers

astro-ph.HE2026

Evidence of cosmic-ray acceleration up to sub-PeV energies in the supernova remnant IC 443

Zhen Cao, F. Aharonian, Y. X. Bai +309

Supernova remnants (SNRs) have been considered as the primary contributors to cosmic rays (CRs) in our Galaxy. However, the maximum energy of particles that can be accelerated by s…

hep-ex2025

Search for

BESIII Collaboration, M. Ablikim, M. N. Achasov +650

Using collision data at 13 center-of-mass energies ranging from 4.600 to 4.950 GeV collected with the BESIII detector, we search for the unmeasured $e^+e^-\to K_S^0 K_S^0…

hep-ex2025

Measurement of the branching fraction of the decay

BESIII Collaboration, M. Ablikim, M. N. Achasov +645

A high precision measurement of the branching fraction of the decay is performed using events recorded by the {BESIII} d…

hep-ex2025

Observation and branching fraction measurement of the decay

M. Ablikim, M. N. Achasov, P. Adlarson +612

The first observation of the decays and is reported using $J\…

hep-ex2025

Observation of and First Study of Decay Dynamics

BESIII Collaboration, M. Ablikim, M. N. Achasov +648

Using of collision data collected at the center-of-mass energy 3.773\,GeV with the BESIII detector, we report the first observation of the semileptonic…

hep-ex2025

Measurement of Born cross section of at GeV

BESIII Collaboration, M. Ablikim, M. N. Achasov +654

Using collision data collected with the BESIII detector at the BEPCII collider at thirty-two center-of-mass energies from 3.50 to 4.95 GeV, corresponding to an integrated…