Symmetry and Neutrinos Astronomy
A special issue of Symmetry (ISSN 2073-8994). This special issue belongs to the section "Physics".
Deadline for manuscript submissions: 30 April 2026 | Viewed by 14
Special Issue Editors
Interests: neutrino oscillations; neutrino astronomy; cosmic rays; air showers; beyond standard model
Special Issue Information
Dear Colleagues,
Neutrino astronomy stands at the frontier of modern astroparticle physics, offering a unique and powerful probe into both the largest and most energetic phenomena in the universe and the earliest cosmic epochs. Spanning an enormous energy range—from the elusive cosmic neutrino background (relic neutrinos), through MeV-scale supernova neutrinos, to PeV–EeV neutrinos associated with ultra-high-energy cosmic rays (UHECRs)—neutrinos serve as pristine messengers across time and space. Their weak interactions and ability to travel unimpeded from distant and dense regions grant access to astrophysical processes otherwise hidden from electromagnetic observation.
This Special Issue explores the full landscape of neutrino astronomy and emphasizes the underlying symmetry relations that link neutrinos to other cosmic messengers. From the energy transfer symmetry between cosmic rays and neutrinos in hadronic interactions, through deeper theoretical symmetries embedded in particle interactions and cosmic evolution, to the symmetry of the neutrino flavor composition in the propagation, these connections guide us toward unified interpretations of astrophysical data.
We invite contributions addressing all aspects of neutrino astrophysics—from theoretical developments and detector technologies to data-driven studies and multi-messenger synergies. We particularly welcome work that reflects on how symmetry principles can enhance our understanding across different energy regimes and cosmic epochs.
Dr. Baobiao Yue
Dr. Alexander Sandrock
Guest Editors
Manuscript Submission Information
Manuscripts should be submitted online at www.mdpi.com by registering and logging in to this website. Once you are registered, click here to go to the submission form. Manuscripts can be submitted until the deadline. All submissions that pass pre-check are peer-reviewed. Accepted papers will be published continuously in the journal (as soon as accepted) and will be listed together on the special issue website. Research articles, review articles as well as short communications are invited. For planned papers, a title and short abstract (about 100 words) can be sent to the Editorial Office for announcement on this website.
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Please visit the Instructions for Authors page before submitting a manuscript. The Article Processing Charge (APC) for publication in this open access journal is 2400 CHF (Swiss Francs). Submitted papers should be well formatted and use good English. Authors may use MDPI's English editing service prior to publication or during author revisions.
Keywords
- neutrino astronomy
- ultra-high-energy cosmic rays (UHECRs)
- cosmic neutrino background
- supernova neutrinos
- multi-messenger astrophysics
- neutrino flavor composition
- hadronic interactions
- high-energy neutrino detection
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