الرئيسية › دليل الباحثين › R. Buompane
R. Buompane
الانتماء : Istituto Nazionale di Fisica Nucleare · University of Campania "Luigi Vanvitelli" · Istituto Nazionale di Fisica Nucleare, Sezione di Napoli
- 44منشورات (انتماء إيطالي)
- 135مجموع المنشورات
- 1822الاستشهادات
- 25مؤشر h
الملف البحثي
لدى R. Buompane 44 منشور(ات) مفهرسة (2016–2026). تُنشر أعماله أساسًا في «Journal of High Energy Physics»، «Journal of Instrumentation» و«The European Physical Journal C». أكثر مقالاته استشهادًا هو «Observation of an ultra-high-energy cosmic neutrino with KM3NeT» (2025)، وقد استُشهد به 146 مرة. 24 من هذه المنشورات تعود إلى آخر ثلاث سنوات من النشاط. شارك في تأليف أعماله 12 باحثًا على الأقل، منهم باحثون من مؤسسات في فرنسا، إسبانيا، هولندا، ألمانيا.
هل هذا أنت؟ عرّف بأبحاثك
أنشئ ملفك على DzCademia مجانًا وأضف مقالاتك: ستظهر بسهولة أكبر على Google وفي مساعدي الذكاء الاصطناعي مثل ChatGPT، فيقرؤها ويستشهد بها عدد أكبر من الناس.
إنشاء ملفي المجاني إضافة منشوراتيمجالات البحث
- Neutrino Physics Research
- Astrophysics and Cosmic Phenomena
- Nuclear physics research studies
- Particle Detector Development and Performance
- Radioactive Decay and Measurement Techniques
المنشورات (44)
- Characterizing Candidate Blazar Counterparts of the Ultra-high-energy Event KM3-230213A
- Blazars as a potential origin of the KM3-230213A event
- On the Potential Galactic Origin of the Ultra-high-energy Event KM3-230213A
- Constraining gamma-ray burst parameters with the first ultra-high energy neutrino event KM3-230213A
- Search for an eV-scale sterile neutrino with the first six detection units of KM3NeT/ORCA
- Optimizing the potential of KM3NeT in detecting core-collapse supernovae
- Observation of an ultra-high-energy cosmic neutrino with KM3NeT
- Ultrahigh-Energy Event KM3-230213A within the Global Neutrino Landscape
- Author Correction: Observation of an ultra-high-energy cosmic neutrino with KM3NeT
- Search for quantum decoherence in neutrino oscillations with six detection units of KM3NeT/ORCA
- KM3NeT constraint on Lorentz-violating superluminal neutrino velocity
- Evaluation of the upgraded 3-inch Hamamatsu photomultiplier for the KM3NeT Neutrino Telescope
- Addendum: Measurement of neutrino oscillation parameters with the first six detection units of KM3NeT/ORCA
- Study of tau neutrinos and non-unitary neutrino mixing with the first six detection units of KM3NeT/ORCA
- Probing invisible neutrino decay with the first six detection units of KM3NeT/ORCA
- Astronomy potential of KM3NeT/ARCA
- Differential Sensitivity of the KM3NeT/ARCA detector to a diffuse neutrino flux and to point-like source emission: Exploring the case of the Starburst Galaxies
- Measurement of neutrino oscillation parameters with the first six detection units of KM3NeT/ORCA
- Atmospheric muons measured with the KM3NeT detectors in comparison with updated numeric predictions
- Search for neutrino emission from GRB 221009A using the KM3NeT ARCA and ORCA detectors
- Searches for neutrino counterparts of gravitational waves from the LIGO/Virgo third observing run with KM3NeT
- Prospects for combined analyses of hadronic emission from $$\gamma $$-ray sources in the Milky Way with CTA and KM3NeT
- The Power Board of the KM3NeT Digital Optical Module: Design, Upgrade, and Production
- Measurement of neutrino oscillation parameters with the first six detection units of KM3NeT/ORCA
- First observation of the cosmic ray shadow of the Moon and the Sun with KM3NeT/ORCA
- KM3NeT broadcast optical data transport system
- Probing invisible neutrino decay with KM3NeT/ORCA
- Determining the neutrino mass ordering and oscillation parameters with KM3NeT/ORCA
- The KM3NeT multi-PMT optical module
- Implementation and first results of the KM3NeT real-time core-collapse supernova neutrino search
- Combined sensitivity of JUNO and KM3NeT/ORCA to the neutrino mass ordering
- The KM3NeT potential for the next core-collapse supernova observation with neutrinos
- Architecture and performance of the KM3NeT front-end firmware
- Sensitivity to light sterile neutrino mixing parameters with KM3NeT/ORCA
- KM3NeT/ARCA expectations in view of a novel multimessenger study of starburst galaxies
- Sensitivity to light sterile neutrino mixing parameters with KM3NeT/ORCA
- gSeaGen: The KM3NeT GENIE-based code for neutrino telescopes
- Dependence of atmospheric muon flux on seawater depth measured with the first KM3NeT detection units
- Event reconstruction for KM3NeT/ORCA using convolutional neural networks
- Deep-sea deployment of the KM3NeT neutrino telescope detection units by self-unrolling
- Sensitivity of the KM3NeT/ARCA neutrino telescope to point-like neutrino sources
- Characterisation of the Hamamatsu photomultipliers for the KM3NeT Neutrino Telescope
- Intrinsic limits on resolutions in muon- and electron-neutrino charged-current events in the KM3NeT/ORCA detector
- A method to stabilise the performance of negatively fed KM3NeT photomultipliers
مجلات النشر
- Journal of High Energy Physics × 9
- Journal of Instrumentation × 8
- The European Physical Journal C × 8
- Journal of Cosmology and Astroparticle Physics × 5
- Nature × 2
- Astroparticle Physics × 2
المنشورات حسب السنة
- 20266
- 20259
- 20249
- 20233
- 20224
- 20215
- 20204
- 20191
- 20181
- 20171
التعاون العلمي
المؤسسات الشريكة : Istituto Nazionale di Fisica Nucleare, Laboratori Nazionali del Sud · Istituto Nazionale di Fisica Nucleare, Sezione di Roma I · Istituto Nazionale di Fisica Nucleare, Sezione di Bologna · Sapienza University of Rome · Centre National de la Recherche Scientifique
بلدان المؤلفين المشاركين : فرنسا · إسبانيا · هولندا · ألمانيا
المؤلفون المشاركون
- S. Biagi
- T. Chiarusi
- A. Capone
- G. Cuttone
- R. Coniglione
- Carla Distefano
- M. Circella
- B. Caiffi
- I. Di Palma
- Paolo Castaldi
- F. Benfenati
- Riccardo Bruno
البيانات البيبليوغرافية مصدرها OpenAlex (قاعدة مفتوحة).
لماذا تختارون Dzcademia؟
ملفات أكاديمية ومقالات ومداخلات علمية: امنحوا أبحاثكم حضوراً عاماً منظماً. تساعد البيانات الوصفية المدمجة محركات البحث ومساعدات الذكاء الاصطناعي على التعرف على أعمالكم وفهم مراجعها.
علّق عبر Google
سجّل الدخول عبر Google للتعليق مباشرة على هذه الصفحة.