Publications (93)
Final assessment of radioactive impurities in the JUNO detector
Thomas Adam, Fengpeng An, Costas Andreopoulos +569
The Jiangmen Underground Neutrino Observatory (JUNO) collaboration has completed the construction of the 20,000-ton liquid scintillator detector and the associated muon veto detect…
The 17 MeV Anomaly in Beryllium Decays and Portal to Dark Matter
Chian-Shu Chen, Guey-Lin Lin, Yen-Hsun Lin +1
The experiment of Krasznahorkay \textit{et al} observed the transition of a excited state to its ground state and accompanied by an emission of pair with…
Sensitivities of IceCube DeepCore Detector to Signatures of Low-Mass Dark Matter in the Galactic Halo
Fei-Fan Lee, Guey-Lin Lin, Yue-Lin Sming Tsai
We discuss the event rate in DeepCore array due to neutrino flux produced by annihilations and decays of galactic dark matter. This event rate is calculated with a 10 GeV threshold…
Real-time Monitoring for the Next Core-Collapse Supernova in JUNO
Angel Abusleme, Thomas Adam, Shakeel Ahmad +623
The core-collapse supernova (CCSN) is considered one of the most energetic astrophysical events in the universe. The early and prompt detection of neutrinos before (pre-SN) and dur…
Heavy Quark Effective Theory on the Light Front
Wei-Min Zhang, Guey-Lin Lin, Chi-Yee Cheung
The light-front heavy quark effective theory is derived to all orders in . In the limit , the theory exhibits the familiar heavy quark spin-flavor sym…
Another Look at Charged Higgs Boson Production at LEP
Shinya Kanemura, Takashi Kasai, Guey-Lin Lin +3
The current atmospheric and solar neutrino experimental data favors the bi-maximal mixing solution of the Zee-type neutrino mass matrix in which neutrino masses are generated radia…
Embedded underwater front-end electronics for the 3-inch photomultipliers in the JUNO experiment
Cédric Cerna, Miao He, Xiaoshan Jiang +591
The Jiangmen Underground Neutrino Observatory (JUNO) is a 20-kton liquid scintillator-based, low-radioactivity, multi-purpose neutrino detector located 693 meters (1800 m.w.e.) und…
A semi-analytic calculation on the atmospheric tau neutrino flux in the GeV to TeV energy range
Fei-Fan Lee, Guey-Lin Lin
We present a semi-analytic calculation on the atmospheric tau neutrino flux in the GeV to TeV energy range. The atmospheric flux is calculated for the entire zenith angle r…
The technique of inverse Mellin transform for processes occurring in a background magnetic field
Guey-Lin Lin
We develop the technique of inverse Mellin transform for processes occurring in a background magnetic field. We show by analyticity that the energy (momentum) derivatives of a fiel…
The JUNO experiment Top Tracker
JUNO Collaboration, Angel Abusleme, Thomas Adam +609
The main task of the Top Tracker detector of the neutrino reactor experiment Jiangmen Underground Neutrino Observatory (JUNO) is to reconstruct and extrapolate atmospheric muon tra…
Polarization effects in the search for dark vector boson at colliders
Fei-Fan Lee, Guey-Lin Lin, Vo Quang Nhat
We argue that the search for dark vector boson through can determine the Lorentz structure of couplings with the detection of leptonic decays $Z_d\to…
The weak-field expansion for processes in a homogeneous background magnetic field
Tzuu-Kang Chyi, Chien-Wen Hwang, W. F. Kao +3
The weak-field expansion of the charged fermion propagator under a uniform magnetic field is studied. Starting from Schwinger's proper-time representation, we express the charged f…
Probing annihilations and decays of low-mass galactic dark matter in IceCube DeepCore array: Track events
Fei-Fan Lee, Guey-Lin Lin
The deployment of DeepCore array significantly lowers IceCube's energy threshold to about 10 GeV and enhances the sensitivity of detecting neutrinos from annihilations and decays o…
Probing Dark Matter Self-Interaction in the Sun with IceCube-PINGU
Chian-Shu Chen, Fei-Fan Lee, Guey-Lin Lin +1
We study the capture, annihilation and evaporation of dark matter (DM) inside the Sun. It has been shown that the DM self-interaction can increase the DM number inside the Sun. We…
Exploring dark sector parameters in light of neutron star temperatures
Guey-Lin Lin, Yen-Hsun Lin
Using neutron stars (NS) as a dark matter (DM) probe has gained broad attention recently, either from heating due to DM annihilation or its stability under the presence of DM. In t…
Neutrino Flavor Ratio on Earth and at Astrophysical Sources
Kwang-Chang Lai, Guey-Lin Lin, T. C. Liu
We present the reconstruction of neutrino flavor ratios at astrophysical sources. For distinguishing the pion source and the muon-damped source to the 3 level, the neutrino flu…
JUNO Sensitivity to Invisible Decay Modes of Neutrons
JUNO Collaboration, Angel Abusleme, Thomas Adam +651
We explore the decay of bound neutrons into invisible particles (e.g., or ) in the JUNO liquid scintillator detector, which do not produce…
Probing the coupling of heavy dark matter to nucleons by detecting neutrino signature from the Earth core
Guey-Lin Lin, Yen-Hsun Lin
We argue that the detection of neutrino signature from the Earth core is an ideal approach for probing the coupling of heavy dark matter ( GeV) to nucleons. We first n…
Like Sign Top Pair Production at LHC
Guey-Lin Lin
Having a mass comparable to the weak scale, the top quark may have a sizable flavor changing couplings to Higgs bosons. We show that such couplings can be probed at the LHC through…
Thermal transport of the solar captured dark matter and its impact on the indirect dark matter search
Chian-Shu Chen, Guey-Lin Lin, Yen-Hsun Lin
We study the thermal transport occurring in the system of solar captured dark matter (DM) and explore its impact on the DM indirect search signal. We particularly focus on the scen…
The dark matter self-interaction and its impact on the critical mass for dark matter evaporations inside the sun
Chian-Shu Chen, Fei-Fan Lee, Guey-Lin Lin +1
We study the capture, annihilation and evaporation of dark matter (DM) inside the Sun. It has been shown that the DM self-interaction can increase the DM number inside the Sun. We…
Determination of the Source Flavor Ratio of Ultrahigh Energy Neutrinos
T. C. Liu, M. A. Huang, Guey-Lin Lin
We discuss the reconstruction of neutrino flavor neutrino at a distant source in the very high en- ergy regime. This reconstruction procedure is relevant to the confirmation of det…
High energy tau neutrinos: production, propagation and prospects of observations
H. Athar, Jie-Jun Tseng, Guey-Lin Lin
High energy tau neutrinos with energy greater than several thousands of GeV may be produced in some astrophysical sites. A summary of the intrinsic high energy tau neutrino flux es…
Complementary Test of the Dark Matter Self-Interaction by Direct and Indirect Detections
Chian-Shu Chen, Guey-Lin Lin, Yen-Hsun Lin
The halo dark matter (DM) can be gravitationally captured by the Sun. For self-interacting DM (SIDM), we show that the number of DM trapped inside the Sun remains unsuppressed even…
Determination of the total absorption peak in an electromagnetic calorimeter
Jia-Hua Cheng, Zhe Wang, Logan Lebanowski +2
A physically-motivated function was developed to accurately determine the total absorption peak in an electromagnetic calorimeter and to overcome biases present in many commonly us…
Comparison of high-energy galactic and atmospheric tau neutrino flux
H. Athar, Kingman Cheung, Guey-Lin Lin +1
We compare the tau neutrino flux arising from the galaxy and the earth atmosphere for 10^3 < E/GeV < 10^11. The intrinsic and oscillated tau neutrino fluxes from both sources are c…
Flavor Transition Mechanisms of Propagating Astrophysical Neutrinos -A Model Independent Parametrization
Kwang-Chang Lai, Guey-Lin Lin, T. C. Liu
One of the important goals for future neutrino telescopes is to identify the flavors of astrophysical neutrinos and therefore determine the flavor ratio. The flavor ratio of astrop…
The Dispersive Approach to Electroweak Processes in the Background Magnetic Field
Guey-Lin Lin
We propose a new method to compute amplitudes of electroweak processes in the strong background magnetic field, using as an example. We show that the {\it moments} o…
Strong-Field QED and the Inverse Mellin Transform
Guey-Lin Lin
We introduce the technique of inverse Mellin transform in a problem of strong-field QED. We show that the {\it moments} of pair production width in a uniform background magnetic fi…
Feasibility and physics potential of detecting B solar neutrinos at JUNO
JUNO collaboration, Angel Abusleme, Thomas Adam +589
The Jiangmen Underground Neutrino Observatory~(JUNO) features a 20~kt multi-purpose underground liquid scintillator sphere as its main detector. Some of JUNO's features make it an…
The matter effects to neutrino oscillations ν_μ\to ν_e, ν_μat very long baselines and the neutrino mixing angles θ_13 and θ_23
Guey-Lin Lin, Yoshiaki Umeda
We study the matter effects to neutrino oscillations ν_μ\to ν_e and ν_μ\to ν_μat very long baselines. It has been observed that, for a very long baseline L~10000 km, the res…
Like Sign Top Quark Pair Production at Linear Colliders
Wei-Shu Hou, Guey-Lin Lin
In the general two Higgs doublet model with flavor changing neutral Higgs couplings, neutral Higgs bosons may decay dominantly via or final states. At the linea…
Prospects for geoneutrino detection with JUNO
Thomas Adam, Shakeel Ahmad, Rizwan Ahmed +625
Geoneutrinos, which are antineutrinos emitted during the decay of long-lived radioactive elements inside Earth, serve as a unique tool for studying the composition and heat budget…
Letter of Intent: Jinping Neutrino Experiment
John F. Beacom, Shaomin Chen, Jianping Cheng +34
Jinping Neutrino Experiment (Jinping) is proposed to significantly improve measurements on solar neutrinos and geoneutrinos in China Jinping Laboratory - a lab with a number of unp…
Probing Neutrino Mass Hierarchy by Comparing the Charged-Current and Neutral-Current Interaction Rates of Supernova Neutrinos
Kwang-Chang Lai, Fei-Fan Lee, Feng-Shiuh Lee +3
The neutrino mass hierarchy is one of the neutrino fundamental properties yet to be determined. We introduce a method to determine neutrino mass hierarchy by comparing the interact…
Neutrino-photon scattering and its crossed processes in a background magnetic field
Tzuu-Kang Chyi, Chien-Wen Hwang, W. F. Kao +3
We study the neutrino-photon processes such as and in a background magnetic field smaller than the critical magnetic field . Us…
On the Prospects of Tau Neutrino Astronomy in Gev Energies and Beyond
H. Athar, Fei-Fan Lee, Guey-Lin Lin
We point out the opportunity of tau neutrino astronomy for neutrino energies of the order of 10 GeV to 10 GeV. In this energy range, it is demonstrated that the flavor depend…
SN1987A constraints to BSM models with extra neutral bosons near the trapping regime: model as an illustrative example
Kwang-Chang Lai, Chun Sing Jason Leung, Guey-Lin Lin
New physics beyond the Standard Model (BSM) with an extra neutral boson can be constrained from the observation of SN1987A, since the production of this neutral boson in a supernov…
Probing Flavor Changing Neutral Higgs Couplings at LHC
Wei-Shu Hou, Guey-Lin Lin, Chien-Yi Ma +1
Uniquely heavy with mass at the weak scale, the top quark may have large flavor changing couplings to Higgs bosons that are as yet unexplored. We show that such couplings can be di…
A New Type of Plasma Wakefield Accelerator Driven by Magnetowaves
Pisin Chen, Feng-Yin Chang, Guey-Lin Lin +2
We present a new concept for a plasma wakefield accelerator driven by magnetowaves (MPWA). This concept was originally proposed as a viable mechanism for the "cosmic accelerator" t…
Testing the hypothesis of vector X17 boson by D meson, Charmonium, and meson decays
Fei-Fan Lee, Lam Thi Thuc Uyen, Guey-Lin Lin
The recent ATOMKI experiments provided evidence pointing towards the existence of an X17 boson in the anomalous nuclear transitions of Beryllium-8, Helium-4, and Carbon-12. In this…
Determination of the Neutrino Flavor Ratio at the Astrophysical Source
Kwang-Chang Lai, Guey-Lin Lin, T. C. Liu
We discuss the reconstruction of neutrino flavor ratios at astrophysical sources through the future neutrino-telescope measurements. Taking the ranges of neutrino mixing parameters…
Model Independent Approach of the JUNO B Solar Neutrino Program
JUNO Collaboration, Jie Zhao, Baobiao Yue +593
The physics potential of detecting B solar neutrinos will be exploited at the Jiangmen Underground Neutrino Observatory (JUNO), in a model independent manner by using three dis…
Neutrino Physics with JUNO
Fengpeng An, Guangpeng An, Qi An +224
The Jiangmen Underground Neutrino Observatory (JUNO), a 20 kton multi-purpose underground liquid scintillator detector, was proposed with the determination of the neutrino mass hie…
Sub-percent Precision Measurement of Neutrino Oscillation Parameters with JUNO
JUNO Collaboration, Angel Abusleme, Thomas Adam +596
JUNO is a multi-purpose neutrino observatory under construction in the south of China. This publication presents new sensitivity estimates for the measurement of the ,…
Heavy-Flavor-Conserving Hadronic Weak Decays of Heavy Baryons
Hai-Yang Cheng, Chi-Yee Cheung, Guey-Lin Lin +3
More than two decades ago, we studied heavy-flavor-conserving weak decays of heavy baryons within the framework that incorporates both heavy-quark and chiral symmetries. In view of…
GeoSynchrotron Radiation from Earth Skimming Tau Neutrino Shower
Kwang-Chang Lai, Guey-Lin Lin, Tsung-Che Liu +2
Cosmogenic neutrinos are expected from ultrahigh energy cosmic rays undergoing the GZK process and anticipated to be observed by detecting air showers from the decays of tau lepton…
Phenomenology of Higgs bosons in the Zee-Model
Shinya Kanemura, Takashi Kasai, Guey-Lin Lin +3
To generate small neutrino masses radiatively, the Zee-model introduces two Higgs doublets and one weak-singlet charged Higgs boson to its Higgs sector. From analyzing the renormal…
Initial performance results of the JUNO detector
Angel Abusleme, Thomas Adam, Kai Adamowicz +1131
The Jiangmen Underground Neutrino Observatory (JUNO) started physics data taking on 26 August 2025. JUNO consists of a 20-kton liquid scintillator central detector, surrounded by a…
Mass Testing and Characterization of 20-inch PMTs for JUNO
Angel Abusleme, Thomas Adam, Shakeel Ahmad +556
Main goal of the JUNO experiment is to determine the neutrino mass ordering using a 20kt liquid-scintillator detector. Its key feature is an excellent energy resolution of at least…
Signatures of afterglows from light dark matter boosted by supernova neutrinos in current and future large underground detectors
Yen-Hsun Lin, Tsung-Han Tsai, Guey-Lin Lin +2
Supernova neutrino boosted dark matter (SN BDM) and its afterglow effect have been shown to be a promising signature for beyond Standard Model (bSM) physics. The time-evolution…
Potential to identify neutrino mass ordering with reactor antineutrinos at JUNO
JUNO Collaboration, Angel Abusleme, Thomas Adam +622
The Jiangmen Underground Neutrino Observatory (JUNO) is a multi-purpose neutrino experiment under construction in South China. This paper presents an updated estimate of JUNO's sen…
JUNO sensitivity to the annihilation of MeV dark matter in the galactic halo
JUNO Collaboration, Angel Abusleme, Thomas Adam +596
We discuss JUNO sensitivity to the annihilation of MeV dark matter in the galactic halo via detecting inverse beta decay reactions of electron anti-neutrinos resulting from the ann…
Constraining dark matter capture and annihilation cross sections by searching for neutrino signature from the Earth core
Fei-Fan Lee, Guey-Lin Lin, Yue-Lin Sming Tsai
We study the sensitivity of IceCube/DeepCore detector to dark matter annihilations in the Earth core. We focus on annihilation modes ,…
GZK Horizons and the Recent Pierre Auger Result on the Anisotropy of Highest-energy Cosmic Ray Sources
Chia-Chun Lu, Guey-Lin Lin
Motivated by recent Pierre Auger result on the correlation of the highest-energy cosmic rays with the nearby active galactic nuclei, we explore possible ultrahigh energy cosmic ray…
Calibration Strategy of the JUNO Experiment
JUNO collaboration, Angel Abusleme, Thomas Adam +588
We present the calibration strategy for the 20 kton liquid scintillator central detector of the Jiangmen Underground Neutrino Observatory (JUNO). By utilizing a comprehensive multi…
Design, waterproofing, and mass production of the 3-inch PMT frontend system of JUNO
Jilei Xu, Miao He, Cédric Cerna +628
Over 25,600 3-inch photomultiplier tubes (PMTs) have been instrumented for the central detector of the Jiangmen Underground Neutrino Observatory. Each PMT is equipped with a high-v…
The Design and Sensitivity of JUNO's scintillator radiopurity pre-detector OSIRIS
JUNO Collaboration, Angel Abusleme, Thomas Adam +598
The OSIRIS detector is a subsystem of the liquid scintillator fillling chain of the JUNO reactor neutrino experiment. Its purpose is to validate the radiopurity of the scintillator…
The inclusive B->eta' X_s decay and b-> sg* form factors
Guey-Lin Lin
We compute the branching ratio of inclusive decay based upon the QCD anomaly mechanism: . To obtain a reliable branching rati…
TAO Conceptual Design Report: A Precision Measurement of the Reactor Antineutrino Spectrum with Sub-percent Energy Resolution
JUNO Collaboration, Angel Abusleme, Thomas Adam +585
The Taishan Antineutrino Observatory (TAO, also known as JUNO-TAO) is a satellite experiment of the Jiangmen Underground Neutrino Observatory (JUNO). A ton-level liquid scintillato…
JUNO sensitivity to Be, , and CNO solar neutrinos
Angel Abusleme, Thomas Adam, Shakeel Ahmad +609
The Jiangmen Underground Neutrino Observatory (JUNO), the first multi-kton liquid scintillator detector, which is under construction in China, will have a unique potential to perfo…
Effective Lagrangian Approach to Weak Radiative Decays of Heavy Hadrons
Hai-Yang Cheng, Chi-Yee Cheung, Guey-Lin Lin +3
Motivated by the observation of the decay by CLEO, we have systematically analyzed the two-body weak radiative decays of bottom and charmed hadrons. There…
Taking Neutrino Pictures via Electrons
Guey-Lin Lin, Thi Thuy Linh Nguyen, Martin Spinrath +2
In this paper we discuss the prospects to take a picture of an extended neutrino source, i.e., resolving its angular neutrino luminosity distribution. This is challenging since neu…
JUNO Sensitivity on Proton Decay Searches
JUNO Collaboration, Angel Abusleme, Thomas Adam +602
The Jiangmen Underground Neutrino Observatory (JUNO) is a large liquid scintillator detector designed to explore many topics in fundamental physics. In this paper, the potential on…
JUNO Physics and Detector
JUNO Collaboration, Angel Abusleme, Thomas Adam +607
The Jiangmen Underground Neutrino Observatory (JUNO) is a 20 kton LS detector at 700-m underground. An excellent energy resolution and a large fiducial volume offer exciting opport…
Radioactivity control strategy for the JUNO detector
JUNO collaboration, Angel Abusleme, Thomas Adam +594
JUNO is a massive liquid scintillator detector with a primary scientific goal of determining the neutrino mass ordering by studying the oscillated anti-neutrino flux coming from tw…
Corrections to Chiral Dynamics of Heavy Hadrons: SU(3) Symmetry Breaking, (with some minor corrections)
Hai-Yang Cheng, Chi-Yee Cheung, Guey-Lin Lin +3
In previous publications we have analyzed the strong and electromagnetic decays of heavy mesons and heavy baryons in a formalism which incorporates heavy-quark and chiral symmetrie…
First measurement of reactor neutrino oscillations at JUNO
Angel Abusleme, Thomas Adam, Kai Adamowicz +1131
Neutrino oscillations, a quantum effect manifesting at macroscopic scales, are governed by lepton flavor mixing angles and neutrino mass-squared differences that are fundamental pa…
On non hadronic origin of high energy neutrinos
H. Athar, Guey-Lin Lin
Some of the non hadronic interactions, such as the ηresonance formation in the γγinteractions and the muon pair production in the eγinteractions, are identified as possible sou…
Analysis on the black hole formations inside old neutron stars by isospin-violating dark matter with self-interaction
Guey-Lin Lin, Yen-Hsun Lin
Fermionic dark matter (DM) with attractive self-interaction is possible to form black holes (BH) inside the Gyr-old neutron stars (NS). Therefore by observing such NS corresponding…
in the Standard Model
Xiao-Gang He, Guey-Lin Lin
We study within the framework of the Standard Model. Several mechanisms such as from the QCD anomaly, and and from…
Ultra High Energy Cosmic Ray Puzzle and the Plasma Wakefield Acceleration
Feng-Yin Chang, Pisin Chen, Guey-Lin Lin +3
Magnetowave induced plasma wakefield acceleration (MPWA) in a relativistic astrophysical outflow has been proposed as a viable mechanism for the acceleration of cosmic particles to…
Constraining the Mass Scale of a Lorentz-Violating Hamiltonian with the Measurement of Astrophysical Neutrino-Flavor Composition
Kwang-Chang Lai, Wei-Hao Lai, Guey-Lin Lin
We study Lorentz violation effects on flavor transitions of high energy astrophysical neutrinos. It is shown that the appearance of Lorentz violating Hamiltonian can drastically ch…
Damping signatures at JUNO, a medium-baseline reactor neutrino oscillation experiment
JUNO collaboration, Jun Wang, Jiajun Liao +598
We study damping signatures at the Jiangmen Underground Neutrino Observatory (JUNO), a medium-baseline reactor neutrino oscillation experiment. These damping signatures are motivat…
Gauge Independent Effective Potential and the Higgs Mass Bound
Guey-Lin Lin, Tzu-Kang Chyi
We introduce the Vilkovisky-DeWitt formalism for deriving the lower bound of the Higgs boson mass. We illustrate the formalism with a simplified version of the Standard Electroweak…
Implications of for high-energy observation
H. Athar, Guey-Lin Lin
Absorption of high-energy over electrons above the W boson production threshold is reexamined. It is pointed out that, in the case of photon emissions along the directio…
JUNO sensitivity to low energy atmospheric neutrino spectra
JUNO Collaboration, Angel Abusleme, Thomas Adam +604
Atmospheric neutrinos are one of the most relevant natural neutrino sources that can be exploited to infer properties about cosmic rays and neutrino oscillations. The Jiangmen Unde…
Probing Neutrino Flavor Transition Mechanism with Ultra High Energy Astrophysical Neutrinos
Kwang-Chang Lai, Guey-Lin Lin, Tsung-Che Liu
Observation of ultra-high energy astrophysical neutrinos and identification of their flavors have been proposed for future neutrino telescopes. The flavor ratio of astrophysical ne…
Subleading Corrections to Semileptonic Lambda_c Decays
Guey-Lin Lin, Thomas Mannel
The semileptonic decay is considered in the framework of heavy quark effective theory beyond the leading order in the expansion. According to our estim…
Perturbative QCD study of the B-> K^* gamma decay
Hsiang-nan Li, Guey-Lin Lin
We apply the perturbative QCD factorization theorem developed recently for nonleptonic heavy meson decays to the radiative decay . In this formalism the evolution of th…
Probing the coupling of heavy dark matter to nucleons by detecting neutrino signature from the Earth's core
Guey-Lin Lin, Yen-Hsun Lin, Fei-Fan Lee
We argue that the detection of neutrino signature from the Earth's core can effectively probe the coupling of heavy dark matter ( GeV) to nucleons. We first note that…
GZK Horizons and the Anisotropy of Highest-energy Cosmic Ray Sources
Chia-Chun Lu, Guey-Lin Lin
Motivated by recent Pierre Auger result on the correlation of the highest-energy cosmic rays with the nearby active galactic nuclei, we explore possible ultrahigh energy cosmic ray…
QCD Corrections to and Exclusive Decay
Chia-Hung V. Chang, Guey-Lin Lin, York-Peng Yao
The short distance QCD corrections to are calculated in the leading logarithmic approximation. The equivalence of operator basis reduction for S-matrix elements by usi…
Simulation of the Background from CO Reaction in the JUNO Scintillator
JUNO Collaboration, Thomas Adam, Kai Adamowicz +627
Large-scale organic liquid scintillator detectors are highly efficient in the detection of MeV-scale electron antineutrinos. These signal events can be detected through inverse bet…
Probing the octant of with very long baseline neutrino oscillation experiments: a global look
Guey-Lin Lin, Yoshiaki Umeda
We investigate the baseline range in which the degeneracy in neutrino oscillation probabilities is absent for fixed values of and CP violation phase $δ_{\rm CP…
Prediction of Energy Resolution in the JUNO Experiment
JUNO Collaboration, Angel Abusleme, Thomas Adam +645
This paper presents an energy resolution study of the JUNO experiment, incorporating the latest knowledge acquired during the detector construction phase. The determination of neut…
A Low-energy Threshold and Multi-messenger Trigger System for the JUNO Experiment
Thomas Adam, Fengpeng An, Costas Andreopoulos +563
The paper presents a new multi‑messenger trigger system for the JUNO liquid‑scintillator detector that lowers the energy threshold to about 110 keV and adds real‑time monitoring of…
Testing MSW effect in supernova explosion with neutrino event rates
Kwang-Chang Lai, C. S. Jason Leung, Guey-Lin Lin
Flavor transition mechanisms of supernova (SN) neutrinos during their propagation deserve a close scrutiny. We present a method to verify Mikheyev-Smirnov-Wolfenstein (MSW) effect…
A new look at the pair-production width in a strong magnetic field
W. F. Kao, Guey-Lin Lin, Jie-Jun Tseng
We reexamine the process in a background magnetic field comparable to . This process is known to be non-perturbative in the magnetic-field stren…
Magnetowave Induced Plasma Wakefield Acceleration for Ultra High Energy Cosmic Rays
Feng-Yin Chang, Pisin Chen, Guey-Lin Lin +2
Magnetowave induced plasma wakefield acceleration (MPWA) in a relativistic astrophysical outflow has been proposed as a viable mechanism for the acceleration of cosmic particles to…
Prospects for Detecting the Diffuse Supernova Neutrino Background with JUNO
JUNO Collaboration, Angel Abusleme, Thomas Adam +592
We present the detection potential for the diffuse supernova neutrino background (DSNB) at the Jiangmen Underground Neutrino Observatory (JUNO), using the inverse-beta-decay (IBD)…
Vilkovisky-DeWitt Effective Potential and the Higgs-Mass Bound
Guey-Lin Lin, Tzuu-Kang Chyi
We compute the Vilkovisky-DeWitt effective potential of a simplified version of the Standard Electroweak Model, where all charged boson fields as well as the bottom-quark field are…
B--> eta' X_s in the Standard Model
Xiao-Gang He, Guey-Lin Lin
We study within the framework of the Standard Model. Several mechanisms such as through the QCD anomaly, and and a…