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06/08/2021 Gmail - NSPDI17: contributory talk
Moon Moon Devi
NSPDI17: contributory talk
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https://mail.google.com/mail/u/0?ik=2af6c32334&view=pt&search=all&permmsgid=msg-f%3A1578609287920334673&simpl… 1/1 June 7, 2018 8:55 WSPC/CRC 9.75 x 6.5 1860100
XXXI International Workshop on High Energy Physics: Critical Points in the Modern Particle Physics International Journal of Modern Physics: Conference Series Vol. 47 (2018) 1860100 (5 pages) c The Author(s) DOI: 10.1142/S201019451860100X
The Effects of Majorana Phases in Estimating the Masses of Neutrinos
Ng. K. Francis∗ and Ankur Nath Department of Physics, Tezpur University, Sonitpur, Assam 784028, India ∗[email protected] www.tezu.ernet.in
Published 6 June 2018
Majorana CP violating phases coming from heavy right-handed Majorana mass matrices(MRR) are considered to estimate the masses of neutrinos. The effects of phases on quasi-degenerate neutrinos mass matrix obeying µ − τ symmetry predicts the results consistent with observations for (i) solar mixing angle(θ12) below TBM, (ii) absolute neutrino mass parameters[mee] in neutrinoless double beta(0νββ) decay, and (iii) cos- P mological upper bound i mi. Analysis is carried out through parameterization of light left-handed Majorana neutrino matrices (mLL) using only two unknown parameters (, η) within µ − τ symmetry. We consider the charge lepton and up quark matrices as diagonal form of Dirac neutrino mass matrix (mLR), and mRR are generated using mLL through inversion of Type-I seesaw formula. The analysis shows that the masses of neutrinos are in agreement with the upper bound from cosmology and neutrinoless double beta decay. The results presented in this article will have important implications in discriminating the neutrinos mass models.
Keywords: Majorana phases; absolute neutrino masses; QDN models.
1. Introduction Int. J. Mod. Phys. Conf. Ser. 2018.47. Downloaded from www.worldscientific.com Since the present neutrino oscillation data1 on neutrino mass parameters are not suf- ficient to predict the three absolute neutrino masses in the case of quasi-degenerate neutrino (QDN) mass models,2–12 such mass scale is usually taken as input rang- ing from 0.1 to 0.4 eV in most of the theoretical calculations.13 As the latest
by TEZPUR UNIVERSITY on 08/05/21. Re-use and distribution is strictly not permitted, except for Open Access articles. cosmological tightest upper bound on the sum of the three absolute masses is P 14–16 i mi ≤ 0.28eV , larger value of neutrino mass m3 ≥ 0.1eV in QDN models, has been disfavoured. The upper bound on mee ≥ 0.2eV in neutrinoless double beta decay (0νββ)14–16 also disfavour larger values of neutrino mass eigenvalues with
This is an Open Access article published by World Scientific Publishing Company. It is distributed under the terms of the Creative Commons Attribution 4.0 (CC-BY) License. Further distribution of this work is permitted, provided the original work is properly cited.
1860100-1 June 7, 2018 8:55 WSPC/CRC 9.75 x 6.5 1860100
N. K. Francis & A. Nath
same CP-parity. Some important points for further investigations in QDN models for both NH and IH patterns are searches for QDN models which can accomodate lower values of absolute neutrino masses m3 ≥ 0.09eV , solar mixing angle which is lower than tribimaximal mixing (TBM)17 and effects of CP-phases on neutrino masses. In this paper, we introduce a general classification for QDN models based on their CP-parity patterns and then parameterize the mass matrix within µ − τ symmetry, and finally, numerical calculations are carried out.
2. Parameterizations of neutrino mass matrix A general µ-τ symmetric neutrino mass matrix18–20 with its four unknown inde- pendent matrix elements, requires at least four independent equations for realistic numerical solution. m11 m12 m13 mLL = m21 m22 m23 (1) m31 m32 m33
The three mass eigenvalues mi and solar mixing angles θ12 are given by, √ m1 = m11 − 2 tan θ12m12, √ m2 = m11 + 2 cot θ12m12, (2)
m3 = m22 − m23. √ 2 2m12 Thus, tan 2θ12 = (3) m11 − m22 − m23 2 2 2 The observed mass-squared differences are calculated as 4m12 = m2 − m1 > 0, 2 2 2 4m32 = m3 − m2 . In the basis where charged lepton mass matrix is diagonal, we have the leptonic mixing matrix UPMNS = U, where cos θ12 sin θ12 0 U = sin√θ12 cos√θ12 − √1 (4) PMNS 2 2 2 sin√θ12 cos√θ12 1 2 2 2 Int. J. Mod. Phys. Conf. Ser. 2018.47. Downloaded from www.worldscientific.com The mass parameters mee in νββ decay and the sum of the absolute neutrino masses P in WMAP cosmological bound mi are given respectively by, 2 2 2 mee = m1Ue1 + m2Ue2 + m3Ue3 (5)
and mcosmos = m1 + m2 + m3 (6) by TEZPUR UNIVERSITY on 08/05/21. Re-use and distribution is strictly not permitted, except for Open Access articles. A general classification for three-fold quasi-degenerate neutrino mass models18, 19 with respect to Majorana CP-phases in their three mass eigenvalues, is adopted here. Diagonalisation of left-handed Majorana neutrino mass matrix mLL in Eq. T 1 is given by mLL = UDU , where U is the diagonalising matrix in Eq. 7 and iα iβ Diag= D(m1, m2e , m3e ) is the diagonal matrix with two unknown Majorana phases (α, β). In the basis where charged lepton mass matrix is diagonal, the leptonic 20 mixing matrix is given by U = UPMNS. We, then, adopt the following classificaion
1860100-2 June 7, 2018 8:55 WSPC/CRC 9.75 x 6.5 1860100
The Effects of Majorana Phases in Estimating the Masses of Neutrinos
Table 1. The absolute neutrino masses in eV, estimated from oscillation data using calculated ψ = 0.031667 as defined in the text.
Input m3 Calculated ρ NH-QD IH-QD m1 m2 m1 m2 0.40 0.015 0.39689 0.39699 0.40289 0.40299 0.10 0.24 0.08674 0.8718 0.11104 0.11136 0.08 0.375 0.06264 0.6326 0.09340 0.09381
according to their CP-parity patterns in the mass eigenvalues mi namely Type IA: (+-+) for D= Diag(m1, −m2, m3); Type IB: (+++) for D= Diag(m1, m2, m3) and Type IC: (++-) for D= Diag(m1, −m2, −m3) respectively. We now introduce the following parameterization for µ-τ symmetric neutrino mass matrices µLL which could satisfy the above classifications.18, 19
2.1. Parameterizations: In the next step, we parameterize the mass matrix Eq. 1 into three types:
18, 19 Type IA with D= Diag(m1, −m2, m3): The mass matrix of this type can be parameterized using two parameters (,η): − 2η −c −c 1 1 mLL = −c 2 − dη − 2 − η m0 (7) 1 1 −c − 2 − η 2 − dη √ 2c 2 This predicts the solar mixing angle, tan θ12 = − 1+(d−1) η . When c = d = 1.0, we √ 2 get the Tri-Bimaximal Mixing(TBM) tan 2θ12 = −2 2(tan θ12 = 0.50) and the values of and η are calculated for both NH-QD and IH-QD cases, by using the values of Table-1 in these two expressions: m1 = (2−2η)m3 and m2 = (−−2η)m3. 2 We calculate for tan θ12 = 0.50 and tan θ12 = 0.45. The solar angle can be further lowered by taking the values c < 1 and d > 1 while using the earlier values of and η extracted using TBM.
Int. J. Mod. Phys. Conf. Ser. 2018.47. Downloaded from www.worldscientific.com 18, 19 Type-IB with D= Diag(m1, m2, m3): This type of quasi-degenerate mass pattern is given by the mass matrix, 1 − − 2η c c mLL = c 1 − dη −η m3 (8)
by TEZPUR UNIVERSITY on 08/05/21. Re-use and distribution is strictly not permitted, except for Open Access articles. c −η 1 − dη This predicts the solar mixing angle, √ 2c 2 tan 2θ12 = η (9) 1 + (1 − d) which gives the TBM solar mixing angle with the input values c=1 and d=1. Like in Type-IA, here and η values are computed for NH-QD and IH-QD, by using Table-1 in m1 = (1 − 2 − 2η)m3 and m2 = (1 + 2 − 2η)m3. m1 = (1 − 2 − 2η)m3.
1860100-3 June 7, 2018 8:55 WSPC/CRC 9.75 x 6.5 1860100
N. K. Francis & A. Nath
Type-IC with D= Diag(m1, m2, −m3): It is not necessary to treat this model18, 19 separately as it is similar to Type-IB except the interchange of two matrix elements (22) and (23) in the mass matrix in Eq. 8, and this effectively imparts an additional odd CP-parity on the third mass eigenvalue m3 in Type-IC. Such change does not alter the predictions of Type-IB. Our numerical results for both tan θ12 =0.5 and 0.45 cases, in all types of QD models (Type-IA, IB) are con- sistent with observational bound from cosmological and both NH and IH patterns are valid within quasi-degenerate model.
3. Numerical Analysis and Results For numerical computation of absolute neutrino masses, we take the following obser- 2 2 2 −5 2 2 2 2 vational data: 4m12 = m2 − m1 = 7.6 × 10 eV , 4m32 = m3 − m2 = 4m2 2 −3 2 | 23| 4m21 2.40 × 10 eV ; and define the following parameters φ = m2 and ψ = 2 , 3 |4m23| where m3 is the input quantity. For NH-QD, the other two mass eigenvalues are √ p estimated from m2 = m3 1 − φ; m1 = m3 1 − φ(1 + ψ) and for IH-QD from √ p m2 = m3 1 + φ; m1 = m3 1 + φ(1 − ψ). For suitable input value of m3, one can estimate the values of m1 and m2 for both NH-QD and IH-QD cases, using the 2 2 observational values of 4m23 and 4m21. Table-1 gives the calculated numerical 2 −5 2 values for two models namely, NH-QD and IH-QD for 4m23 = 7.6 × 10 eV 2 −3 2 and 4m21 = 2.40 × 10 eV .
4. Conclusion We have studied the effects of Majorana phases on the predictions of absolute neu- trino masses in three types of quasi-degenerate neutrino mass models having both normal and inverted hierarchical patterns within µ-τ symmetry. These predictions are consistent with data on the mass squared difference derived from various oscil- lation experiments, and from the upper bound on absolute neutrino masses in 0νββ as well as upper bound of cosmology. The results presented in this article will have important implications in the discrimination of neutrino mass models. Int. J. Mod. Phys. Conf. Ser. 2018.47. Downloaded from www.worldscientific.com
Acknowledgements This work is carried out through the DST-SERB, Govt. of India, Research project entitled “Neutrino mass ordering, leptonic CP violation and matter- by TEZPUR UNIVERSITY on 08/05/21. Re-use and distribution is strictly not permitted, except for Open Access articles. antimatter asymmetry” vide grant no. EMR/2015/001683.
References 1. T. Schwetz, M. T´ortolaand J. W. Valle, Three-flavour neutrino oscillation update, New Journal of Physics 10, p. 113011 (2008). 2. M. Maltoni and T. Schwetz, Three-flavour neutrino oscillation update and comments on possible hints for a non-zero θ13, arXiv preprint arXiv:0812.3161 (2008).
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The Effects of Majorana Phases in Estimating the Masses of Neutrinos
3. A. Bandyopadhyay, S. Choubey, R. Gandhi, S. Goswami, B. Roberts, J. Bouchez, I. Antoniadis, J. Ellis, G. Giudice, T. Schwetz et al., Physics at a future neutrino factory and super-beam facility, Reports on Progress in Physics 72, p. 106201 (2009). 4. A. S. Joshipura, Almost degenerate neutrinos, Zeitschrift f¨urPhysik C Particles and Fields 64, 31 (1994). 5. S. T. Petcov and A. Y. Smirnov, Neutrinoless double beta decay and the solar neutrino problem, Physics Letters B 322, 109 (1994). 6. A. S. Joshipura and K. M. Patel, Quasidegenerate neutrinos in SO(10), Physical Review D 82, p. 031701 (2010). 7. R. Barbieri, L. J. Hall, G. L. Kane and G. G. Ross, Nearly degenerate neutrinos and broken flavour symmetry, arXiv preprint hep-ph/9901228 (1999). 8. S. Antusch and S. F. King, From hierarchical to partially degenerate neutrinos via type II upgrade of type I see-saw models, Nuclear Physics B 705, 239 (2005). 9. P. Binetruy, S. Lavignac, S. Petcov and P. Ramond, Quasi-degenerate neutrinos from an abelian family symmetry, Nuclear Physics B 496, 3 (1997). 10. G. C. Branco, M. N. Rebelo and J. I. Silva-Marcos, Degenerate and quasidegenerate majorana neutrinos, Physical Review Letters 82, p. 683 (1999). 11. G. C. Branco, M. N. Rebelo and J. I. Silva-Marcos, Quasi degenerate neutrino masses with universal strength yukawa couplings, Physics Letters B 428, 136 (1998). 12. S. Pascoli and S. T. Petcov, Majorana neutrinos, neutrino mass spectrum, and the |< m >| = 10−3eV frontier in neutrinoless double beta decay, Physical Review D 77, p.113003 (2008). 13. I. de Medeiros Varzielas, G. G. Ross and M. Serna, Quasidegenerate neutrinos and tribimaximal mixing, Physical Review D 80, p. 073002 (2009). 14. P. Harrison and W. Scott, µ − τ reflection symmetry in lepton mixing and neutrino oscillations, Physics Letters B 547, 219 (2002). 15. P. F. Harrison, D. H. Perkins and W. Scott, Tri-bimaximal mixing and the neutrino oscillation data, Physics Letters B 530, 167 (2002). 16. P. Harrison and W. Scott, Permutation symmetry, tri-bimaximal neutrino mixing and the S3 group characters, Physics Letters B 557, 76 (2003). 17. G. Altarelli and F. Feruglio, Neutrino masses and mixings: a theoretical perspective, Physics reports 320, 295 (1999). 18. Z. Maki, M. Nakagawa and S. Sakata, Remarks on the uni ed model of elementary particles, Progress of Theoretical Physics 28, 870 (1962). 19. B. Pontecorvo, Neutrino experiments and the problem of conservation of leptonic charge, Sov. Phys. JETP 26, p. 165 (1968).
Int. J. Mod. Phys. Conf. Ser. 2018.47. Downloaded from www.worldscientific.com 20. N. K. Francis and N. N. Singh, Validity of quasi-degenerate neutrino mass models and their predictions on baryogenesis, Nuclear Physics B 863, 19 (2012). by TEZPUR UNIVERSITY on 08/05/21. Re-use and distribution is strictly not permitted, except for Open Access articles.
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Review Talks
Thermal WIMPs on the Brink Tim Linden
Exploring the Extreme Universe with Gamma-ray Observations Reshmi Mukherjee
Highlight Talks
The CALorimetric Electron Telescope (CALET) on the Yoichi Asaoka International Space Station
Recent Results of Cosmic Ray Measurements from Dennis Soldin IceCube and IceTop
Latest Results from the Alpha Magnetic Spectrometer on Bruna Bertucci the International Space Station
Neutrino - NU5
ANTARES-IceCube Combined Search for Neutrino Giulia Illuminati Point Sources in the Southern Hemisphere
All Sky Time-Integrated Point Source Searches using Tessa Carver https://www.icrc2019.org/presentations.html 9/27 30/09/2020 Presentations
10 years of IceCube Data Home Registration Program Meeting Site Proceedings Organization Prizes & Awards Contact Us
Search for High-energy Neutrinos from AGN Cores Federica Bradascio
Search for Astronomical Neutrino from Blazar Kaito Hagiwara TXS0506+056 in Super-Kamiokande
Searching for Time-Dependent Neutrino Emission Erin O'Sullivan from Blazars
Cosmic Ray Indirect - CRI5
The Effects of the Galactic Magnetic Field on UHECR Andrew M. Taylor From Local Sources
Evidence for UHECR Origin in Starburst Galaxies Jorge F. Soriano
Search for magnetically-induced signatures in the arrival directions of ultra-high energy cosmic rays measured Marcus Wirtz by the Pierre Auger Observatory
Developments in Modeling the Galactic Magnetic Glennys Farrar Field
Propagation of Ultra-high-energy Cosmic Rays in the Jihyun Kim Magnetized Cosmic Web
New constraints on galactic CRE transport from radio Ralf-Juergen Dettmar continuum observations
Cosmic Ray Indirect - CRI6
Latest results for Proton-proton Cross Section Francesco Cafagna Measurements with the TOTEM experiment at LHC
Future Proton-Oxygen Beam Collisions at the LHC for Hans Dembinski Air Shower Physics
The results and future prospects of the LHCf Hiroaki Menjo experiment
Measurements of the very-forward energy in pp collisions at the LHC and constraints for cosmic ray air Sebastian Baur showers
The Cosmic-Ray Program of the NA61/SHINE facility Michael Unger at the CERN SPS
Collective Hadronization and Air Showers: Can LHC Tanguy Pierog Data Solve the Muon Puzzle ?
Solar & Heliospheric - SH4 https://www.icrc2019.org/presentations.html 10/27 30/09/2020 Presentations
Home Registration Program Meeting Site Proceedings Organization Prizes & Awards Contact Us Cosmic-ray variability on the multi-millennial time Ilya Usoskin scale: A new multi-proxy reconstruction
Obtaining a History of the Flux of Cosmic Rays using In Segev BenZvi Situ Cosmogenic Carbon-14 Trapped in Polar Ice
Spectra of solar energetic particle and galactic cosmic rays over a million years reconstructed using aluminium-26 data Stepan V. Poluianov from lunar rocks
Long-term variation of galactic cosmic ray intensity Kazuoki Munakata observed with the Nagoya multidirectional muon detector
27-Day Modulation of Cosmic Ray Intensities During Richard A. Leske the Last Two Solar Minima
Gamma Ray Direct - GAD2
Shell like Supernova Remnants Observed with Francesco de Palma Fermi-LAT
Gamma-ray Spectral and Morphological study of David Green HESS J1912+101 observed by MAGIC and Fermi-LAT
Efficient particle acceleration from HESS J1640.6- Arnaud Mares 4633 and the PeVatron candidate HESS J1641.0-4619
Gamma-ray Pulsars with DAMPE Maria Munoz
Energy-dependent morphology of the pulsar wind Giacomo Principe nebula HESS J1825-137 seen by the Fermi-LAT
휂 Carinae: particle acceleration and multi-messenger Roland Walter aspects
Gamma Ray Indirect - GAI5
MAGIC eyes to the extreme: testing the blazar Elisa Prandini emission models on EHBLs
ValueObservations of the FSRQ 3C 279 during the flaring Gabriel Emery state of June 2018 with H.E.S.S
FACT - Highlights from more than Seven Years of Thomas Bretz Unbiased Monitoring at TeV Energies
Variability Study of Extreme Blazars with VERITAS Orel Gueta
Resolving the kpc jet of Centaurus A in TeV gamma- Mathieu de Naurois rays
https://www.icrc2019.org/presentations.html 11/27 30/09/2020 Presentations
Studying the Extreme Behaviour of 1ES 2344+51.4 Axel Arbet-Engels Home Registration Program Meeting Site Proceedings Organization Prizes & Awards Contact Us
VHE detection and monitoring of the radio galaxy 3C Jodi Christiansen 264
Investigating the unusually hard gamma-ray Thomas Weisgarber spectrum of the extreme blazar 1ES 0229+200 with HAWC
Cosmic Ray Indirect - CRI7
Cosmic Ray Spectrum and Composition from PeV to Karen G. Andeen EeV from the IceCube Neutrino Observatory
The Energy Scale of the Pierre Auger Observatory Bruce R. Dawson
Measurement of the Cosmic Ray Flux near the Alan Coleman Second Knee with the Pierre Auger Observatory
Measurement of the energy spectrum of ultra-high Valerio Verzi energy cosmic rays using the Pierre Auger Observatory
Energy Spectrum Measured by the Telescope Array Dmitri Ivanov
The energy spectrum of ultra-high energy cosmic rays measured at the Pierre Auger Observatory and at the Olivier Deligny Telescope Array
From the Observation of UHECR Radio Signal in [1- 200] MHz to the Composition: CODALEMA and EXTASIS Antony Escudie Status Report
Cosmic Ray Direct - CRD5
Non-linear Diffusion of Cosmic Rays Escaping from Supernovae Remants in the Cold Partially Neutral Atomic Loann Brahimi and Molecular Phases
Study on the anisotropic diffusion and large-scale Hongbo Hu anisotropy of the galactic cosmic rays
Core-collapse Supernovae as Cosmic Ray Sources Vikram V. Dwarkadas
Acceleration and escape of first cosmic rays Yutaka Ohira
Particle acceleration by shock waves propagating in a Shota Yokoyama non-uniform medium
Three dimensional global test particle simulation of Shoma Kamijima cosmic-ray acceleration and escape in supernova remnants
On the Spectrum of Electrons Accelerated in Rebecca Diesing Supernova Remnants https://www.icrc2019.org/presentations.html 12/27 30/09/2020 Presentations
Cosmic RayH oIndirectme Re g-is CRI8tration Program Meeting Site Proceedings Organization Prizes & Awards Contact Us
Cosmic-ray detection with and novel reconstruction Anna Nelles algorithms for the ARIANNA experiment
Seven years of Tunka-Rex operation Vladimir Lenok
Coherent transition radiation from the geomagnetic Krijn D. de Vries air shower current
Symmetrizing the signal distribution of radio emission Tim Huege from inclined air showers
Frequency-optimised radio air shower arrays for Aswathi Balagopal V. enhanced performance
Measurements of Inclined Air Showers with the Auger Marvin Gottowik Engineering Radio Array at the Pierre Auger Observatory
The energy scale of cosmic rays detected with LOFAR Katharine Mulrey
Neutrino - NU6
Multi-messenger Gravitational-Wave + High-Energy Azadeh Keivani Neutrino Searches with LIGO, Virgo and IceCube
IceCube Search for Galactic Neutrino Sources based Ali Kheirandish on HAWC Observations of the Galactic Plane
Search for Correlations of High-energy Neutrinos and Anastasia Maria Ultra-high Energy Cosmic Rays Barbano
ANTARES 2007-2017 Search for Point Sources Using Sergio Navas All Neutrino Flavours
Probing neutrino emission at GeV energies from Gwenhaël De compact binary mergers with IceCube Wasseige
A DECam Search for Explosive Optical Transients Robert A. Morgan Associated with IceCube Neutrinos
Observation of Optical Transients and Search for PeV- Satoru Ogawa EeV Tau Neutrinos with Ashra-1
ANTARES search for high-energy neutrinos from TeV- emitting blazars, Markarian 421 and 501, in coincidence with Mukharbek Organokov HAWC gamma-ray flares
Monday, July 29th
https://www.icrc2019.org/presentations.html 13/27 30/09/2020 Presentations Review Talks Home Registration Program Meeting Site Proceedings Organization Prizes & Awards Contact Us
The Dynamical Role of Cosmic Rays in Galaxies Ellen Zweibel
Highlight Talks
Results from IceCube Dawn Williams
Probing High-Energy Hadronic Interactions with Lorenzo Cazon Extensive Air Showers
Combined Dark Matter Searches Towards Dwarf Spheroidal Galaxies with Fermi-LAT, HAWC, HESS, MAGIC and Louise Oakes VERITAS
Cosmic Ray Indirect - CRI9
Search for the diffuse gamma ray emission from the Yuhua Yao galactic plane in 100 TeV region
Non-thermal emission from the reverse shock of the Martin Pohl youngest galactic Supernova remnant G1.9+0.3
Undiscovered Pulsar as the Explanation of the High- Ruben Lopez-Coto energy Cosmic Ray All-electron Flux
Gamma-Ray Bursts as Sources of Ultra-High Energy Daniel Biehl Cosmic Rays across the Ankle
Ultra-high-energy cosmic rays by Cygnus A or the bulk Björn Eichmann of non-local radio galaxies?
A parametrized catalog of radio galaxies as UHECR Jörg P. Rachen sources
Gamma Ray Indirect - GAI6
Searching for Variability of the Crab Nebula Flux at TeV Energies using MAGIC Very Large Zenith Angle Juliane van Scherpenberg Observations
Orbital parameters for the gamma-ray binaries LMC Brian van Soelen P3 and 1FGL J1018.6-5856
Long-term gamma-ray observations of the binary Gernot Maier HESS J0632+057 with H.E.S.S., MAGIC and VERITAS
Probing orbital parameters of gamma-ray binaries Iurii Sushch with TeV light curves
X-ray and TeV gamma-ray emission from the 50-year Tyler Williamson https://www.icrc2019.org/presentations.html 14/27 30/09/2020 Presentations
period binary system PSR J2032+4127/MT91 213 Home Registration Program Meeting Site Proceedings Organization Prizes & Awards Contact Us
Characterizing the VHE Emission of LS I +61 303 using David Kieda VERITAS Observations
Neutrino - NU7
The IceCube Upgrade - Design and Science Goals Aya Ishihara
KM3NeT/ORCA Detector for Neutrino Research at the Bruno Strandberg Bottom of the Mediterranean Sea
Neutrino telescope in Lake Baikal: Present and Future Fedor Simkovic
Status and prospects of the Hyper-Kamiokande Yoshitaka Itow project
Performance of the ARIANNA pilot array, and implications for the next generation of UHE neutrino Christian Glaser detectors
Radio Phased Arrays: A low-threshold detector in the Eric Oberla Askaryan Radio Array (ARA)
Solar & Heliospheric - SH5
ORCA (Antarctic Cosmic Ray Observatory): 2018 Juan Jose Blanco Latitudinal Survey
Galactic Cosmic-Ray Anisotropy During Forbush Decreases: Alejandro Sáiz Evidence for Diffusive Barriers and Large-Scale Flow
Long Duration Gamma-ray Flares and High Energy G.A. de Nolfo Solar Energetic Particles: Is there a Connection?
Modeling the 2017 September 10 Long Duration James Ryan Gamma Ray Flare
Solar Energetic Particles measured by the Alpha Magnetic Spectrometer on the International Space Station during solar Veronica Bindi cycle 2
Gamma Ray Direct - GAD3
Recent Gamma-ray Results from DAMPE Xiang Li
All-Sky Medium Energy Gamma-ray Observatory Alexander Moiseev (AMEGO)
High-Energy Gamma-ray Observations Using the Masaki Mori CALorimetric Electron Telescope (CALET) on the ISS https://www.icrc2019.org/presentations.html 15/27 30/09/2020 Presentations
GRAINE project and first results on 2018 balloon- Satoru Takahashi Home Registration Program Meeting Site Proceedings Organization Prizes & Awards Contact Us borne experiment
BurstCube: Mission Concept, Performance, and Jacob Smith Status
Overview of the POLAR Mission Jinchao Sun
Cosmic Ray Indirect - CRI10
A New View on Auger Data and Cosmogenic Neutrinos in Light of Different Nuclear Disintegration and Air- Anatoli Fedynitch shower Models
Ultra-high Energy Cosmic Rays and Neutrinos from Soebur Razzaque Light Nuclei Composition
Cosmic ray transport in starburst galaxies and Enrico Peretti possible observables
Constraints on UHECR sources and their environments, from fitting UHECR spectrum and composition, Marco Muzio and neutrinos and gammas
Follow-up searches for ultra-high energy neutrinos and photons from transient astrophysical sources with the Michael Schimp Pierre Auger Observtory
Telescope Array Search for EeV Photons Mikhail Kuznetsov
POEMMA: Probe Of Extreme Multi-Messenger Angela V. Olinto Astrophysics
Gamma Ray Indirect - GAI7
Extreme High-energy Peaked BL Lac Objects and their TeV Gamma-ray Emission: Are They a Homogeneous Luca Foffano Population?
A Northern Sky Survey for 100TeV Gamma-ray Sources Using the Tibet Air Shower Array and Muon Xu Chen Detector Array
Possible origin of the slow-diffusion region around Kun Fang Geminga
Spectral and Morphological Studies of the Very High Francisco Salesa Energy Gamma-Ray Source 2HWC J1825-134 Greus
Electron Spectrum of the Dragonfly Pulsar Wind Chad Brisbois Nebula from X-ray to TeV
https://www.icrc2019.org/presentations.html 16/27 30/09/2020 Presentations
Highlights of Galactic Physics with VERITAS Gregory T. Richards Home Registration Program Meeting Site Proceedings Organization Prizes & Awards Contact Us
Gamma Ray Indirect - GAI8
MAGIC observation and broadband characterization Mitsunari Takahashi of the remarkably bright flares of 1ES 1959+650 in 2016
Sub-parsec and parsec VHE emission from the core of Juan C. Rodríguez LLAGNs Ramírez
Revisit of non-linear Landau damping for electrostatic Martin Pohl instability driven by blazar-induced pair beams
Unravelling the complex behavior of Mrk421 with simultaneous X-ray and VHE observations during an extreme flaring activity in Ana Babic April 2013
Highlights from the VERITAS AGN Observation Wystan Benbow Program
A survey of active galaxies with the HAWC gamma-ray Alberto Carramiñana observatory
Broadband emission of blazar S5 0716+714 during Yuki Kajiwara impressive outbursts
A 3-year HAWC/Swift monitoring of gamma-ray/X- José Andrés García- ray flux and correlations in the BL Lac Mrk 421 González
Cosmic Ray Direct - CRD6
Cosmic ray transport from AMS-02 B/C data: Yoann Genolini reference parameters and physical interpretation
Properties of Secondary Cosmic Rays Lithium, Beryllium and Boron Measured by the Alpha Magnetic Alberto Oliva Spectrometer on the International Space Station
Cosmic-Ray Helium Isotopes with the Alpha Carlos Delgado Magnetic Spectrometer
Cosmic-Ray Lithium Isotopes with the Alpha Laurent Derome Magnetic Spectrometer
Overall Status of the High Energy Cosmic Radiation Yongwei Dong Detection Facility Onboard the Future China's Space Station
Fitting B/C cosmic-ray data in the AMS-02 era Laurent Derome
Is the B/C slope in AMS-02 data actually telling us Manuela Vecchi something about the diffusion coefficient slope ?
https://www.icrc2019.org/presentations.html 17/27 30/09/2020 Presentations
Cosmic-ray Isotope Measurements with HELIX Nahee Park Home Registration Program Meeting Site Proceedings Organization Prizes & Awards Contact Us
Dark Matter - DM1
Potential Dark Matter Signals at Neutrino Telescopes Marco Chianese
Interpretation of the CALET Electron+Positron Holger M. Motz Spectrum concerning Dark Matter Signatures
Searches for dark matter with the ANTARES and Rebecca Gozzini KM3NeT neutrino telescopes
Status of cosmic-ray antinuclei searches Philip von Doetinchem
Constraints on dark matter scattering with long-lived Davide Serini mediators using gamma-rays from the Sun
Perspective on dark matter annihilation limits from the LHAASO gamma-ray observation of dwarf Spheroidal Xiaojun Bi galaxies
Reverse Direct Detection: Cosmic Ray Scattering With Kenny C. Y. Ng Light Dark Matter
Recent Results from the Dark Matter Search of Dan Baxter DAMIC-100 at SNOLAB
Tuesday, July 30th
Review Talks
Physics and Astrophysics with Ultra-High Energy Cosmic Abigail Vieregg Neutrinos
Gamma-ray Insights into Cosmic-ray transport Gwenael Giacinti
Highlight Talks
Testing cosmic ray acceleration in the laboratory Subir Sarkar
Highlights from the Tibet ASgamma Experiment Kazumasa Kawata
Results from the Mediterranean neutrino detectors Rosa Coniglone
Cosmic Ray Indirect - CRI11
Large-scale anisotropies above 0.03 EeV measured Esteban Roulet by the Pierre Auger Observatory
Full-sky searches for anisotropies in UHECR arrival directions Armando di Matteo https://www.icrc2019.org/presentations.html 18/27 30/09/2020 Presentations
with the Pierre Auger Observatory and the Home Registration Program Meeting Site Proceedings Organization Prizes & Awards Contact Us Telescope Array
Anisotropy in the mass composition from the Yana Zhezher Telescope Array Surface Detector data
On the origin of ultra-high energy cosmic ray Chen Ding anisotropy
Anisotropies of the Highest Energy Cosmic-ray Events Recorded by the Pierre Auger Observatory in 15 years Lorenzo Caccianiga of Operation
Supergalactic Structure of Energy-Angle Correlations Jon Paul Lundquist
Gamma Ray Indirect - GAI9
Study of Middle-aged Pulsar Wind Nebulae Showing Large Offsets Between their Pulsar and their VHE Gamma- ray Michelle Tsirou Emission
Highest Energy Photons Ever Observed and High- James T. Linnemann Energy Crab Spectrum
The Crab Nebula Spectrum at ~ 100 TeV Measured Michele Peresano With MAGIC Under Very Large Zenith Angles
Modeling of Broadband Spectra and Radial Profiles of Wataru Ishizaki Emission of Pulsar Wind Nebulae
Neutrino - NU8
Measurement of the Atmospheric Neutrino Matthew Strait Oscillation Parameters with NOvA
High-energy Neutrino Event Simulation at NLO in Alfonso Garcia Genie for KM3NeT and Other Observatories
A new calculation of Earth-skimming very- and ultra- Mary Hall Reno high energy tau neutrinos
Characterizing the High Energy Activity of Blazars Ankur Sharma Possibly Correlated with Observed Astrophysical Neutrinos
First double cascade tau neutrino candiates in IceCube and a new measurement of the flavor composition” is Juliana Stachurska confirmed
Cosmic Ray Direct - CRD7
Properties of Primary Cosmic Rays Neon, Magnesium and Qi Yan https://www.icrc2019.org/presentations.html 19/27 30/09/2020 Presentations
Silicon Measured with the Alpha Magnetic Spectrometer on the Home Registration Program Meeting Site Proceedings Organization Prizes & Awards Contact Us ISS
Elemental analysis of Cosmic-Ray flux with DAMPE Ya-Peng Zhang
Cosmic-Ray Elemental Spectra Measured with ISS- Ryuji Takeishi CREA
The Status of DAMPE Satellite in Space Yunlong Zhang
Cosmic Ray Energetics And Mass for the International Eun-Suk Seo Space Station (ISS-CREAM)
Dark Matter - DM2
Searching for Dark Matter decay signals in the Daniele Ninci Galactic halo with the MAGIC telescopes
Recent results from the DM-Ice17 and COSINE-100 Jay Hyun Jo experiment
Dark Matter Search with H.E.S.S. Towards Ultra-faint Lucia Rinchiuso Dwarf Nearby DES Satellites of the Milky Way
Combined Search for Neutrinos from Dark Matter Nadège Iovine Annihilation in the Galactic Centre using ANTARES and IceCube
Cosmic Ray Indirect - CRI12
Espresso Acceleration of Ultra-High-Energy Cosmic Rostom Mbarek Rays in Realistic Jet Environments
Electron Acceleration at Rippled Low Mach Number Jacek Niemiec Shocks in Merging Galaxy Clusters
The role of re-acceleration in the understanding of Martina Cardillo Cosmic-Ray direct and indirect data
The Issue with Diffusive Shock Acceleration Damiano Caprioli
Modeling the saturation of the Bell instability using Georgios Zacharegkas hybrid simulations
Acceleration of He nuclei at non-relativistic Cory Cotter collisionless shocks
On measuring the cosmic-ray production rate in Jiro Shimoda supernova remnant shocks by polarized Balmer line emission
Gamma Ray Indirect - GAI10
Constraining the magnetic field in the EM170817 Stefan Ohm https://www.icrc2019.org/presentations.html 20/27 30/09/2020 Presentations
ejecta with H.E.S.S. observation Home Registration Program Meeting Site Proceedings Organization Prizes & Awards Contact Us
Gamma-rays and neutrinos from TXS 0506+056: interpretation of the 2018/2019 MAGIC and MWL Matteo Cerruti monitoring campaign
Recent results from the VERITAS multi-messenger program Marcos Santander
Search for very-high-energy photons from gamma-ray bursts Nissim Fraija with HAWC
Search for gamma-ray counterparts of gravitational wave events Israel Martinez-Castellanos with HAWC
Neutrino - NU9
Neutrino source searches and a realtime neutrino Sarah Mancina alert stream in the southern sky with IceCube starting tracks
The Next Generation of IceCube Real-time Neutrino Chun Fai Tung Alerts
Search for High-Energy Neutrinos from Populations of Robert Stein Optical Transients
Searching for Common Sources of Gravitational Raamis Hussain Waves and Neutrinos
Ten years of multi-wavelength follow-up observations Damien Dornic of ANTARES neutrino alerts
AMON: TeV Gamma and Neutrino Coincidence Alerts Hugo Alberto Ayala from HAWC and IceCube subthreshold data Solares
IceCube as a Multi-messenger Follow-up Observatory Justin for Astrophysical Transients Vandenbroucke
Search for neutrino counterparts of cataloged GW events from run O2 and offline follow-up of new GW alerts Marta Colomer Molla from run O3 with ANTARES
Cosmic Ray Direct - CRD8
Precision Measurement of the Monthly Carbon and Oxygen Fluxes in Cosmic Rays with the Alpha Magnetic Federico Donnini Spectrometer on the International Space Station
Properties of Primary Protons, Helium, Carbon and Oxygen Nuclei Measured with the Alpha Magnetic Qi Yan Spectrometer on the ISS
Precision Measurement of the Daily Proton and Helium Fluxes in Cristina Consolandi https://www.icrc2019.org/presentations.html 21/27 30/09/2020 Presentations
Cosmic Rays with the Alpha Magnetic Home Registration Program Meeting Site Proceedings Organization Prizes & Awards Contact Us Spectrometer on the International Space Station
Precision Measurement of the Monthly Proton and Helium Fluxes in Cosmic Rays with the Alpha Magnetic Nicola Tomassetti Spectrometer on the International Space Station
Measurement of the Proton Spectrum with CALET on Pier S. Marrocchesi the ISS
Measurement of the energy spectra of carbon and Paolo Maestro oxygen nuclei in cosmic rays with CALET
Measurement of cosmic ray proton spectrum with Chuan Yue the Dark Matter Particle Explorer
Helium spectrum in the cosmic rays measured by the Margherita Di Santo DAMPE detector
Solar & Heliospheric - SH6
Penetrating Particle Analyzer (PAN) Giorvani Ambrosi
Ground and flight performances of the balloon-borne Pierre-Simon Mangeard magnet spectrometer AESOP-Lite
Measurement of the low energy (20-300 MeV) electron and positron spectra with the AESOP-Lite balloon Sarah Mechbal mission
Space-Weather capabilities and preliminary results of the High Energy Particle Detector (HEPD) on-board the CSES Matteo Martucci satellite
Energetic Particle Acceleration in the Heliosphere Eric Christian from the IMAP mission
Solar Neutron and Gamma-ray Detector for a 3U Kazutaka Yamaoka CubeSat
The updated and upgraded SANAE neutron monitor Du Toit Strauss
Wednesday, July 31st
Highlight Talks
Progresses of the Dark Matter Particle Explorer Qiang Yuan experiment
Cosmogenic Evidences for Past SEP Events Fusa Miyake https://www.icrc2019.org/presentations.html 22/27 30/09/2020 Presentations
Seeing >100 TeV Gamma Rays with Extensive Air Kirsten Tollefson Home Registration Program Meeting Site Proceedings Organization Prizes & Awards Contact Us Shower Arrays
Neutrino - NU10
High-elevation synoptic radio array for detection of upward moving air-showers, deployed in the Antarctic Jiwoo Nam mountains
GRAND: science and design Olivier Martineau-Huynh
Trinity: An Air-Shower Imaging System for the Nepomuk Otte Detection of Cosmogenic Neutrinos
SuperK-Gd: The Gd future of Super-Kamiokande Lluis Marti Magro
Concept Study for the Beamforming Elevated Array Stephanie Wissel for Cosmic Neutrinos (BEACON)
Cosmic Ray Indirect - CRI13
Seasonal Variation of Atmospheric Neutrinos in Serap Tilav IceCube
Studying the Temporal Variation of the Cosmic-Ray Paolo Desiati Sun Shadow Using IceCube Data
Probing the Anomalous Flux of Very-high-energy Mehr Un Nisa Gamma rays from the Sun with HAWC
Measurement of the electrical properties of a thundercloud through muon imaging by the GRAPES-3 Hari Haran Balakrishnan experiment
Cosmic Ray Indirect - CRI14
A Cosmic Rays Tracking System for the Stability Germano Bonomi Monitoring of Historical Buildings
Improvement of cosmic-ray muography for Earth László Oláh sciences and civil engineering
Measurement of the Energy Spectrum of Nearly Ahron S. Barber Horizontal Muons with HAWC
EAS Thermal Neutron Detector Array to Add into Xinhua Ma LHAASO
Observation of electron rings with imaging air Haritha Retnakaran Cherenkov telescopes
https://www.icrc2019.org/presentations.html 23/27 30/09/2020 Presentations Solar & Heliospheric - SH7 Home Registration Program Meeting Site Proceedings Organization Prizes & Awards Contact Us
Solar Energetic Particle Observations with the Alessandro Bruno PAMELA Experiment
Re-examination of the First Five Ground-Level Events M. A. Shea
A neutron monitor as an integral spectrometer for GLE Sergey Koldobskiy analysis: Effective rigidity and reassessment of integral fluxes
Vertical Geomagnetic Cutoff Rigidities for Epoch 2015 D. F. Smart
Relativistic solar proton propagation in the Silvia Dalla interplanetary medium
Usage of the global NM network for assessment of the Alexander Mishev radiation exposure at flight altitudes
Gamma Ray Direct - GAD4
Cosmic Rays in the Orion-Eridanus Superbubble Theo Joubaud
Detection of a gamma-ray halo around Geminga Silvia Manconi with the Fermi-LAT and implications for the positron flux
The Surprising Gamma Ray emission from the Sun Kenny C. Y. Ng
A Consistent Model of the Interstellar Gamma-Ray Emission to Interpret Fermi LAT Observations of Diffuse Elena Orlando Emissions
Gamma Ray Indirect - GAI11
Search for Primordial Black Hole evaporations with H.E.S.S. Thomas Tavernier
Measurement of the Extragalactic Background Light Elisa Pueschel with VERITAS
Constraints on Lorentz invariance violation using Humberto Martínez-Huerta HAWC observations above 100 TeV
A Systematic Search for TeV Halos associated with Andrew Smith known pulsars
Positrons and 511 keV radiation as tracers of recent Volodymyr Takhistov binary neutron star mergers
New stringent LIV limits from astrophysical gamma-ray sources Rodrigo Guedes Lang
Cosmic Ray Indirect - CRI15
https://www.icrc2019.org/presentations.html 24/27 30/09/2020 Presentations
Hadronic interactions and EAS muon multiplicity investigated Liuming Zhai Home Registration Program Meeting Site Proceedings Organization Prizes & Awards Contact Us with the new Tibet hybrid experimental muon data
Measurement of the fluctuations in the number of muons in Felix Riehn inclined air showers with the Pierre Auger Observatory
Study on the muon lateral distribution based on the Guangguang Xin first stage of LHAASO-KM2A
The muon component of extensive air showers above 10^17.5 Federico Sánchez eV measured with the Pierre Auger Observatory
Working Group Report on the Combined Analysis of Muon Density Measurements from Eight Leading Air Shower Lorenzo Cazon Experiments
A study of the uncertainty due to hadron models on Moon Moon Devi UHECR: the impact on the secondary particles
Spatial and Temporal Characteristics of EAS with Dmitriy Beznosko Delayed Particles
Probing the High Energy Spectrum of Neutral Pions Ruben Conceição in Ultra-high-energy Proton-Air Interactions
Neutrino - NU11
Enabling a New Detection Channel for BSM Physics Anna Pollmann with in-situ Measurements of Luminescence
The Baikal-GVD neutrino telescope: muon track Lukáš Fajt events reconstruction
Astrophysical Tau Neutrino Identification with Logan Wille IceCube Waveforms
NU11d: Light diffusion in birefringent polycrystals and the Dmitry Chirkin IceCube ice anisotropy
Exciting Prospects for Detecting Late-Time Neutrinos Shirley Li from Core-Collapse Supernovae
Coherent radar reflections from an electron-beam Steven Prohira induced particle cascade
Investigations of ice and emitter properties from Robert Lahmann radio signals recorded with ARIANNA
Cosmic Ray Indirect - CRI16
The Large-scale Anisotropy of Cosmic Rays Wei Gao Observation with the Partial LHAASO-KM2A Arrays https://www.icrc2019.org/presentations.html 25/27 30/09/2020 Presentations
Large-scaleHome CosmicRegi sRaytrat Anisotrion opyPro withgram Tibet airMe eting Site Proceedings Organization Prizes & Awards Contact Us Yi Zhang shower array
The Anisotropy of CRs Observed by YBJ-HA Experiment Yingying Guo
Observation of cosmic ray anisotropy with GRAPES-3 Pravata Mohanty Experiment
The anisotropy of cosmic rays observed by the Tibet Yoshiaki Nakamura air shower array and muon detector array
Particle-in-Cell Simulations of Relativistic Weibel Sara Tomita Mediated Shocks Propagating into Inhomogeneous Media
Cosmic-Ray Transport between the Knee and the Lukas Merten Ankle with CRPropa
Understanding the Linear and Nonlinear Effects of Cosmic Ray Streaming Instabilities with Self Consistent Colby Haggerty Hybrid Simulations
Dark Matter - DM3
Dark Matter Searches with HAWC Joseph Lundeen
Constraints on cross section and lifetime of dark Sergio Hernández Cadena matter with HAWC Observations of dwarf Irregular galaxies
Setting Upper Limits on the Local Burst Rate Density Kristi Engel of Primordial Black Holes Using HAWC
Search for dark photons as candidates for Dark Ralph Engel Matter with FUNK
Searching for ultra-faint galaxies in three years of Keith Bechtol data from the Dark Energy Survey
Voyager Probing Dark Matter Mathieu Boudaud
Status of the Galactic Center Gamma-Ray and Carlos Blanco Cosmic-Ray Antiproton Excesses
New Venues in Formation and Detection of Volodymyr Takhistov Primordial Black Hole Dark Matter
Thursday, August 1st
Rapporteur Talks
Cosmic Ray Direct Observations Roberta Sparvoli https://www.icrc2019.org/presentations.html 26/27 30/09/2020 Presentations
Gamma rays: direct observations Riccardo Rando Home Registration Program Meeting Site Proceedings Organization Prizes & Awards Contact Us
News on Cosmic-Ray Air Showers (CRI) Frank Schröder
Solar and Heliospheric Physics Silvia Dalla
Neutrinos Alexander Kappes
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