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Related papers: Probing the general axion-nucleon interaction in w…

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In this study, we present the first multidimensional core-collapse supernovae (CCSNe) simulations including QCD axions in order to assess the impact on the CCSN explosion mechanism. We include axions in our simulations through the…

High Energy Astrophysical Phenomena · Physics 2022-09-26 Aurore Betranhandy , Evan O'Connor

We present a new design for the water Cherenkov detectors that are in use in various cosmic ray observatories. This novel design can provide a significant improvement in the independent measurement of the muonic and electromagnetic…

Instrumentation and Methods for Astrophysics · Physics 2015-06-19 Antoine Letessier-Selvon , Pierre Billoir , Miguel Blanco , Ioana C. Maris , Mariangela Settimo

We investigate the existence of bound $\Xi$ \break states in systems with $A=4-7$ baryons using the Jacobi NCSM approach in combination with chiral NN and $\Xi$N interactions. We find three shallow bound states for the NNN$\Xi$ system (with…

Nuclear Theory · Physics 2022-01-05 Hoai Le , Johann Haidenbauer , Ulf-G. Meißner , Andreas Nogga

The Born approximation to the quark-gluon-exchange mechanism for K$^+$N scattering is used as a starting point to generate a potential for this system. The valence quark wave function of the nucleon is generalized from a single Gaussian to…

Nuclear Theory · Physics 2008-05-20 W. R. Gibbs , R. Arceo

Scattering of neutrons in the 24-150 keV incident energy range from H2O relative to that of D2O and H2O-D2O mixtures was reported very recently. Studying time-of-flight integrated intensities, the applied experimental procedure appears to…

Other Condensed Matter · Physics 2007-05-23 C. A. Chatzidimitriou-Dreismann

Supernova 1987A remains the most well-observed and well-studied supernova to date. Observations produced excellent broad-band photometric and spectroscopic coverage over a wide wavelength range at all epochs. Here, we focus on the very…

We discuss the diffuse flux of electron neutrinos and antineutrinos from cosmological failed supernovae, stars that collapse directly into a black hole, with no explosion. This flux has a hotter energy spectrum compared to regular,…

Cosmology and Nongalactic Astrophysics · Physics 2015-03-17 James G. Keehn , Cecilia Lunardini

The SNO+ experiment is the follow-up to the Sudbury Neutrino Observatory (SNO). The heavy water that was in SNO will be replaced with a liquid scintillator of linear alkylbenzene (plus fluor). SNO+ has many physics goals including detecting…

High Energy Physics - Experiment · Physics 2019-08-14 Mark C. Chen

Lithium chloride water solution is a good option for solar neutrino detection. The $\nu_e$ charged-current (CC) interaction cross-section on $\rm{{}^{7}Li}$ is evaluated with new B(GT) experimental measurements. The total CC interaction…

High Energy Physics - Experiment · Physics 2022-03-29 Wenhui Shao , Weiran Xu , Ye Liang , Wentai Luo , Tong Xu , Ming Qi , Jialiang Zhang , Benda Xu , Zhe Wang , Shaomin Chen

We report the results of a neutrino search in Super-Kamiokande for coincident signals with the first detected gravitational wave produced by a binary neutron star merger, GW170817, which was followed by a short gamma-ray burst, GRB170817A,…

High Energy Astrophysical Phenomena · Physics 2018-04-25 K. Abe , C. Bronner , Y. Hayato , M. Ikeda , K. Iyogi , J. Kameda , Y. Kato , Y. Kishimoto , Ll. Marti , M. Miura , S. Moriyama , M. Nakahata , Y. Nakajima , Y. Nakano , S. Nakayama , A. Orii , G. Pronost , H. Sekiya , M. Shiozawa , Y. Sonoda , A. Takeda , A. Takenaka , H. Tanaka , S. Tasaka , T. Yano , R. Akutsu , T. Kajita , Y. Nishimura , K. Okumura , K. M. Tsui , L. Labarga , P. Fernandez , F. d. M. Blaszczyk , C. Kachulis , E. Kearns , J. L. Raaf , J. L. Stone , L. R. Sulak , S. Berkman , S. Tobayama , J. Bian , M. Elnimr , W. R. Kropp , S. Locke , S. Mine , P. Weatherly , M. B. Smy , H. W. Sobel , V. Takhistov , K. S. Ganezer , J. Hill , J. Y. Kim , I. T. Lim , R. G. Park , Z. Li , E. O'Sullivan , K. Scholberg , C. W. Walter , M. Gonin , J. Imber , Th. A. Mueller , T. Ishizuka , T. Nakamura , J. S. Jang , K. Choi , J. G. Learned , S. Matsuno , J. Amey , R. P. Litchfield , W. Y. Ma , Y. Uchida , M. O. Wascko , M. G. Catanesi , R. A. Intonti , E. Radicioni , G. De Rosa , A. Ali , G. Collazuol , L. Ludovici , S. Cao , M. Friend , T. Hasegawa , T. Ishida , T. Ishii , T. Kobayashi , T. Nakadaira , K. Nakamura , Y. Oyama , K. Sakashita , T. Sekiguchi , T. Tsukamoto , KE. Abe , M. Hasegawa , A. T. Suzuki , Y. Takeuchi , T. Hayashino , S. Hirota , M. Jiang , M. Mori , KE. Nakamura , T. Nakaya , R. A. Wendell , L. H. V. Anthony , N. McCauley , A. Pritchard , Y. Fukuda , Y. Itow , M. Murase , F. Muto , P. Mijakowski , K. Frankiewicz , C. K. Jung , X. Li , J. L. Palomino , G. Santucci , C. Viela , M. J. Wilking , C. Yanagisawa , D. Fukuda , H. Ishino , S. Ito , A. Kibayashi , Y. Koshio , H. Nagata , M. Sakuda , C. Xu , Y. Kuno , D. Wark , F. Di Lodovico , B. Richards , S. Molina Sedgwick , R. Tacik , S. B. Kim , A. Cole , L. Thompson , H. Okazawa , Y. Choi , K. Ito , K. Nishijima , M. Koshiba , Y. Suda , M. Yokoyama , R. G. Calland , M. Hartz , K. Martens , M. Murdoch , B. Quilain , C. Simpson , Y. Suzuki , M. R. Vagins , D. Hamabe , M. Kuze , Y. Okajima , T. Yoshida , M. Ishitsuka , J. F. Martin , C. M. Nantais , H. A. Tanaka , T. Towstego , A. Konaka , S. Chen , L. Wan , A. Minamino

The IceCube neutrino observatory uses $1\,\mathrm{km}^{3}$ of the natural Antarctic ice near the geographic South Pole as optical detection medium. When charged particles, such as particles produced in neutrino interactions, pass through…

High Energy Astrophysical Phenomena · Physics 2019-08-21 Anna Pollmann

New neutrino states \nu_b, sterile under the Standard Model interactions, can be coupled to baryons via the isoscalar vector currents that are much stronger than the Standard Model weak interactions. If some fraction of solar neutrinos…

High Energy Physics - Phenomenology · Physics 2015-03-19 Maxim Pospelov

We argue that analyzing the nu_e- and bar{nu_e}-induced CC reactions nu_e n --> e^- pi^0 p and bar{nu}_e p --> e^+ pi^0 n along with quasielastics may significantly enhance the sensitivity of a water Cherenkov detector to subleading…

High Energy Physics - Experiment · Physics 2007-05-23 A. Asratyan , V. Verebryusov

The detection of neutrinos from SN 1987A by the Kamiokande-II and Irvine-Michigan-Brookhaven detectors provided the first glimpse of core collapse in a supernova, complementing the optical observations and confirming our basic understanding…

Astrophysics · Physics 2008-11-26 Hasan Yuksel , John F. Beacom

In neutrino oscillation experiments, neutrino interactions at the detector are simulated using event generators which attempt to reflect our understanding of nuclear physics. We study the impact of different neutrino interactions and…

High Energy Physics - Phenomenology · Physics 2014-04-23 Pilar Coloma , Patrick Huber , Chun-Min Jen , Camillo Mariani

I address the question of what can be learned from the observation of the diffuse supernova neutrino flux in the precision phase, at next generation detectors of Megaton scale. An analytical study of the spectrum of the diffuse flux shows…

Astrophysics · Physics 2008-11-26 Cecilia Lunardini

We calculated the matter effect, including both the Earth and supernova, on the detection of neutrinos from type II supernovae at the proposed Daya Bay reactor neutrino experiment. It is found that apart from the dependence on the flip…

High Energy Physics - Phenomenology · Physics 2009-11-11 X. -H. Guo , Bing-Lin Young

We study theoretically interaction potentials and low energy collisions between different alkali atoms and alkali ions. Specifically, we consider systems like X + Y$^{+}$, where X(Y$^{+})$ is either Li(Cs$^+$) or Cs(Li$^+$), Na(Cs$^+$) or…

Atomic Physics · Physics 2016-09-13 Arpita Rakshit , Chedli Ghanmi , Hamid Berriche , Bimalendu Deb