English
Related papers

Related papers: Supernova 1987A did not test the neutrino mass hie…

200 papers

We discuss the flavor conversion of supernova neutrinos in the three-flavor mixing scheme of neutrinos. We point out that by neutrino observation from supernova one can discriminate the inverted hierarchy of neutrino masses from the normal…

High Energy Physics - Phenomenology · Physics 2009-10-31 Hisakazu Minakata , Hiroshi Nunokawa

Detection of 5 events by the Liquid Scintillation Detector (LSD) on February, 23, 1987 was recently interpreted as a detection of the electron neutrino flux from the first stage of the two-stage Supernova collapse. We show that, if neutrino…

High Energy Physics - Phenomenology · Physics 2007-05-23 Oleg Lychkovskiy

The only experimentally observed phenomenon that lies outside the standard model of the electroweak interaction is neutrino oscillations. A way to try to unify the extensive neutrino oscillation data is to add a phenomenological mass term…

Nuclear Theory · Physics 2017-08-23 D. J. Ernst , B. K. Cogswell , H. R. Burroughs , J. Escamilla-Roa , D. C. Latimer

We present a search for non-zero theta_{13} and deviations of sin^2 theta_{23} from 0.5 in the oscillations of atmospheric neutrino data from Super-Kamiokande -I, -II, and -III. No distortions of the neutrino flux consistent with non-zero…

High Energy Physics - Experiment · Physics 2012-08-27 Kamiokande Collaboration , R. Wendell , C. Ishihara , K. Abe , Y. Hayato , T. Iida , M. Ikeda , K. Iyogi , J. Kameda , K. Kobayashi , Y. Koshio , Y. Kozuma , M. Miura , S. Moriyama , M. Nakahata , S. Nakayama , Y. Obayashi , H. Ogawa , H. Sekiya , M. Shiozawa , Y. Suzuki , A. Takeda , Y. Takenaga , Y. Takeuchi , K. Ueno , K. Ueshima , H. Watanabe , S. Yamada , T. Yokozawa , S. Hazama , H. Kaji , T. Kajita , K. Kaneyuki , T. McLachlan , K. Okumura , Y. Shimizu , N. Tanimoto , M. R. Vagins , F. Dufour , E. Kearns , M. Litos , J. L. Raaf , J. L. Stone , L. R. Sulak , W. Wang , M. Goldhaber , K. Bays , D. Casper , J. P. Cravens , W. R. Kropp , S. Mine , C. Regis , M. B. Smy , H. W. Sobel , K. S. Ganezer , J. Hill , W. E. Keig , J. S. Jang , J. Y. Kim , I. T. Lim , J. Albert , M. Fechner , K. Scholberg , C. W. Walter , S. Tasaka , J. G. Learned , S. Matsuno , Y. Watanabe , T. Hasegawa , T. Ishida , T. Ishii , T. Kobayashi , T. Nakadaira , K. Nakamura , K. Nishikawa , H. Nishino , Y. Oyama , K. Sakashita , T. Sekiguchi , T. Tsukamoto , A. T. Suzuki , A. Minamino , T. Nakaya , Y. Fukuda , Y. Itow , G. Mitsuka , T. Tanaka , C. K. Jung , G. Lopez , C. McGrew , C. Yanagisawa , N. Tamura , H. Ishino , A. Kibayashi , S. Mino , T. Mori , M. Sakuda , H. Toyota , Y. Kuno , M. Yoshida , S. B. Kim , B. S. Yang , T. Ishizuka , H. Okazawa , Y. Choi , K. Nishijima , Y. Yokosawa , M. Koshiba , M. Yokoyama , Y. Totsuka , S. Chen , Y. Heng , Z. Yang , H. Zhang , D. Kielczewska , P. Mijakowski , K. Connolly , M. Dziomba , E. Thrane , R. J. Wilkes

We investigate the feasibility of probing the neutrino mass hierarchy and the mixing angle $\phi_{13}$ with the neutrino burst from a future supernova. An inverse power-law density $\rho \sim r^{n} $ with varying $n$ is adopted in the…

High Energy Physics - Phenomenology · Physics 2007-05-23 Shao-Hsuan Chiu , T. K. Kuo

Recent works combining neutrino oscillation and cosmological data to determine the neutrino hierarchy found a range of odds in favour of the normal hierarchy. These results arise from differing approaches to incorporating prior knowledge…

Cosmology and Nongalactic Astrophysics · Physics 2020-04-15 Constance Mahony , Boris Leistedt , Hiranya V. Peiris , Jonathan Braden , Benjamin Joachimi , Andreas Korn , Linda Cremonesi , Ryan Nichol

We reconsider the impact of $\bar\nu_e \leftrightarrow \bar\nu_{\mu,\tau}$ neutrino oscillations on the observed $\bar\nu_e$ signal of supernova SN 1987A. Performing a maximum-likelihood analysis using as fit parameters the released binding…

High Energy Physics - Phenomenology · Physics 2009-10-31 M. Kachelriess , R. Tomas , J. W. F. Valle

We introduce three right-handed Majorana neutrinos and combine the type-I seesaw and inert doublet mechanisms. The resultant (active) neutrino mass matrix is divided into rank=1 and =2 parts with different energy scales. The different…

High Energy Physics - Phenomenology · Physics 2015-05-27 Takeshi Araki

We investigate neutrino non-radiative two-body decay in vacuum, in relation to SN1987A. In a full $3\nu$ decay framework, we perform a detailed likelihood analysis of the 24 neutrino events from SN1987A observed by Kamiokande-II, IMB, and…

High Energy Physics - Phenomenology · Physics 2023-11-06 Pilar Iváñez-Ballesteros , M. Cristina Volpe

Motivated by recent results from neutrino experiments, we study the neutrino masses and mixing in the framework of a SUSY $SU(5)\times \mathbb{A}_{4} $ model. The hybrid of Type I and Type II seesaw mechanisms leads to the nonzero value of…

High Energy Physics - Phenomenology · Physics 2018-07-11 R. Ahl Laamara , M. A. Loualidi , M. Miskaoui , E. H. Saidi

In a new application of the discrete non-Abelian symmetry A_4 using the canonical seesaw mechanism, a three-parameter form of the neutrino mass matrix is derived. It predicts the following mixing angles for neutrino oscillations:…

High Energy Physics - Phenomenology · Physics 2009-11-11 Ernest Ma

An attempt is made to explore the possibility for deviations of solar mixing angle ($\theta_{12}$) from tri-bimaximal mixings, without sacrificing the predictions of maximal atmospheric mixing angle ($\theta_{23}=\pi/4$) and zero reactor…

High Energy Physics - Phenomenology · Physics 2008-11-26 N. Nimai Singh , Monisa Rajkhowa , Abhijit Borah

Collective neutrino flavor transformations deep inside a supernova are sensitive to the neutrino mass hierarchy even at extremely small values of theta(13). Exploiting this effect, we show that comparison of the antineutrino signals from a…

High Energy Physics - Phenomenology · Physics 2008-11-26 Basudeb Dasgupta , Amol Dighe , Alessandro Mirizzi

We examine the possibility of determining the neutrino mass hierarchy in the limit \theta_{13} = 0 using atmospheric neutrinos as the source. In this limit, in which \theta_{13} driven matter effects are absent, independent measurements of…

High Energy Physics - Phenomenology · Physics 2014-11-18 Raj Gandhi , Pomita Ghoshal , Srubabati Goswami , S Uma Sankar

We investigate the prospects for scenarios with vanishing determinant neutrino mass matrices and vanishing $\theta_{13}$ mixing angle. Normal and inverse mass hierarchies are considered separately. For normal hierarchy it is found that…

High Energy Physics - Phenomenology · Physics 2013-05-29 Bhag C. Chauhan , Joao Pulido , Marco Picariello

The recent observational data supports the deviation from Tri-bimaximal (TBM) mixings. Different neutrino mass models suggest the interdependency among the observational parameters involving the mixing angles. On phenomenological ground we…

High Energy Physics - Phenomenology · Physics 2015-06-11 Subhankar Roy , N. Nimai Singh

The recent measurement of a non-zero neutrino mixing angle $\theta_{13}$ requires a modification of the tri-bimaximal mixing pattern that predicts a zero value for it. We propose a new neutrino mixing pattern based on a spontaneously-broken…

High Energy Physics - Phenomenology · Physics 2013-05-30 Y. H. Ahn , Seungwon Baek , Paolo Gondolo

It is proposed that light neutrinos form a triplet in a global SU(3) flavor symmetry. Within this framework, a symmetry principle predicts sin^2 theta_{23}=0.5 and gives the so called inverted neutrino mass hierarchy, theta _{13}=0 and a…

High Energy Physics - Phenomenology · Physics 2007-05-23 Riazuddin

We study the effects of neutrino oscillation on supernova neutrino in the case of the inverted mass hierarchy ($m_{3} \ll m_{1} < m_{2}$) as well as the normal mass hierarchy ($m_{1} < m_{2} \ll m_{3}$). Numerical analysis using a realistic…

High Energy Physics - Phenomenology · Physics 2009-11-07 K. Takahashi , K. Sato

We examine a phenomenon recently predicted by numerical simulations of supernova neutrino flavor evolution: the swapping of supernova $\nu_e$ and $\nu_{\mu,\tau}$ energy spectra below (above) energy $\EC$ for the normal (inverted) neutrino…

Astrophysics · Physics 2008-11-26 Huaiyu Duan , George M. Fuller , J. Carlson , Yong-Zhong Qian
‹ Prev 1 2 3 10 Next ›