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Related papers: Probing the Neutrino Mass Hierarchy beyond $\Lambd…

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It is well known that the neutrino mass matrix contains more parameters than experimentalists can hope to measure in the foreseeable future even if we impose CP invariance. Thus, various authors have proposed ansatzes to restrict the form…

High Energy Physics - Phenomenology · Physics 2014-11-17 X. -G. He , A. Zee

Assuming lepton number conservation, hermiticity of the neutrino mass matrix and $\nu_{\mu} - \nu_{\tau}$ exchange symmetry, we show that we can determine the neutrino mass matrix completely from the existing data. Comparing with the…

High Energy Physics - Phenomenology · Physics 2014-05-26 Shreyashi Chakdar , Kirtiman Ghosh , S. Nandi

Recent results from DESI combined with cosmic microwave background data give the tightest constraints on the sum of neutrino masses to date. However, these analyses approximate the neutrino mass hierarchy by three degenerate-mass (DM)…

Cosmology and Nongalactic Astrophysics · Physics 2025-04-11 Laura Herold , Marc Kamionkowski

Recent DESI results indicate a strong preference for dynamical dark energy (DE) when baryon acoustic oscillation (BAO) measurements are combined with supernovae (SNe) and cosmic microwave background (CMB) data using the…

Cosmology and Nongalactic Astrophysics · Physics 2026-01-26 Shubham Barua , Shantanu Desai

Current measurements of the low and high redshift Universe are in tension if we restrict ourselves to the standard six parameter model of flat $\Lambda$CDM. This tension has two parts. First, the Planck satellite data suggest a higher…

Cosmology and Nongalactic Astrophysics · Physics 2014-02-10 Mark Wyman , Douglas H. Rudd , R. Ali Vanderveld , Wayne Hu

We report on measurements of neutrino oscillation using data from the T2K long-baseline neutrino experiment collected between 2010 and 2013. In an analysis of muon neutrino disappearance alone, we find the following estimates and 68%…

High Energy Physics - Experiment · Physics 2015-05-06 T2K Collaboration , K. Abe , J. Adam , H. Aihara , T. Akiri , C. Andreopoulos , S. Aoki , A. Ariga , S. Assylbekov , D. Autiero , M. Barbi , G. J. Barker , G. Barr , P. Bartet-Friburg , M. Bass , M. Batkiewicz , F. Bay , V. Berardi , B. E. Berger , S. Berkman , S. Bhadra , F. d. M. Blaszczyk , A. Blondel , S. Bolognesi , S. Bordoni , S. B. Boyd , D. Brailsford , A. Bravar , C. Bronner , N. Buchanan , R. G. Calland , J. Caravaca Rodríguez , S. L. Cartwright , R. Castillo , M. G. Catanesi , A. Cervera , D. Cherdack , N. Chikuma , G. Christodoulou , A. Clifton , J. Coleman , S. J. Coleman , G. Collazuol , K. Connolly , L. Cremonesi , A. Dabrowska , I. Danko , R. Das , S. Davis , P. de Perio , G. De Rosa , T. Dealtry , S. R. Dennis , C. Densham , D. Dewhurst , F. Di Lodovico , S. Di Luise , S. Dolan , O. Drapier , T. Duboyski , K. Duffy , J. Dumarchez , S. Dytman , M. Dziewiecki , S. Emery-Schrenk , A. Ereditato , L. Escudero , T. Feusels , A. J. Finch , G. A. Fiorentini , M. Friend , Y. Fujii , Y. Fukuda , A. P. Furmanski , V. Galymov , A. Garcia , S. Giffin , C. Giganti , K. Gilje , D. Goeldi , T. Golan , M. Gonin , N. Grant , D. Gudin , D. R. Hadley , L. Haegel , A. Haesler , M. D. Haigh , P. Hamilton , D. Hansen , T. Hara , M. Hartz , T. Hasegawa , N. C. Hastings , T. Hayashino , Y. Hayato , C. Hearty , R. L. Helmer , M. Hierholzer , J. Hignight , A. Hillairet , A. Himmel , T. Hiraki , S. Hirota , J. Holeczek , S. Horikawa , F. Hosomi , K. Huang , A. K. Ichikawa , K. Ieki , M. Ieva , M. Ikeda , J. Imber , J. Insler , T. J. Irvine , T. Ishida , T. Ishii , E. Iwai , K. Iwamoto , K. Iyogi , A. Izmaylov , A. Jacob , B. Jamieson , M. Jiang , S. Johnson , J. H. Jo , P. Jonsson , C. K. Jung , M. Kabirnezhad , A. C. Kaboth , T. Kajita , H. Kakuno , J. Kameda , Y. Kanazawa , D. Karlen , I. Karpikov , T. Katori , E. Kearns , M. Khabibullin , A. Khotjantsev , D. Kielczewska , T. Kikawa , A. Kilinski , J. Kim , S. King , J. Kisiel , P. Kitching , T. Kobayashi , L. Koch , T. Koga , A. Kolaceke , A. Konaka , L. L. Kormos , A. Korzenev , Y. Koshio , W. Kropp , H. Kubo , Y. Kudenko , R. Kurjata , T. Kutter , J. Lagoda , I. Lamont , E. Larkin , M. Laveder , M. Lawe , M. Lazos , T. Lindner , C. Lister , R. P. Litchfield , A. Longhin , J. P. Lopez , L. Ludovici , L. Magaletti , K. Mahn , M. Malek , S. Manly , A. D. Marino , J. Marteau , J. F. Martin , P. Martins , S. Martynenko , T. Maruyama , V. Matveev , K. Mavrokoridis , E. Mazzucato , M. McCarthy , N. McCauley , K. S. McFarland , C. McGrew , A. Mefodiev , C. Metelko , M. Mezzetto , P. Mijakowski , C. A. Miller , A. Minamino , O. Mineev , A. Missert , M. Miura , S. Moriyama , Th. A. Mueller , A. Murakami , M. Murdoch , S. Murphy , J. Myslik , T. Nakadaira , M. Nakahata , K. G. Nakamura , K. Nakamura , S. Nakayama , T. Nakaya , K. Nakayoshi , C. Nantais , C. Nielsen , M. Nirkko , K. Nishikawa , Y. Nishimura , J. Nowak , H. M. O'Keeffe , R. Ohta , K. Okumura , T. Okusawa , W. Oryszczak , S. M. Oser , T. Ovsyannikova , R. A. Owen , Y. Oyama , V. Palladino , J. L. Palomino , V. Paolone , D. Payne , O. Perevozchikov , J. D. Perkin , Y. Petrov , L. Pickard , E. S. Pinzon Guerra , C. Pistillo , P. Plonski , E. Poplawska , B. Popov , M. Posiadala-Zezula , J. -M. Poutissou , R. Poutissou , P. Przewlocki , B. Quilain , E. Radicioni , P. N. Ratoff , M. Ravonel , M. A. M. Rayner , A. Redij , M. Reeves , E. Reinherz-Aronis , C. Riccio , P. A. Rodrigues , P. Rojas , E. Rondio , S. Roth , A. Rubbia , D. Ruterbories , A. Rychter , R. Sacco , K. Sakashita , F. Sánchez , F. Sato , E. Scantamburlo , K. Scholberg , S. Schoppmann , J. Schwehr , M. Scott , Y. Seiya , T. Sekiguchi , H. Sekiya , D. Sgalaberna , R. Shah , F. Shaker , D. Shaw , M. Shiozawa , S. Short , Y. Shustrov , P. Sinclair , B. Smith , M. Smy , J. T. Sobczyk , H. Sobel , M. Sorel , L. Southwell , P. Stamoulis , J. Steinmann , B. Still , Y. Suda , A. Suzuki , K. Suzuki , S. Y. Suzuki , Y. Suzuki , R. Tacik , M. Tada , S. Takahashi , A. Takeda , Y. Takeuchi , H. K. Tanaka , H. A. Tanaka , M. M. Tanaka , D. Terhorst , R. Terri , L. F. Thompson , A. Thorley , S. Tobayama , W. Toki , T. Tomura , Y. Totsuka , C. Touramanis , T. Tsukamoto , M. Tzanov , Y. Uchida , A. Vacheret , M. Vagins , G. Vasseur , T. Wachala , K. Wakamatsu , C. W. Walter , D. Wark , W. Warzycha , M. O. Wascko , A. Weber , R. Wendell , R. J. Wilkes , M. J. Wilking , C. Wilkinson , Z. Williamson , J. R. Wilson , R. J. Wilson , T. Wongjirad , Y. Yamada , K. Yamamoto , C. Yanagisawa , T. Yano , S. Yen , N. Yershov , M. Yokoyama , K. Yoshida , T. Yuan , M. Yu , A. Zalewska , J. Zalipska , L. Zambelli , K. Zaremba , M. Ziembicki , E. D. Zimmerman , M. Zito , J. Żmuda

The extraction of the neutrino mass ordering is one of the major challenges in particle physics and cosmology, not only for its implications for a fundamental theory of mass generation in nature, but also for its decisive role in the scale…

Within the standard three-neutrino framework, the absolute neutrino masses and their ordering (either normal, NO, or inverted, IO) are currently unknown. However, the combination of current data coming from oscillation experiments,…

High Energy Physics - Phenomenology · Physics 2017-06-07 Francesco Capozzi , Eleonora Di Valentino , Eligio Lisi , Antonio Marrone , Alessandro Melchiorri , Antonio Palazzo

Based on the independent measurements on neutrino mass splitting $|\Delta m^2_{\mu\mu}|$, $|\Delta m^2_{ee}|$, $\Delta m^2_{21}$, and recent measurements by the T2K Collaboration, we carry out a simple fitting analysis on $\Delta m^2_{32}$…

High Energy Physics - Phenomenology · Physics 2014-07-16 Yijia Zhang , Bo-Qiang Ma

We perform a global analysis of cosmological observables in generalized cosmologies which depart from $\Lambda$CDM models by allowing non-vanishing curvature $\Omega_k\neq 0$, dark energy with equation of state with $\omega\neq -1$, the…

High Energy Physics - Phenomenology · Physics 2011-06-17 M. C. Gonzalez-Garcia , Michele Maltoni , Jordi Salvado

We inspect recently updated neutrino oscillation data -- specifically coming from the Tokai to Kamioka and NuMI Off-axis $\nu_e$ Appearance experiments -- and how they are analyzed to determine whether the neutrino mass ordering is normal…

High Energy Physics - Phenomenology · Physics 2021-01-12 Kevin J. Kelly , Pedro A. N. Machado , Stephen J. Parke , Yuber F. Perez-Gonzalez , Renata Zukanovich Funchal

In the current 3nu paradigm, flavor oscillations probe 3 mixing angles (theta_12, theta_23, theta_13), one CP phase delta, and two squared mass differences delta m^2>0 and Delta m^2, where sign(Delta m^2)=+ (-) for normal (inverted)…

High Energy Physics - Phenomenology · Physics 2021-09-29 Francesco Capozzi , Eleonora Di Valentino , Eligio Lisi , Antonio Marrone , Alessandro Melchiorri , Antonio Palazzo

We discuss the role of lightest neutrino mass (m_0) in the neutrino mass matrix, defined in a flavor basis, through a bottom-up approach using the current neutrino oscillation data. We find that if m_0 < 10^{-3} eV, then the deviation…

High Energy Physics - Phenomenology · Physics 2015-06-15 Rupak Dutta , Upender Ch , Anjan K. Giri , Narendra Sahu

Four zero neutrino Yukawa textures in a specified weak basis, combined with $\mu\tau$ symmetry and type-I seesaw, yield a highly constrained and predictive scheme. Two alternately viable $3\times3$ light neutrino Majorana mass matrices…

High Energy Physics - Phenomenology · Physics 2015-05-27 Biswajit Adhikary , Ambar Ghosal , Probir Roy

Early JWST observations reveal an unexpectedly abundant population of high-redshift candidate massive galaxies at $z \gtrsim 7$, and recent DESI measurements show a preference for dynamical dark energy, which together present a significant…

Cosmology and Nongalactic Astrophysics · Physics 2025-12-18 Sheng-Han Zhou , Tian-Nuo Li , Guo-Hong Du , Jun-Qian Jiang , Jing-Fei Zhang , Xin Zhang

We study a simple extension of the Standard Model supplemented by an electroweak triplet scalar field to accommodate small neutrino masses by the type-II seesaw mechanism, while an additional singlet scalar field can play the role of cold…

High Energy Physics - Phenomenology · Physics 2014-05-07 P. S. Bhupal Dev , Dilip Kumar Ghosh , Nobuchika Okada , Ipsita Saha

The sum of the masses of the three neutrino mass eigenstates is now constrained both from above and below, and lies between 55 and 6900 meV. The lower limit is set by neutrino oscillations and the fact that masses are non-negative. The…

Nuclear Experiment · Physics 2009-07-24 R. G. Hamish Robertson

We present an analysis of normal and inverted hierarchical neutrino mass models within the framework of tri-bi-maximal (TBM) mixing. Considering the neutrinos to be quasi-degenerate (QDN), we study two different neutrino mass models with…

High Energy Physics - Phenomenology · Physics 2012-11-07 Mrinal Kumar Das , Debasish Borah , Rinku Mishra

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 present an updated global fit of neutrino oscillation data in the simplest three-neutrino framework. In the present study we include up-to-date analyses from a number of experiments. Concerning the atmospheric and solar sectors, we give…

High Energy Physics - Phenomenology · Physics 2021-02-12 P. F. de Salas , D. V. Forero , S. Gariazzo , P. Martínez-Miravé , O. Mena , C. A. Ternes , M. Tórtola , J. W. F. Valle