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Related papers: Prospects in spectroscopy with Belle II

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The Belle II detector operating at the future upgrade to the KEKB accelerator will perform high-statistics precision investigations into the flavor sector of the Standard Model. As charged hadron identification is a vital element of the…

Instrumentation and Detectors · Physics 2019-08-14 K. Nishimura

Radio pulsars have been responsible for many astonishing astrophysical and fundamental physics breakthroughs since their discovery 50 years ago. In this review I will discuss many of the highlights, most of which were only possible because…

Instrumentation and Methods for Astrophysics · Physics 2018-08-22 Matthew Bailes

We measure the photon-energy spectrum in radiative bottom-meson ($B$) decays into inclusive final states involving a strange hadron and a photon. We use SuperKEKB electron-positron collisions corresponding to $189~\mathrm{fb}^{-1}$ of…

High Energy Physics - Experiment · Physics 2022-10-20 Belle II Collaboration , F. Abudinén , I. Adachi , K. Adamczyk , L. Aggarwal , P. Ahlburg , H. Ahmed , J. K. Ahn , H. Aihara , N. Akopov , A. Aloisio , F. Ameli , L. Andricek , N. Anh Ky , D. M. Asner , H. Atmacan , V. Aulchenko , T. Aushev , V. Aushev , T. Aziz , V. Babu , S. Bacher , H. Bae , S. Baehr , S. Bahinipati , A. M. Bakich , P. Bambade , Sw. Banerjee , S. Bansal , M. Barrett , G. Batignani , J. Baudot , M. Bauer , A. Baur , A. Beaubien , A. Beaulieu , J. Becker , P. K. Behera , J. V. Bennett , E. Bernieri , F. U. Bernlochner , V. Bertacchi , M. Bertemes , E. Bertholet , M. Bessner , S. Bettarini , V. Bhardwaj , B. Bhuyan , F. Bianchi , T. Bilka , S. Bilokin , D. Biswas , A. Bobrov , D. Bodrov , A. Bolz , A. Bondar , G. Bonvicini , A. Bozek , M. Bračko , P. Branchini , N. Braun , R. A. Briere , T. E. Browder , D. N. Brown , A. Budano , L. Burmistrov , S. Bussino , M. Campajola , L. Cao , G. Casarosa , C. Cecchi , D. Červenkov , M. -C. Chang , P. Chang , R. Cheaib , P. Cheema , V. Chekelian , C. Chen , Y. Q. Chen , Y. Q. Chen , Y. -T. Chen , B. G. Cheon , K. Chilikin , K. Chirapatpimol , H. -E. Cho , K. Cho , S. -J. Cho , S. -K. Choi , S. Choudhury , D. Cinabro , L. Corona , L. M. Cremaldi , S. Cunliffe , T. Czank , S. Das , N. Dash , F. Dattola , E. De La Cruz-Burelo , S. A. De La Motte , G. de Marino , G. De Nardo , M. De Nuccio , G. De Pietro , R. de Sangro , B. Deschamps , M. Destefanis , S. Dey , A. De Yta-Hernandez , R. Dhamija , A. Di Canto , F. Di Capua , S. Di Carlo , J. Dingfelder , Z. Doležal , I. Domínguez Jiménez , T. V. Dong , M. Dorigo , K. Dort , D. Dossett , S. Dreyer , S. Dubey , S. Duell , G. Dujany , P. Ecker , S. Eidelman , M. Eliachevitch , D. Epifanov , P. Feichtinger , T. Ferber , D. Ferlewicz , T. Fillinger , C. Finck , G. Finocchiaro , P. Fischer , K. Flood , A. Fodor , F. Forti , A. Frey , M. Friedl , B. G. Fulsom , M. Gabriel , A. Gabrielli , N. Gabyshev , E. Ganiev , M. Garcia-Hernandez , R. Garg , A. Garmash , V. Gaur , A. Gaz , U. Gebauer , A. Gellrich , J. Gemmler , T. Geßler , G. Ghevondyan , G. Giakoustidis , R. Giordano , A. Giri , A. Glazov , B. Gobbo , R. Godang , P. Goldenzweig , B. Golob , P. Gomis , G. Gong , P. Grace , W. Gradl , S. Granderath , E. Graziani , D. Greenwald , T. Gu , Y. Guan , K. Gudkova , J. Guilliams , C. Hadjivasiliou , S. Halder , K. Hara , T. Hara , O. Hartbrich , K. Hayasaka , H. Hayashii , S. Hazra , C. Hearty , M. T. Hedges , I. Heredia de la Cruz , M. Hernández Villanueva , A. Hershenhorn , T. Higuchi , E. C. Hill , H. Hirata , M. Hoek , M. Hohmann , S. Hollitt , T. Hotta , C. -L. Hsu , K. Huang , T. Humair , T. Iijima , K. Inami , G. Inguglia , N. Ipsita , J. Irakkathil Jabbar , A. Ishikawa , S. Ito , R. Itoh , M. Iwasaki , Y. Iwasaki , S. Iwata , P. Jackson , W. W. Jacobs , D. E. Jaffe , E. -J. Jang , M. Jeandron , H. B. Jeon , Q. P. Ji , S. Jia , Y. Jin , C. Joo , K. K. Joo , H. Junkerkalefeld , I. Kadenko , J. Kahn , H. Kakuno , M. Kaleta , A. B. Kaliyar , J. Kandra , K. H. Kang , S. Kang , P. Kapusta , R. Karl , G. Karyan , Y. Kato , H. Kawai , T. Kawasaki , C. Ketter , H. Kichimi , C. Kiesling , C. -H. Kim , D. Y. Kim , H. J. Kim , K. -H. Kim , K. Kim , S. -H. Kim , Y. -K. Kim , Y. Kim , T. D. Kimmel , H. Kindo , K. Kinoshita , C. Kleinwort , B. Knysh , P. Kodyš , T. Koga , S. Kohani , K. Kojima , I. Komarov , T. Konno , A. Korobov , S. Korpar , N. Kovalchuk , E. Kovalenko , R. Kowalewski , T. M. G. Kraetzschmar , F. Krinner , P. Križan , R. Kroeger , J. F. Krohn , P. Krokovny , H. Krüger , W. Kuehn , T. Kuhr , J. Kumar , M. Kumar , R. Kumar , K. Kumara , T. Kumita , T. Kunigo , M. Künzel , S. Kurz , A. Kuzmin , P. Kvasnička , Y. -J. Kwon , S. Lacaprara , Y. -T. Lai , C. La Licata , K. Lalwani , T. Lam , L. Lanceri , J. S. Lange , M. Laurenza , K. Lautenbach , P. J. Laycock , R. Leboucher , F. R. Le Diberder , I. -S. Lee , S. C. Lee , P. Leitl , D. Levit , P. M. Lewis , C. Li , L. K. Li , S. X. Li , Y. B. Li , J. Libby , K. Lieret , J. Lin , Z. Liptak , Q. Y. Liu , Z. A. Liu , D. Liventsev , S. Longo , A. Loos , A. Lozar , P. Lu , T. Lueck , F. Luetticke , T. Luo , C. Lyu , C. MacQueen , M. Maggiora , R. Maiti , S. Maity , R. Manfredi , E. Manoni , A. Manthei , S. Marcello , C. Marinas , L. Martel , A. Martini , T. Martinov , L. Massaccesi , M. Masuda , T. Matsuda , K. Matsuoka , D. Matvienko , J. A. McKenna , J. McNeil , F. Meggendorfer , F. Meier , M. Merola , F. Metzner , M. Milesi , C. Miller , K. Miyabayashi , H. Miyake , H. Miyata , R. Mizuk , K. Azmi , G. B. Mohanty , N. Molina-Gonzalez , S. Moneta , H. Moon , T. Moon , J. A. Mora Grimaldo , T. Morii , H. -G. Moser , M. Mrvar , F. J. Müller , Th. Muller , G. Muroyama , C. Murphy , R. Mussa , I. Nakamura , K. R. Nakamura , E. Nakano , M. Nakao , H. Nakayama , H. Nakazawa , A. Narimani Charan , M. Naruki , Z. Natkaniec , A. Natochii , L. Nayak , M. Nayak , G. Nazaryan , D. Neverov , C. Niebuhr , M. Niiyama , J. Ninkovic , N. K. Nisar , S. Nishida , K. Nishimura , M. H. A. Nouxman , K. Ogawa , S. Ogawa , S. L. Olsen , Y. Onishchuk , H. Ono , Y. Onuki , P. Oskin , F. Otani , E. R. Oxford , H. Ozaki , P. Pakhlov , G. Pakhlova , A. Paladino , T. Pang , A. Panta , E. Paoloni , S. Pardi , K. Parham , H. Park , S. -H. Park , B. Paschen , A. Passeri , A. Pathak , S. Patra , S. Paul , T. K. Pedlar , I. Peruzzi , R. Peschke , R. Pestotnik , F. Pham , M. Piccolo , L. E. Piilonen , G. Pinna Angioni , P. L. M. Podesta-Lerma , T. Podobnik , S. Pokharel , L. Polat , V. Popov , C. Praz , S. Prell , E. Prencipe , M. T. Prim , M. V. Purohit , H. Purwar , N. Rad , P. Rados , S. Raiz , A. Ramirez Morales , R. Rasheed , N. Rauls , M. Reif , S. Reiter , M. Remnev , I. Ripp-Baudot , M. Ritter , M. Ritzert , G. Rizzo , L. B. Rizzuto , M. Röhrken , S. H. Robertson , D. Rodríguez Pérez , J. M. Roney , C. Rosenfeld , A. Rostomyan , N. Rout , M. Rozanska , G. Russo , D. Sahoo , Y. Sakai , D. A. Sanders , S. Sandilya , A. Sangal , L. Santelj , P. Sartori , Y. Sato , V. Savinov , B. Scavino , M. Schnepf , M. Schram , H. Schreeck , J. Schueler , C. Schwanda , A. J. Schwartz , B. Schwenker , M. Schwickardi , Y. Seino , A. Selce , K. Senyo , I. S. Seong , J. Serrano , M. E. Sevior , C. Sfienti , V. Shebalin , C. P. Shen , H. Shibuya , T. Shillington , T. Shimasaki , J. -G. Shiu , B. Shwartz , A. Sibidanov , F. Simon , J. B. Singh , S. Skambraks , J. Skorupa , K. Smith , R. J. Sobie , A. Soffer , A. Sokolov , Y. Soloviev , E. Solovieva , S. Spataro , B. Spruck , M. Starič , S. Stefkova , Z. S. Stottler , R. Stroili , J. Strube , J. Stypula , Y. Sue , R. Sugiura , M. Sumihama , K. Sumisawa , T. Sumiyoshi , W. Sutcliffe , S. Y. Suzuki , H. Svidras , M. Tabata , K. Tackmann , M. Takahashi , M. Takizawa , U. Tamponi , S. Tanaka , K. Tanida , H. Tanigawa , N. Taniguchi , Y. Tao , P. Taras , F. Tenchini , R. Tiwary , D. Tonelli , E. Torassa , N. Toutounji , K. Trabelsi , I. Tsaklidis , T. Tsuboyama , N. Tsuzuki , M. Uchida , I. Ueda , S. Uehara , Y. Uematsu , T. Ueno , T. Uglov , K. Unger , Y. Unno , K. Uno , S. Uno , P. Urquijo , Y. Ushiroda , Y. V. Usov , S. E. Vahsen , R. van Tonder , G. S. Varner , K. E. Varvell , A. Vinokurova , L. Vitale , V. Vobbilisetti , V. Vorobyev , A. Vossen , B. Wach , E. Waheed , H. M. Wakeling , K. Wan , W. Wan Abdullah , B. Wang , C. H. Wang , E. Wang , M. -Z. Wang , X. L. Wang , A. Warburton , M. Watanabe , S. Watanuki , J. Webb , S. Wehle , M. Welsch , C. Wessel , J. Wiechczynski , P. Wieduwilt , H. Windel , E. Won , L. J. Wu , X. P. Xu , B. D. Yabsley , S. Yamada , W. Yan , S. B. Yang , H. Ye , J. Yelton , J. H. Yin , M. Yonenaga , Y. M. Yook , K. Yoshihara , T. Yoshinobu , C. Z. Yuan , Y. Yusa , L. Zani , Y. Zhai , J. Z. Zhang , Y. Zhang , Y. Zhang , Z. Zhang , V. Zhilich , J. Zhou , Q. D. Zhou , X. Y. Zhou , V. I. Zhukova , V. Zhulanov , R. Žlebčík

New results on hadron physics from the Belle experiment are presented

High Energy Physics - Experiment · Physics 2019-08-14 P. Krokovny

Optical spectroscopy is an important and widely used technique, for instance, to characterize new materials and to identify unknown compounds. Spectra are typically reported as a function of the wavelength of light, yet the information…

Optics · Physics 2026-05-06 Erik F. Woering , Richard Hildner

Science opportunities and recommendations concerning optical/infrared polarimetry for the upcoming decade in the fields of stars and stellar evolution. Community-based White Paper to Astro2010 in response to the call for such papers.

Type II supernovae (SNe II), which show abundant hydrogen in their spectra, belong to a class of SNe with diverse observed properties. It is commonly accepted that SNe II are produced by core collapse and explosion of massive stars.…

High Energy Astrophysical Phenomena · Physics 2024-01-12 Han Lin , Jujia Zhang , Xinghan Zhang

A family of local models containing two angles as hidden variables is defined for experiments measuring polarization correlation of optical photons. Searching for the best model of the family, that is giving predictions most close to…

Quantum Physics · Physics 2021-06-16 Emilio Santos

The large data sample recorded with the Belle detector at the Y(5S) energy provides a unique opportunity to study the poorly-known $\bs$ meson. Two analyses, performed with a data sample representing an integrated luminosity of 121 /fb, are…

High Energy Physics - Experiment · Physics 2019-08-13 Remi Louvot

The Belle II experiment currently under construction at the $e^+e^-$-collider SuperKEKB in Japan is designed to explore new physics beyond the standard model with an approximately 50 times larger data sample compared to its predecessor. The…

Instrumentation and Detectors · Physics 2017-03-21 H. Ye , C. Neibuhr , R. Stever , K. Gadow , C. Camien

Deep learning and other big data technologies have over time become very powerful and accurate. There are algorithms and models developed that have near human accuracy in their task. In health care, the amount of data available is massive…

Computers and Society · Computer Science 2019-09-09 Dinesh Samuel Sathia Raj , Vijayakumar V , Bharat Rawal , Longzhi Yang

Information theory is rapidly approaching its 70th birthday. What are promising future directions for research in information theory? Where will information theory be having the most impact in 10-20 years? What new and emerging areas are…

Stellar abundances of beryllium are useful in different areas of astrophysics, including studies of the Galactic chemical evolution, of stellar evolution, and of the formation of globular clusters. Determining Be abundances in stars is,…

Solar and Stellar Astrophysics · Physics 2015-06-19 R. Smiljanic

The first observation of $\mathcal{B}\left(B^+\rightarrow K^+\nu\nu\right)$ by the Belle II experiment lies almost $3\sigma$ away from the Standard Model expectation. In this letter we study this result in the SMEFT, extended by a light…

High Energy Physics - Phenomenology · Physics 2024-08-28 L. P. S. Leal , S. Rosauro-Alcaraz

The Belle and Belle II experiments have collected an 1.6 ab$^{-1}$ sample of $e^+e^-$ collision data at center-of-mass energies near the $\Upsilon(nS)$ resonances. In particular, the Belle II experiment collected a 19.2 fb$^{-1}$ sample of…

High Energy Physics - Experiment · Physics 2026-01-27 Martin Bartl for the Belle , Belle-II Collaborations

We report preliminary measurements of the first (mean) and second moment (variance) of the inclusive photon energy spectrum in $B\to X_s\gamma$ decays, for threshold values of the photon energy in the range 1.8--2.3 GeV as measured in the…

High Energy Physics - Experiment · Physics 2012-08-27 Belle Collaboration

Large numbers of $\tau$ leptons are produced at Belle II. These could potentially decay into sterile neutrinos that, for the mass range under consideration, are typically long-lived, leading to displaced-vertex signatures. Here, we study a…

High Energy Physics - Phenomenology · Physics 2022-08-31 Guanghui Zhou , Julian Y. Günther , Zeren Simon Wang , Jordy de Vries , Herbi K. Dreiner

We report the recent results of a search for the decay B- --> tau- anti-nu_tau, observations of new resonances X, Y and Z, and the first results from Upsilon(5S) data collected with the Belle detector at KEKB e+e- collider.

High Energy Physics - Experiment · Physics 2007-05-23 T. A. -Kh. Aushev

The measurements of COBE/FIRAS have shown that the CMB spectrum is extremely close to a perfect blackbody. There are, however, a number of processes in the early Universe that should create spectral distortions at a level which is within…

Cosmology and Nongalactic Astrophysics · Physics 2014-05-28 Jens Chluba

The next decade of survey astronomy has the potential to transform our knowledge of variable stars. Stellar variability underpins our knowledge of the cosmological distance ladder, and provides direct tests of stellar formation and…