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CERN Document Server 16 のレコードが見つかりました。  1 - 10次  レコードへジャンプ: 検索にかかった時間: 0.62 秒 
1.
Working Group Report : Neutrino and Astroparticle Physics / Goswami, S ; Rangarajan, R ; Agashe, K ; Bandyopadhyay, A ; Bhattacharya, K K ; Brahmachari, B ; Burgess, C ; Chun, E J ; Choudhury, D ; Das-Prasanta, Kumar et al.
This is the report of neutrino and astroparticle physics working group at WHEPP-8. We present the discussions carried out during the workshop on selected topics in the above fields and also indicate progress made subsequently. [...]
hep-ph/0409225.- 2004 - 14 p. - Published in : Pramana - J. Phys. 63 (2004) 1391-1405 External link: Fulltext
In : 8th Workshop On High Energy Physics Phenomenology, Mumbai, India, 5 - 16 Jan 2004, pp.1391-1405
2.
CKM elements from tree-level b decays and lifetimes / Battaglia, Marco ; Barberio, E (convener) ; Lellouch, L P (convener) ; Schubert, Klaus R (convener) ; Artuso, M ; Bauer, C ; Becirevic, D ; Beneke, Martin ; Bigi, Ikaros I ; Brandt, T B et al.
CERN, 2003 Published version from CERN: PDF;
In : The CKM matrix and the unitarity triangle. Workshop, CERN, Geneva, Switzerland, 13-16 Feb 2002: Proceedings, pp.39-141
3.
Supernova pointing with low- and high-energy neutrino detectors / Tomás, R (Munich, Max Planck Inst.) ; Semikoz, Dmitry V (Munich, Max Planck Inst.) ; Raffelt, Georg G (Munich, Max Planck Inst.) ; Kachelriess, M (Munich, Max Planck Inst.) ; Dighe, Amol S (Munich, Max Planck Inst.)
A future galactic SN can be located several hours before the optical explosion through the MeV-neutrino burst, exploiting the directionality of $nu$-$e$-scattering in a water Cherenkov detector such as Super-Kamiokande. We study the statistical efficiency of different methods for extracting the SN direction and identify a simple approach that is nearly optimal, yet independent of the exact SN neutrino spectra. [...]
hep-ph/0307050; MPP-2003-21.- Geneva : CERN, 2003 - 12 p. - Published in : Phys. Rev. D 68 (2003) 093013
- Published in : PoS: AHEP2003 (2003) , pp. 020 Published version from PoS: AHEP2003-020 - PDF; 020proc - PDF; External link: Fulltext
In : International Workshop on Astroparticle and High Energy Physics, Valencia, Spain, 14 - 18 Oct 2003, pp.020
4.
Semi-leptonic and rare decays / Borzumati, Francesca M ; Champion, T J ; Aoki, M ; Bevan, A ; Cottingham, W N ; Dighe, Amol S ; Gambino, Paolo ; De Groot, N ; Harrison, P F ; Khalil, S et al.
We review the theoretical and experimental results on semi-leptonic and rare B decays presented in working group 2 of the UK phenomenology workshop on heavy flavour physics and CP violation in Durham, 2000. (0 refs)..
Geneva : CERN, 2001 - Published in : J. Phys. G 27 (2001) 1159-1160
5.
Earth matter effects on the supernova neutrino spectra / Dighe, Amol S. (CERN)
We explore the earth matter effects on the energy spectra of neutrinos from a supernova. We show that the observations of the energy spectra of $\nu_e$ and $\bar{\nu}_e$ from a galactic supernova may enable us to identify the solar neutrino solution, to determine the sign of $\Delta m^2_{32}$, and to probe the mixing matrix element $|U_{e3}|^2$ to values as low as $10^{-3}$. [...]
hep-ph/0106325; MPI-PHT-2001-19; MPI-PHT-2001-19.- München : Max-Planck Inst., 2001 - 8 p. - Published in : , pp. 275-282 Access to fulltext document: PDF; Fulltext: PDF; External link: hep-ph/0106325 PDF
In : Cairo International Conference On High Energy Physics, Cairo, Egypt, 9 - 14 Jan 2001, pp.275-282
6.
No-go for exactly degenerate neutrinos at high scale? / Dighe, Amol S. (CERN) ; Joshipura, Anjan S. (CERN ; Ahmedabad, Phys. Res. Lab)
We show in a model independent manner that, if the magnitudes of Majorana masses of neutrinos are exactly equal at some high scale, the radiative corrections cannot reproduce the observed masses and mixing spectrum at the low scale, irrespective of the Majorana phases or the mixing angles at the high scale..
hep-ph/0010079 ; CERN-TH-2000-301 ; CERN-TH-2000-301.
- 2000. - 8 p.
Preprint - Full text - Access to fulltext document - Access to fulltext document
7.
The CKM phase $\alpha$ through $B \to a_{0}\pi$ / Dighe, Amol S. (CERN) ; Kim, C.S. (Yonsei U. ; Wisconsin U., Madison)
We propose the decay modes $B \to a_0 (\to \eta \pi) \pi$ to determine the CKM phase $\alpha$. One can analyze these modes through (i) the $B \to a_0 \pi$ isospin pentagon, (ii) the time dependent Dalitz plot of $B^0(t) \to a_0^{\pm} \pi^{\mp} \to \eta \pi^+ \pi^-$, and (iii) the time dependence of $B^0(t) \to a_0^0 (\to \eta \pi^0) \pi^0$. [...]
hep-ph/0004244; CERN-TH-2000-122; YUMS-00-04; CERN-TH-2000-122; YUMS-2000-04.- Geneva : CERN, 2000 - 10 p. - Published in : Phys. Rev. D 62 (2000) 111302 APS Published version, local copy: PDF; Access to fulltext document: PDF; Fulltext: PDF; External link: Preprint
In : 30th International Conference on High-energy Physics, Osaka, Japan, 27 Jul - 2 Aug 2000, pp.e-page 85 - Please contact the library if you need to access this document.
8.
Radiative magnification of neutrino mixings and a natural explanation of the neutrino anomalies / Balaji, K.R.S. (IMSc, Chennai) ; Dighe, Amol S. (CERN) ; Mohapatra, R.N. (Maryland U.) ; Parida, M.K. (Northeastern Hill U., Shillong)
We show that the neutrino mixing pattern with the large mixing required for the atmospheric neutrino problem and the small mixing angle MSW solution for the solar neutrino problem can be naturally generated through radiative magnification, even though all the mixing angles at the seesaw scale may be small. This can account for the neutrino anomalies as well as the CHOOZ constraints in the context of quark-lepton unified theories, where the quark and lepton mixing angles are expected to be similar in magnitude at the high scale. [...]
hep-ph/0002177; CERN-TH-2000-044; IMSC-2000-02-04; UMD-PP-00-054; CERN-TH-2000-044; IMSC-2000-02-04; UMD-PP-2000-054.- Geneva : CERN, 2000 - 14 p. - Published in : Phys. Lett. B 481 (2000) 33-38 Access to fulltext document: PDF; Fulltext: PDF; External link: Preprint - Please contact the library if you need to access this document.
9.
Generation of large flavor mixing from radiative corrections / Balaji, K.R.S. (IMSc, Chennai) ; Dighe, Amol S. (CERN) ; Mohapatra, R.N. (Maryland U.) ; Parida, M.K. (Northeastern Hill U., Shillong)
We provide a model independent criterion which would guarantee a large flavor mixing of two quasi-degenerate Majorana neutrinos at the low scale, irrespective of the mixing at the high scale. We also show that such a situation is realizable for a phenomenologically interesting range of parameters of the weak scale theory. [...]
hep-ph/0001310; CERN-TH-2000-026; IMSC-2000-01-01; CERN-TH-2000-026; IMSC-2000-01-01.- Geneva : CERN, 2000 - 14 p. - Published in : Phys. Rev. Lett. 84 (2000) 5034-5037 APS Published version, local copy: PDF; Access to fulltext document: PDF; Fulltext: PDF; External link: Preprint - Please contact the library if you need to access this document.
10.
Resolving ambiguities in the neutrino mass-flavour spectrum from supernova neutrinos / Dighe, Amol S. (CERN)
We analyze the neutrino conversions inside a supernova in the 3$\nu$ mixing scheme, and their effects on the neutrino spectra observed at the earth. We find that the observations of the energy spectra of neutrinos from a future galactic supernova may enable us to identify the solar neutrino solution, to determine the sign of $\Delta m^2_{32}$, and to probe the mixing matrix element |U_{e3}|^2 to values as low as 10^{-4}-10^{-3}..
hep-ph/9912414; CERN-TH-99-382; CERN-TH-99-382.- Geneva : CERN, 2000 - 3 p. - Published in : Nucl. Phys. B, Proc. Suppl. 87 (2000) 327-329 Access to fulltext document: PDF; Fulltext: PDF; External link: Preprint
In : 6th International Workshop on Topics in Astroparticle and Underground Physics, Paris, France, 6 - 10 Sep 1999, pp.327-329 - Please contact the library if you need to access this document.

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