Optimised sensitivity to leptonic CP violation from spectral information: the LBNO case at 2300 km baseline
One of the main goals of the Long Baseline Neutrino Observatory (LBNO) is to study the \(L/E\) behaviour (spectral information) of the electron neutrino and antineutrino appearance probabilities, in order to determine the unknown CP-violation phase \(\delta_{CP}\) and discover CP-violation in the le...
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| creator | Agarwalla, S K Aittola, M Alekou, A Asfandiyarov, R Ballett, P Bartmann, W Bay, F Biskup, B Blebea-Apostu, A M Blondel, A Bolognesi, S Borriello, E Buizza-Avanzini, M Calin, M Cantini, C Cata-Danil, G Charitonidis, N Chaussard, L Chesneanu, D De Bonis, I Declais, Y Duchesneau, D Dumarchez, J Efthymiopoulos, I Eliseev, A Enqvist, T Epprecht, L Esanu, T Franco, D Galymov, V Gavrilov, G Giganti, C Goddard, B Gomoiu, C M Gornushkin, Y A Gorodetzky, P Haesler, A Horikawa, S Huitu, K Jipa, A Kainulainen, K Karadzhov, Y Kopylov, A N Korzenev, A Kryn, D Kuusiniemi, P Lazanu, I Loo, K Margineanu, R M Marteau, J Mineev, O Mirizzi, A Mitrica, B Murphy, S Nakadaira, T Nesterenko, D A Nguyen, K Noah, E Oprima, A Ovsyannikova, T Pascoli, S Patzak, T Pectu, M Pennacchio, E Periale, L Pessard, H Popov, B Resnati, F Rummukainen, K Saftoiu, A Saviano, N Scantamburlo, E Sergiampietri, F Sgalaberna, D Shaposhnikova, E Slupecki, M Smargianaki, D Stanca, D Steerenberg, R Sterian, A R Sterian, P Suhonen, J Suvorov, V Toma, G Trzaska, W H Tsenov, R Tuominen, K Valram, M Vankova-Kirilova, G Vannucci, F Vasseur, G Velotti, F Venturi, V Vihonen, S Vincke, H Weber, A S Wu Yershov, N Zambelli, L Zito, M |
| description | One of the main goals of the Long Baseline Neutrino Observatory (LBNO) is to study the \(L/E\) behaviour (spectral information) of the electron neutrino and antineutrino appearance probabilities, in order to determine the unknown CP-violation phase \(\delta_{CP}\) and discover CP-violation in the leptonic sector. The result is based on the measurement of the appearance probabilities in a broad range of energies, covering t he 1st and 2nd oscillation maxima, at a very long baseline of 2300 km. The sensitivity of the experiment can be maximised by optimising the energy spectra of the neutrino and anti-neutrino fluxes. Such an optimisation requires exploring an extended range of parameters describing in details the geometries and properties of the primary protons, hadron target and focusing elements in the neutrino beam line. In this paper we present a numerical solution that leads to an optimised energy spectra and study its impact on the sensitivity of LBNO to discover leptonic CP violation. In the optimised flux both 1st and 2nd oscillation maxima play an important role in the CP sensitivity. The studies also show that this configuration is less sensitive to systematic errors (e.g. on the total event rates) than an experiment which mainly relies on the neutrino-antineutrino asymmetry at the 1st maximum to determine the existence of CP-violation. |
| format | Article |
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The result is based on the measurement of the appearance probabilities in a broad range of energies, covering t he 1st and 2nd oscillation maxima, at a very long baseline of 2300 km. The sensitivity of the experiment can be maximised by optimising the energy spectra of the neutrino and anti-neutrino fluxes. Such an optimisation requires exploring an extended range of parameters describing in details the geometries and properties of the primary protons, hadron target and focusing elements in the neutrino beam line. In this paper we present a numerical solution that leads to an optimised energy spectra and study its impact on the sensitivity of LBNO to discover leptonic CP violation. In the optimised flux both 1st and 2nd oscillation maxima play an important role in the CP sensitivity. The studies also show that this configuration is less sensitive to systematic errors (e.g. on the total event rates) than an experiment which mainly relies on the neutrino-antineutrino asymmetry at the 1st maximum to determine the existence of CP-violation.</description><identifier>EISSN: 2331-8422</identifier><language>eng</language><publisher>Ithaca: Cornell University Library, arXiv.org</publisher><subject>CP violation ; Energy spectra ; Fluxes ; Leptons ; Matter & antimatter ; Maxima ; Neutrino beams ; Neutrinos ; Optimization ; Sensitivity ; Systematic errors</subject><ispartof>arXiv.org, 2014-12</ispartof><rights>2014. This work is published under http://arxiv.org/licenses/nonexclusive-distrib/1.0/ (the “License”). 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E</creatorcontrib><creatorcontrib>Oprima, A</creatorcontrib><creatorcontrib>Ovsyannikova, T</creatorcontrib><creatorcontrib>Pascoli, S</creatorcontrib><creatorcontrib>Patzak, T</creatorcontrib><creatorcontrib>Pectu, M</creatorcontrib><creatorcontrib>Pennacchio, E</creatorcontrib><creatorcontrib>Periale, L</creatorcontrib><creatorcontrib>Pessard, H</creatorcontrib><creatorcontrib>Popov, B</creatorcontrib><creatorcontrib>Resnati, F</creatorcontrib><creatorcontrib>Rummukainen, K</creatorcontrib><creatorcontrib>Saftoiu, A</creatorcontrib><creatorcontrib>Saviano, N</creatorcontrib><creatorcontrib>Scantamburlo, E</creatorcontrib><creatorcontrib>Sergiampietri, F</creatorcontrib><creatorcontrib>Sgalaberna, D</creatorcontrib><creatorcontrib>Shaposhnikova, E</creatorcontrib><creatorcontrib>Slupecki, M</creatorcontrib><creatorcontrib>Smargianaki, D</creatorcontrib><creatorcontrib>Stanca, D</creatorcontrib><creatorcontrib>Steerenberg, R</creatorcontrib><creatorcontrib>Sterian, A R</creatorcontrib><creatorcontrib>Sterian, P</creatorcontrib><creatorcontrib>Suhonen, J</creatorcontrib><creatorcontrib>Suvorov, V</creatorcontrib><creatorcontrib>Toma, G</creatorcontrib><creatorcontrib>Trzaska, W H</creatorcontrib><creatorcontrib>Tsenov, R</creatorcontrib><creatorcontrib>Tuominen, K</creatorcontrib><creatorcontrib>Valram, M</creatorcontrib><creatorcontrib>Vankova-Kirilova, G</creatorcontrib><creatorcontrib>Vannucci, F</creatorcontrib><creatorcontrib>Vasseur, G</creatorcontrib><creatorcontrib>Velotti, F</creatorcontrib><creatorcontrib>Venturi, V</creatorcontrib><creatorcontrib>Vihonen, S</creatorcontrib><creatorcontrib>Vincke, H</creatorcontrib><creatorcontrib>Weber, A</creatorcontrib><creatorcontrib>S Wu</creatorcontrib><creatorcontrib>Yershov, N</creatorcontrib><creatorcontrib>Zambelli, L</creatorcontrib><creatorcontrib>Zito, M</creatorcontrib><title>Optimised sensitivity to leptonic CP violation from spectral information: the LBNO case at 2300 km baseline</title><title>arXiv.org</title><description>One of the main goals of the Long Baseline Neutrino Observatory (LBNO) is to study the \(L/E\) behaviour (spectral information) of the electron neutrino and antineutrino appearance probabilities, in order to determine the unknown CP-violation phase \(\delta_{CP}\) and discover CP-violation in the leptonic sector. The result is based on the measurement of the appearance probabilities in a broad range of energies, covering t he 1st and 2nd oscillation maxima, at a very long baseline of 2300 km. The sensitivity of the experiment can be maximised by optimising the energy spectra of the neutrino and anti-neutrino fluxes. Such an optimisation requires exploring an extended range of parameters describing in details the geometries and properties of the primary protons, hadron target and focusing elements in the neutrino beam line. In this paper we present a numerical solution that leads to an optimised energy spectra and study its impact on the sensitivity of LBNO to discover leptonic CP violation. In the optimised flux both 1st and 2nd oscillation maxima play an important role in the CP sensitivity. The studies also show that this configuration is less sensitive to systematic errors (e.g. on the total event rates) than an experiment which mainly relies on the neutrino-antineutrino asymmetry at the 1st maximum to determine the existence of CP-violation.</description><subject>CP violation</subject><subject>Energy spectra</subject><subject>Fluxes</subject><subject>Leptons</subject><subject>Matter & antimatter</subject><subject>Maxima</subject><subject>Neutrino beams</subject><subject>Neutrinos</subject><subject>Optimization</subject><subject>Sensitivity</subject><subject>Systematic 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arXiv.org</general><scope>8FE</scope><scope>8FG</scope><scope>ABJCF</scope><scope>ABUWG</scope><scope>AFKRA</scope><scope>AZQEC</scope><scope>BENPR</scope><scope>BGLVJ</scope><scope>CCPQU</scope><scope>DWQXO</scope><scope>HCIFZ</scope><scope>L6V</scope><scope>M7S</scope><scope>PHGZM</scope><scope>PHGZT</scope><scope>PIMPY</scope><scope>PKEHL</scope><scope>PQEST</scope><scope>PQGLB</scope><scope>PQQKQ</scope><scope>PQUKI</scope><scope>PRINS</scope><scope>PTHSS</scope></search><sort><creationdate>20141201</creationdate><title>Optimised sensitivity to leptonic CP violation from spectral information: the LBNO case at 2300 km baseline</title><author>Agarwalla, S K ; Aittola, M ; Alekou, A ; Asfandiyarov, R ; Ballett, P ; Bartmann, W ; Bay, F ; Biskup, B ; Blebea-Apostu, A M ; Blondel, A ; Bolognesi, S ; Borriello, E ; Buizza-Avanzini, M ; Calin, M ; Cantini, C ; Cata-Danil, G ; Charitonidis, N ; Chaussard, L ; Chesneanu, D ; De Bonis, I ; Declais, Y ; Duchesneau, D ; Dumarchez, J ; Efthymiopoulos, I ; Eliseev, A ; Enqvist, T ; Epprecht, L ; Esanu, T ; Franco, D ; Galymov, V ; Gavrilov, G ; Giganti, C ; Goddard, B ; Gomoiu, C M ; Gornushkin, Y A ; Gorodetzky, P ; Haesler, A ; Horikawa, S ; Huitu, K ; Jipa, A ; Kainulainen, K ; Karadzhov, Y ; Kopylov, A N ; Korzenev, A ; Kryn, D ; Kuusiniemi, P ; Lazanu, I ; Loo, K ; Margineanu, R M ; Marteau, J ; Mineev, O ; Mirizzi, A ; Mitrica, B ; Murphy, S ; Nakadaira, T ; Nesterenko, D A ; Nguyen, K ; Noah, E ; Oprima, A ; Ovsyannikova, T ; Pascoli, S ; Patzak, T ; Pectu, M ; Pennacchio, E ; Periale, L ; Pessard, H ; Popov, B ; Resnati, F ; Rummukainen, K ; Saftoiu, A ; Saviano, N ; Scantamburlo, E ; Sergiampietri, F ; Sgalaberna, D ; Shaposhnikova, E ; Slupecki, M ; Smargianaki, D ; Stanca, D ; Steerenberg, R ; Sterian, A R ; Sterian, P ; Suhonen, J ; Suvorov, V ; Toma, G ; Trzaska, W H ; Tsenov, R ; Tuominen, K ; Valram, M ; Vankova-Kirilova, G ; Vannucci, F ; Vasseur, G ; Velotti, F ; Venturi, V ; Vihonen, S ; Vincke, H ; Weber, A ; S Wu ; Yershov, N ; Zambelli, L ; Zito, M</author></sort><facets><frbrtype>5</frbrtype><frbrgroupid>cdi_FETCH-proquest_journals_20855237493</frbrgroupid><rsrctype>articles</rsrctype><prefilter>articles</prefilter><language>eng</language><creationdate>2014</creationdate><topic>CP violation</topic><topic>Energy spectra</topic><topic>Fluxes</topic><topic>Leptons</topic><topic>Matter & antimatter</topic><topic>Maxima</topic><topic>Neutrino beams</topic><topic>Neutrinos</topic><topic>Optimization</topic><topic>Sensitivity</topic><topic>Systematic errors</topic><toplevel>online_resources</toplevel><creatorcontrib>Agarwalla, S K</creatorcontrib><creatorcontrib>Aittola, M</creatorcontrib><creatorcontrib>Alekou, A</creatorcontrib><creatorcontrib>Asfandiyarov, R</creatorcontrib><creatorcontrib>Ballett, P</creatorcontrib><creatorcontrib>Bartmann, W</creatorcontrib><creatorcontrib>Bay, F</creatorcontrib><creatorcontrib>Biskup, B</creatorcontrib><creatorcontrib>Blebea-Apostu, A M</creatorcontrib><creatorcontrib>Blondel, A</creatorcontrib><creatorcontrib>Bolognesi, S</creatorcontrib><creatorcontrib>Borriello, E</creatorcontrib><creatorcontrib>Buizza-Avanzini, M</creatorcontrib><creatorcontrib>Calin, M</creatorcontrib><creatorcontrib>Cantini, C</creatorcontrib><creatorcontrib>Cata-Danil, G</creatorcontrib><creatorcontrib>Charitonidis, N</creatorcontrib><creatorcontrib>Chaussard, L</creatorcontrib><creatorcontrib>Chesneanu, D</creatorcontrib><creatorcontrib>De Bonis, I</creatorcontrib><creatorcontrib>Declais, Y</creatorcontrib><creatorcontrib>Duchesneau, D</creatorcontrib><creatorcontrib>Dumarchez, J</creatorcontrib><creatorcontrib>Efthymiopoulos, I</creatorcontrib><creatorcontrib>Eliseev, A</creatorcontrib><creatorcontrib>Enqvist, T</creatorcontrib><creatorcontrib>Epprecht, L</creatorcontrib><creatorcontrib>Esanu, T</creatorcontrib><creatorcontrib>Franco, D</creatorcontrib><creatorcontrib>Galymov, V</creatorcontrib><creatorcontrib>Gavrilov, G</creatorcontrib><creatorcontrib>Giganti, C</creatorcontrib><creatorcontrib>Goddard, B</creatorcontrib><creatorcontrib>Gomoiu, C M</creatorcontrib><creatorcontrib>Gornushkin, Y A</creatorcontrib><creatorcontrib>Gorodetzky, P</creatorcontrib><creatorcontrib>Haesler, A</creatorcontrib><creatorcontrib>Horikawa, S</creatorcontrib><creatorcontrib>Huitu, K</creatorcontrib><creatorcontrib>Jipa, A</creatorcontrib><creatorcontrib>Kainulainen, K</creatorcontrib><creatorcontrib>Karadzhov, Y</creatorcontrib><creatorcontrib>Kopylov, A N</creatorcontrib><creatorcontrib>Korzenev, A</creatorcontrib><creatorcontrib>Kryn, D</creatorcontrib><creatorcontrib>Kuusiniemi, P</creatorcontrib><creatorcontrib>Lazanu, I</creatorcontrib><creatorcontrib>Loo, K</creatorcontrib><creatorcontrib>Margineanu, R M</creatorcontrib><creatorcontrib>Marteau, J</creatorcontrib><creatorcontrib>Mineev, O</creatorcontrib><creatorcontrib>Mirizzi, A</creatorcontrib><creatorcontrib>Mitrica, B</creatorcontrib><creatorcontrib>Murphy, S</creatorcontrib><creatorcontrib>Nakadaira, T</creatorcontrib><creatorcontrib>Nesterenko, D A</creatorcontrib><creatorcontrib>Nguyen, K</creatorcontrib><creatorcontrib>Noah, E</creatorcontrib><creatorcontrib>Oprima, A</creatorcontrib><creatorcontrib>Ovsyannikova, T</creatorcontrib><creatorcontrib>Pascoli, S</creatorcontrib><creatorcontrib>Patzak, T</creatorcontrib><creatorcontrib>Pectu, M</creatorcontrib><creatorcontrib>Pennacchio, E</creatorcontrib><creatorcontrib>Periale, L</creatorcontrib><creatorcontrib>Pessard, H</creatorcontrib><creatorcontrib>Popov, B</creatorcontrib><creatorcontrib>Resnati, F</creatorcontrib><creatorcontrib>Rummukainen, K</creatorcontrib><creatorcontrib>Saftoiu, A</creatorcontrib><creatorcontrib>Saviano, N</creatorcontrib><creatorcontrib>Scantamburlo, E</creatorcontrib><creatorcontrib>Sergiampietri, F</creatorcontrib><creatorcontrib>Sgalaberna, D</creatorcontrib><creatorcontrib>Shaposhnikova, E</creatorcontrib><creatorcontrib>Slupecki, M</creatorcontrib><creatorcontrib>Smargianaki, D</creatorcontrib><creatorcontrib>Stanca, D</creatorcontrib><creatorcontrib>Steerenberg, R</creatorcontrib><creatorcontrib>Sterian, A R</creatorcontrib><creatorcontrib>Sterian, P</creatorcontrib><creatorcontrib>Suhonen, J</creatorcontrib><creatorcontrib>Suvorov, V</creatorcontrib><creatorcontrib>Toma, G</creatorcontrib><creatorcontrib>Trzaska, W H</creatorcontrib><creatorcontrib>Tsenov, R</creatorcontrib><creatorcontrib>Tuominen, K</creatorcontrib><creatorcontrib>Valram, M</creatorcontrib><creatorcontrib>Vankova-Kirilova, G</creatorcontrib><creatorcontrib>Vannucci, F</creatorcontrib><creatorcontrib>Vasseur, G</creatorcontrib><creatorcontrib>Velotti, F</creatorcontrib><creatorcontrib>Venturi, V</creatorcontrib><creatorcontrib>Vihonen, S</creatorcontrib><creatorcontrib>Vincke, H</creatorcontrib><creatorcontrib>Weber, A</creatorcontrib><creatorcontrib>S Wu</creatorcontrib><creatorcontrib>Yershov, N</creatorcontrib><creatorcontrib>Zambelli, L</creatorcontrib><creatorcontrib>Zito, M</creatorcontrib><collection>ProQuest SciTech Collection</collection><collection>ProQuest Technology Collection</collection><collection>Materials Science & Engineering Database (Proquest)</collection><collection>ProQuest Central (Alumni)</collection><collection>ProQuest Central UK/Ireland</collection><collection>ProQuest Central Essentials</collection><collection>ProQuest Central</collection><collection>Technology Collection</collection><collection>ProQuest One Community College</collection><collection>ProQuest Central</collection><collection>SciTech Premium Collection</collection><collection>ProQuest Engineering Collection</collection><collection>Engineering Database</collection><collection>ProQuest Central (New)</collection><collection>ProQuest One Academic (New)</collection><collection>Publicly Available Content Database</collection><collection>ProQuest One Academic Middle East (New)</collection><collection>ProQuest One Academic Eastern Edition (DO NOT USE)</collection><collection>ProQuest One Applied & Life Sciences</collection><collection>ProQuest One Academic</collection><collection>ProQuest One Academic UKI Edition</collection><collection>ProQuest Central China</collection><collection>Engineering collection</collection></facets><delivery><delcategory>Remote Search Resource</delcategory><fulltext>fulltext</fulltext></delivery><addata><au>Agarwalla, S K</au><au>Aittola, M</au><au>Alekou, A</au><au>Asfandiyarov, R</au><au>Ballett, P</au><au>Bartmann, W</au><au>Bay, F</au><au>Biskup, B</au><au>Blebea-Apostu, A M</au><au>Blondel, A</au><au>Bolognesi, S</au><au>Borriello, E</au><au>Buizza-Avanzini, M</au><au>Calin, M</au><au>Cantini, C</au><au>Cata-Danil, G</au><au>Charitonidis, N</au><au>Chaussard, L</au><au>Chesneanu, D</au><au>De Bonis, I</au><au>Declais, Y</au><au>Duchesneau, D</au><au>Dumarchez, J</au><au>Efthymiopoulos, I</au><au>Eliseev, A</au><au>Enqvist, T</au><au>Epprecht, L</au><au>Esanu, T</au><au>Franco, D</au><au>Galymov, V</au><au>Gavrilov, G</au><au>Giganti, C</au><au>Goddard, B</au><au>Gomoiu, C M</au><au>Gornushkin, Y A</au><au>Gorodetzky, P</au><au>Haesler, A</au><au>Horikawa, S</au><au>Huitu, K</au><au>Jipa, A</au><au>Kainulainen, K</au><au>Karadzhov, Y</au><au>Kopylov, A N</au><au>Korzenev, A</au><au>Kryn, D</au><au>Kuusiniemi, P</au><au>Lazanu, I</au><au>Loo, K</au><au>Margineanu, R M</au><au>Marteau, J</au><au>Mineev, O</au><au>Mirizzi, A</au><au>Mitrica, B</au><au>Murphy, S</au><au>Nakadaira, T</au><au>Nesterenko, D A</au><au>Nguyen, K</au><au>Noah, E</au><au>Oprima, A</au><au>Ovsyannikova, T</au><au>Pascoli, S</au><au>Patzak, T</au><au>Pectu, M</au><au>Pennacchio, E</au><au>Periale, L</au><au>Pessard, H</au><au>Popov, B</au><au>Resnati, F</au><au>Rummukainen, K</au><au>Saftoiu, A</au><au>Saviano, N</au><au>Scantamburlo, E</au><au>Sergiampietri, F</au><au>Sgalaberna, D</au><au>Shaposhnikova, E</au><au>Slupecki, M</au><au>Smargianaki, D</au><au>Stanca, D</au><au>Steerenberg, R</au><au>Sterian, A R</au><au>Sterian, P</au><au>Suhonen, J</au><au>Suvorov, V</au><au>Toma, G</au><au>Trzaska, W H</au><au>Tsenov, R</au><au>Tuominen, K</au><au>Valram, M</au><au>Vankova-Kirilova, G</au><au>Vannucci, F</au><au>Vasseur, G</au><au>Velotti, F</au><au>Venturi, V</au><au>Vihonen, S</au><au>Vincke, H</au><au>Weber, A</au><au>S Wu</au><au>Yershov, N</au><au>Zambelli, L</au><au>Zito, M</au><format>book</format><genre>document</genre><ristype>GEN</ristype><atitle>Optimised sensitivity to leptonic CP violation from spectral information: the LBNO case at 2300 km baseline</atitle><jtitle>arXiv.org</jtitle><date>2014-12-01</date><risdate>2014</risdate><eissn>2331-8422</eissn><abstract>One of the main goals of the Long Baseline Neutrino Observatory (LBNO) is to study the \(L/E\) behaviour (spectral information) of the electron neutrino and antineutrino appearance probabilities, in order to determine the unknown CP-violation phase \(\delta_{CP}\) and discover CP-violation in the leptonic sector. The result is based on the measurement of the appearance probabilities in a broad range of energies, covering t he 1st and 2nd oscillation maxima, at a very long baseline of 2300 km. The sensitivity of the experiment can be maximised by optimising the energy spectra of the neutrino and anti-neutrino fluxes. Such an optimisation requires exploring an extended range of parameters describing in details the geometries and properties of the primary protons, hadron target and focusing elements in the neutrino beam line. In this paper we present a numerical solution that leads to an optimised energy spectra and study its impact on the sensitivity of LBNO to discover leptonic CP violation. In the optimised flux both 1st and 2nd oscillation maxima play an important role in the CP sensitivity. The studies also show that this configuration is less sensitive to systematic errors (e.g. on the total event rates) than an experiment which mainly relies on the neutrino-antineutrino asymmetry at the 1st maximum to determine the existence of CP-violation.</abstract><cop>Ithaca</cop><pub>Cornell University Library, arXiv.org</pub><oa>free_for_read</oa></addata></record> |
| fulltext | fulltext |
| identifier | EISSN: 2331-8422 |
| ispartof | arXiv.org, 2014-12 |
| issn | 2331-8422 |
| language | eng |
| recordid | cdi_proquest_journals_2085523749 |
| source | World Web Journals |
| subjects | CP violation Energy spectra Fluxes Leptons Matter & antimatter Maxima Neutrino beams Neutrinos Optimization Sensitivity Systematic errors |
| title | Optimised sensitivity to leptonic CP violation from spectral information: the LBNO case at 2300 km baseline |
| url | https://sfx.bib-bvb.de/sfx_tum?ctx_ver=Z39.88-2004&ctx_enc=info:ofi/enc:UTF-8&ctx_tim=2025-02-14T15%3A59%3A55IST&url_ver=Z39.88-2004&url_ctx_fmt=infofi/fmt:kev:mtx:ctx&rfr_id=info:sid/primo.exlibrisgroup.com:primo3-Article-proquest&rft_val_fmt=info:ofi/fmt:kev:mtx:book&rft.genre=document&rft.atitle=Optimised%20sensitivity%20to%20leptonic%20CP%20violation%20from%20spectral%20information:%20the%20LBNO%20case%20at%202300%20km%20baseline&rft.jtitle=arXiv.org&rft.au=Agarwalla,%20S%20K&rft.date=2014-12-01&rft.eissn=2331-8422&rft_id=info:doi/&rft_dat=%3Cproquest%3E2085523749%3C/proquest%3E%3Curl%3E%3C/url%3E&disable_directlink=true&sfx.directlink=off&sfx.report_link=0&rft_id=info:oai/&rft_pqid=2085523749&rft_id=info:pmid/&rfr_iscdi=true |