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Book ; Thesis: Measurement of [lambda] polarisation observables at the COSY-TOF spectrometer

Pizzolotto, Cecilia

2007

Title variant	Measurement of lambda polaristion
Author's details	Cecilia Pizzolotto
Language	English
Size	III, 106 S., graph. Darst.
Document type	Book ; Thesis
Thesis / German Habilitation thesis	Univ., Diss.--Erlangen, 2007
Database	Library catalogue of the German National Library of Science and Technology (TIB), Hannover

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Article ; Online: DFG-based mid-IR tunable source with 0.5 mJ energy and a 30 pm linewidth.

Stoychev, Lyubomir I / Cabrera, Humberto / Suárez-Vargas, Jose J / Baruzzo, Marco / Gadedjisso-Tossou, Komlan S / Nikolov, Ivaylo P / Sigalotti, Paolo / Demidovich, Alexander A / Mocchiutti, Emiliano / Pizzolotto, Cecilia / Niemela, Joseph / Toci, Guido / Danailov, Miltcho B / Vacchi, Andrea

Optics letters

2020 Volume 45, Issue 19, Page(s) 5526–5529

Abstract: We report on a laser system based on difference frequency generation (DFG) to produce tunable, narrow-linewidth (< ... ...

Abstract	We report on a laser system based on difference frequency generation (DFG) to produce tunable, narrow-linewidth (<30
Language	English
Publishing date	2020-10-02
Publishing country	United States
Document type	Journal Article
ISSN	1539-4794
ISSN (online)	1539-4794
DOI	10.1364/OL.405272
Database	MEDical Literature Analysis and Retrieval System OnLINE

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Article ; Online: 24 mJ Cr

Stoychev, Lyubomir I / Cabrera, Humberto / Gadedjisso-Tossou, Komlan S / Vasiliev, Nikolai / Zaporozhchenko, Yuri / Nikolov, Ivaylo P / Sigalotti, Paolo / Demidovich, Alexander A / Suárez-Vargas, José J / Mocchiutti, Emiliano / Pizzolotto, Cecilia / Niemela, Joseph / Baruzzo, Marco / Danailov, Miltcho B / Vacchi, Andrea

The Review of scientific instruments

2019 Volume 90, Issue 9, Page(s) 93002

Abstract: We present the design of a Cr:forsterite based single-frequency master-oscillator power-amplifier laser system delivering much higher output energy compared to previous literature reports. The system has four amplifying stages with two-pass configuration ...

Abstract	We present the design of a Cr:forsterite based single-frequency master-oscillator power-amplifier laser system delivering much higher output energy compared to previous literature reports. The system has four amplifying stages with two-pass configuration each, thus enabling the generation of 24 mJ output energy in the spectral region around 1262 nm. It is demonstrated that the presented Cr:forsterite amplifier preserves high spectral and pulse quality, allowing a straightforward energy scaling. This laser system is a promising tool for tunable nonlinear down-conversion to the mid-infrared spectral range and will be a key building block in a system for high-resolution muonic hydrogen spectroscopy in the 6.8 μm range.
Language	English
Publishing date	2019-09-30
Publishing country	United States
Document type	Journal Article
ZDB-ID	209865-9
ISSN	1089-7623 ; 0034-6748
ISSN (online)	1089-7623
ISSN	0034-6748
DOI	10.1063/1.5115105
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Article ; Online: Cosmic-ray positron energy spectrum measured by PAMELA.

Adriani, O / Barbarino, G C / Bazilevskaya, G A / Bellotti, R / Bianco, A / Boezio, M / Bogomolov, E A / Bongi, M / Bonvicini, V / Bottai, S / Bruno, A / Cafagna, F / Campana, D / Carbone, R / Carlson, P / Casolino, M / Castellini, G / De Donato, C / De Santis, C /

De Simone, N / Di Felice, V / Formato, V / Galper, A M / Karelin, A V / Koldashov, S V / Koldobskiy, S A / Krutkov, S Y / Kvashnin, A N / Leonov, A / Malakhov, V / Marcelli, L / Martucci, M / Mayorov, A G / Menn, W / Mergé, M / Mikhailov, V V / Mocchiutti, E / Monaco, A / Mori, N / Munini, R / Osteria, G / Palma, F / Papini, P / Pearce, M / Picozza, P / Pizzolotto, C / Ricci, M / Ricciarini, S B / Rossetto, L / Sarkar, R / Scotti, V / Simon, M / Sparvoli, R / Spillantini, P / Stochaj, S J / Stockton, J C / Stozhkov, Y I / Vacchi, A / Vannuccini, E / Vasilyev, G I / Voronov, S A / Yurkin, Y T / Zampa, G / Zampa, N / Zverev, V G

Physical review letters

2013 Volume 111, Issue 8, Page(s) 81102

Abstract: Precision measurements of the positron component in the cosmic radiation provide important information about the propagation of cosmic rays and the nature of particle sources in our Galaxy. The satellite-borne experiment PAMELA has been used to make a ... ...

Abstract	Precision measurements of the positron component in the cosmic radiation provide important information about the propagation of cosmic rays and the nature of particle sources in our Galaxy. The satellite-borne experiment PAMELA has been used to make a new measurement of the cosmic-ray positron flux and fraction that extends previously published measurements up to 300 GeV in kinetic energy. The combined measurements of the cosmic-ray positron energy spectrum and fraction provide a unique tool to constrain interpretation models. During the recent solar minimum activity period from July 2006 to December 2009, approximately 24,500 positrons were observed. The results cannot be easily reconciled with purely secondary production, and additional sources of either astrophysical or exotic origin may be required.
Language	English
Publishing date	2013-08-23
Publishing country	United States
Document type	Journal Article
ZDB-ID	208853-8
ISSN	1079-7114 ; 0031-9007
ISSN (online)	1079-7114
ISSN	0031-9007
DOI	10.1103/PhysRevLett.111.081102
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Article ; Online: Cosmic-ray electron flux measured by the PAMELA experiment between 1 and 625 GeV.

Adriani, O / Barbarino, G C / Bazilevskaya, G A / Bellotti, R / Boezio, M / Bogomolov, E A / Bongi, M / Bonvicini, V / Borisov, S / Bottai, S / Bruno, A / Cafagna, F / Campana, D / Carbone, R / Carlson, P / Casolino, M / Castellini, G / Consiglio, L / De Pascale, M P /

De Santis, C / De Simone, N / Di Felice, V / Galper, A M / Gillard, W / Grishantseva, L / Jerse, G / Karelin, A V / Koldashov, S V / Krutkov, S Y / Kvashnin, A N / Leonov, A / Malakhov, V / Malvezzi, V / Marcelli, L / Mayorov, A G / Menn, W / Mikhailov, V V / Mocchiutti, E / Monaco, A / Mori, N / Nikonov, N / Osteria, G / Palma, F / Papini, P / Pearce, M / Picozza, P / Pizzolotto, C / Ricci, M / Ricciarini, S B / Rossetto, L / Sarkar, R / Simon, M / Sparvoli, R / Spillantini, P / Stochaj, S J / Stockton, J C / Stozhkov, Y I / Vacchi, A / Vannuccini, E / Vasilyev, G / Voronov, S A / Wu, J / Yurkin, Y T / Zampa, G / Zampa, N / Zverev, V G

Physical review letters

2011 Volume 106, Issue 20, Page(s) 201101

Abstract: Precision measurements of the electron component in the cosmic radiation provide important information about the origin and propagation of cosmic rays in the Galaxy. Here we present new results regarding negatively charged electrons between 1 and 625 GeV ...

Abstract	Precision measurements of the electron component in the cosmic radiation provide important information about the origin and propagation of cosmic rays in the Galaxy. Here we present new results regarding negatively charged electrons between 1 and 625 GeV performed by the satellite-borne experiment PAMELA. This is the first time that cosmic-ray e⁻ have been identified above 50 GeV. The electron spectrum can be described with a single power-law energy dependence with spectral index -3.18 ± 0.05 above the energy region influenced by the solar wind (> 30 GeV). No significant spectral features are observed and the data can be interpreted in terms of conventional diffusive propagation models. However, the data are also consistent with models including new cosmic-ray sources that could explain the rise in the positron fraction.
Language	English
Publishing date	2011-05-20
Publishing country	United States
Document type	Journal Article
ZDB-ID	208853-8
ISSN	1079-7114 ; 0031-9007
ISSN (online)	1079-7114
ISSN	0031-9007
DOI	10.1103/PhysRevLett.106.201101
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Article ; Online: PAMELA measurements of cosmic-ray proton and helium spectra.

Adriani, O / Barbarino, G C / Bazilevskaya, G A / Bellotti, R / Boezio, M / Bogomolov, E A / Bonechi, L / Bongi, M / Bonvicini, V / Borisov, S / Bottai, S / Bruno, A / Cafagna, F / Campana, D / Carbone, R / Carlson, P / Casolino, M / Castellini, G / Consiglio, L /

De Pascale, M P / De Santis, C / De Simone, N / Di Felice, V / Galper, A M / Gillard, W / Grishantseva, L / Jerse, G / Karelin, A V / Koldashov, S V / Krutkov, S Y / Kvashnin, A N / Leonov, A / Malakhov, V / Malvezzi, V / Marcelli, L / Mayorov, A G / Menn, W / Mikhailov, V V / Mocchiutti, E / Monaco, A / Mori, N / Nikonov, N / Osteria, G / Palma, F / Papini, P / Pearce, M / Picozza, P / Pizzolotto, C / Ricci, M / Ricciarini, S B / Rossetto, L / Sarkar, R / Simon, M / Sparvoli, R / Spillantini, P / Stozhkov, Y I / Vacchi, A / Vannuccini, E / Vasilyev, G / Voronov, S A / Yurkin, Y T / Wu, J / Zampa, G / Zampa, N / Zverev, V G

Science (New York, N.Y.)

2011 Volume 332, Issue 6025, Page(s) 69–72

Abstract: Protons and helium nuclei are the most abundant components of the cosmic radiation. Precise measurements of their fluxes are needed to understand the acceleration and subsequent propagation of cosmic rays in our Galaxy. We report precision measurements ... ...

Abstract	Protons and helium nuclei are the most abundant components of the cosmic radiation. Precise measurements of their fluxes are needed to understand the acceleration and subsequent propagation of cosmic rays in our Galaxy. We report precision measurements of the proton and helium spectra in the rigidity range 1 gigavolt to 1.2 teravolts performed by the satellite-borne experiment PAMELA (payload for antimatter matter exploration and light-nuclei astrophysics). We find that the spectral shapes of these two species are different and cannot be described well by a single power law. These data challenge the current paradigm of cosmic-ray acceleration in supernova remnants followed by diffusive propagation in the Galaxy. More complex processes of acceleration and propagation of cosmic rays are required to explain the spectral structures observed in our data.
Language	English
Publishing date	2011-04-01
Publishing country	United States
Document type	Journal Article ; Research Support, Non-U.S. Gov't
ZDB-ID	128410-1
ISSN	1095-9203 ; 0036-8075
ISSN (online)	1095-9203
ISSN	0036-8075
DOI	10.1126/science.1199172
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Article ; Online: PAMELA mission

Ricciarini S. B. / Adriani O. / Barbarino G.C. / Bazilevskaya G.A. / Bellotti R. / Boezio M. / Bogomolov E.A. / Bongi M. / Bonvicini V. / Bottai S. / Bruno A. / Cafagna F. / Campana D. / Carbone R. / Carlson P. / Casolino M. / Castellini G. / De Donato C. / De Pascale M.P. /

De Santis C. / De Simone N. / Di Felice V. / Formato V. / Galper A.M. / Karelin A.V. / Kheymits M.D. / Koldashov S.V. / Koldobskiy S. / Krutkov S.Yu. / Kvashnin A.N. / Leonov A. / Malakhov V. / Marcelli L. / Martucci M. / Mayorov A.G. / Menn W. / Mergè M. / Mikhailov V.V. / Mocchiutti E. / Monaco A. / Mori N. / Munini R. / Osteria G. / Palma F. / Panico B. / Papini P. / Pearce M. / Picozza P. / Pizzolotto C. / Ricci M. / Sarkar R. / Simon M. / Scotti V. / Sparvoli R. / Spillantini P. / Stozhkov Y.I. / Vacchi A. / Vannuccini E. / Vasilyev G.I. / Voronov S.A. / Yurkin Y.T. / Zampa G. / Zampa N. / Zverev V.G.

EPJ Web of Conferences, Vol 71, p

heralding a new era in cosmic ray physics

2014 Volume 00115

Abstract: After seven years of data taking in space, the experiment PAMELA is showing very interesting features in cosmic rays, namely in the fluxes of protons, helium, electrons, that might change our basic vision of the mechanisms of production, acceleration and ...

Abstract	After seven years of data taking in space, the experiment PAMELA is showing very interesting features in cosmic rays, namely in the fluxes of protons, helium, electrons, that might change our basic vision of the mechanisms of production, acceleration and propagation of cosmic rays in the galaxy. In addition, PAMELA measurements of cosmic antiproton and positron fluxes are setting strong constraints to the nature of Dark Matter. The continuous particle detection is allowing a constant monitoring of the solar activity and detailed study of the solar modulation for a long period, giving important improvements to the comprehension of the heliosphere mechanisms. PAMELA is also measuring the radiation environment around the Earth, and has recently discovered an antiproton radiation belt.
Keywords	Physics ; QC1-999 ; Science ; Q
Language	English
Publishing date	2014-04-01T00:00:00Z
Publisher	EDP Sciences
Document type	Article ; Online
Database	BASE - Bielefeld Academic Search Engine (life sciences selection)

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Article ; Online: PAMELA results on the cosmic-ray antiproton flux from 60 MeV to 180 GeV in kinetic energy.

De Pascale, M P / De Santis, C / De Simone, N / Di Felice, V / Galper, A M / Gillard, W / Grishantseva, L / Hofverberg, P / Jerse, G / Karelin, A V / Koldashov, S V / Krutkov, S Y / Kvashnin, A N / Leonov, A / Malvezzi, V / Marcelli, L / Mayorov, A G / Menn, W / Mikhailov, V V / Mocchiutti, E / Monaco, A / Mori, N / Nikonov, N / Osteria, G / Papini, P / Pearce, M / Picozza, P / Pizzolotto, C / Ricci, M / Ricciarini, S B / Rossetto, L / Simon, M / Sparvoli, R / Spillantini, P / Stozhkov, Y I / Vacchi, A / Vannuccini, E / Vasilyev, G / Voronov, S A / Wu, J / Yurkin, Y T / Zampa, G / Zampa, N / Zverev, V G

Physical review letters

2010 Volume 105, Issue 12, Page(s) 121101

Abstract: The satellite-borne experiment PAMELA has been used to make a new measurement of the cosmic-ray antiproton flux and the antiproton-to-proton flux ratio which extends previously published measurements down to 60 MeV and up to 180 GeV in kinetic energy. ... ...

Abstract	The satellite-borne experiment PAMELA has been used to make a new measurement of the cosmic-ray antiproton flux and the antiproton-to-proton flux ratio which extends previously published measurements down to 60 MeV and up to 180 GeV in kinetic energy. During 850 days of data acquisition approximately 1500 antiprotons were observed. The measurements are consistent with purely secondary production of antiprotons in the Galaxy. More precise secondary production models are required for a complete interpretation of the results.
Language	English
Publishing date	2010-09-17
Publishing country	United States
Document type	Journal Article
ZDB-ID	208853-8
ISSN	1079-7114 ; 0031-9007
ISSN (online)	1079-7114
ISSN	0031-9007
DOI	10.1103/PhysRevLett.105.121101
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Article: PAMELA Measurements of Cosmic-Ray Proton and Helium Spectra

Adriani, O / Barbarino, G.C / Bazilevskaya, G.A / Bellotti, R / Boezio, M / Bogomolov, E.A / Bonechi, L / Bongi, M / Bonvicini, V / Borisov, S / Bottai, S / Bruno, A / Cafagna, F / Campana, D / Carbone, R / Carlson, P / Casolino, M / Castellini, G / Consiglio, L /

De Pascale, M.P / De Santis, C / De Simone, N / Di Felice, V / Galper, A.M / Gillard, W / Grishantseva, L / Jerse, G / Karelin, A.V / Koldashov, S.V / Krutkov, S.Y / Kvashnin, A.N / Leonov, A / Malakhov, V / Malvezzi, V / Marcelli, L / Mayorov, A.G / Menn, W / Mikhailov, V.V / Mocchiutti, E / Monaco, A / Mori, N / Nikonov, N / Osteria, G / Palma, F / Papini, P / Pearce, M / Picozza, P / Pizzolotto, C / Ricci, M / Ricciarini, S.B / Rossetto, L / Sarkar, R / Simon, M / Sparvoli, R / Spillantini, P / Stozhkov, Y.I / Vacchi, A / Vannuccini, E / Vasilyev, G / Voronov, S.A / Wu, J / Yurkin, Y.T / Zampa, G / Zampa, N / Zverev, V.G

Science. 2011 Apr. 1, v. 332, no. 6025

2011

Abstract	Protons and helium nuclei are the most abundant components of the cosmic radiation. Precise measurements of their fluxes are needed to understand the acceleration and subsequent propagation of cosmic rays in our Galaxy. We report precision measurements of the proton and helium spectra in the rigidity range 1 gigavolt to 1.2 teravolts performed by the satellite-borne experiment PAMELA (payload for antimatter matter exploration and light-nuclei astrophysics). We find that the spectral shapes of these two species are different and cannot be described well by a single power law. These data challenge the current paradigm of cosmic-ray acceleration in supernova remnants followed by diffusive propagation in the Galaxy. More complex processes of acceleration and propagation of cosmic rays are required to explain the spectral structures observed in our data.
Keywords	data analysis ; helium ; protons ; spectral analysis
Language	English
Dates of publication	2011-0401
Size	p. 69-72.
Publishing place	American Association for the Advancement of Science
Document type	Article
ZDB-ID	128410-1
ISSN	1095-9203 ; 0036-8075
ISSN (online)	1095-9203
ISSN	0036-8075
DOI	10.1126/science.1199172
Database	NAL-Catalogue (AGRICOLA)

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Article ; Online: Observation of Complex Time Structures in the Cosmic-Ray Electron and Positron Fluxes with the Alpha Magnetic Spectrometer on the International Space Station.

Aguilar, M / Cavasonza, L Ali / Ambrosi, G / Arruda, L / Attig, N / Aupetit, S / Azzarello, P / Bachlechner, A / Barao, F / Barrau, A / Barrin, L / Bartoloni, A / Basara, L / Başeğmez-du Pree, S / Battarbee, M / Battiston, R / Becker, U / Behlmann, M / Beischer, B /

Berdugo, J / Bertucci, B / Bindel, K F / Bindi, V / de Boer, W / Bollweg, K / Bonnivard, V / Borgia, B / Boschini, M J / Bourquin, M / Bueno, E F / Burger, J / Cadoux, F / Cai, X D / Capell, M / Caroff, S / Casaus, J / Castellini, G / Cervelli, F / Chae, M J / Chang, Y H / Chen, A I / Chen, G M / Chen, H S / Chen, Y / Cheng, L / Chou, H Y / Choumilov, E / Choutko, V / Chung, C H / Clark, C / Clavero, R / Coignet, G / Consolandi, C / Contin, A / Corti, C / Creus, W / Crispoltoni, M / Cui, Z / Dadzie, K / Dai, Y M / Datta, A / Delgado, C / Della Torre, S / Demirköz, M B / Derome, L / Di Falco, S / Dimiccoli, F / Díaz, C / von Doetinchem, P / Dong, F / Donnini, F / Duranti, M / D'Urso, D / Egorov, A / Eline, A / Eronen, T / Feng, J / Fiandrini, E / Fisher, P / Formato, V / Galaktionov, Y / Gallucci, G / García-López, R J / Gargiulo, C / Gast, H / Gebauer, I / Gervasi, M / Ghelfi, A / Giovacchini, F / Gómez-Coral, D M / Gong, J / Goy, C / Grabski, V / Grandi, D / Graziani, M / Guo, K H / Haino, S / Han, K C / He, Z H / Heil, M / Hsieh, T H / Huang, H / Huang, Z C / Huh, C / Incagli, M / Ionica, M / Jang, W Y / Jia, Yi / Jinchi, H / Kang, S C / Kanishev, K / Khiali, B / Kim, G N / Kim, K S / Kirn, Th / Konak, C / Kounina, O / Kounine, A / Koutsenko, V / Kulemzin, A / La Vacca, G / Laudi, E / Laurenti, G / Lazzizzera, I / Lebedev, A / Lee, H T / Lee, S C / Leluc, C / Li, H S / Li, J Q / Li, Q / Li, T X / Li, Z H / Li, Z Y / Lim, S / Lin, C H / Lipari, P / Lippert, T / Liu, D / Liu, Hu / Lordello, V D / Lu, S Q / Lu, Y S / Luebelsmeyer, K / Luo, F / Luo, J Z / Lyu, S S / Machate, F / Mañá, C / Marín, J / Martin, T / Martínez, G / Masi, N / Maurin, D / Menchaca-Rocha, A / Meng, Q / Mikuni, V M / Mo, D C / Mott, P / Nelson, T / Ni, J Q / Nikonov, N / Nozzoli, F / Oliva, A / Orcinha, M / Palermo, M / Palmonari, F / Palomares, C / Paniccia, M / Pauluzzi, M / Pensotti, S / Perrina, C / Phan, H D / Picot-Clemente, N / Pilo, F / Pizzolotto, C / Plyaskin, V / Pohl, M / Poireau, V / Quadrani, L / Qi, X M / Qin, X / Qu, Z Y / Räihä, T / Rancoita, P G / Rapin, D / Ricol, J S / Rosier-Lees, S / Rozhkov, A / Rozza, D / Sagdeev, R / Schael, S / Schmidt, S M / von Dratzig, A Schulz / Schwering, G / Seo, E S / Shan, B S / Shi, J Y / Siedenburg, T / Son, D / Song, J W / Tacconi, M / Tang, X W / Tang, Z C / Tescaro, D / Ting, Samuel C C / Ting, S M / Tomassetti, N / Torsti, J / Türkoğlu, C / Urban, T / Vagelli, V / Valente, E / Valtonen, E / Vázquez Acosta, M / Vecchi, M / Velasco, M / Vialle, J P / Wang, L Q / Wang, N H / Wang, Q L / Wang, X / Wang, X Q / Wang, Z X / Wei, C C / Weng, Z L / Whitman, K / Wu, H / Wu, X / Xiong, R Q / Xu, W / Yan, Q / Yang, J / Yang, M / Yang, Y / Yi, H / Yu, Y J / Yu, Z Q / Zannoni, M / Zeissler, S / Zhang, C / Zhang, F / Zhang, J / Zhang, J H / Zhang, S W / Zhang, Z / Zheng, Z M / Zhuang, H L / Zhukov, V / Zichichi, A / Zimmermann, N / Zuccon, P

Physical review letters

2018 Volume 121, Issue 5, Page(s) 51102

Abstract: We present high-statistics, precision measurements of the detailed time and energy dependence of the primary cosmic-ray electron flux and positron flux over 79 Bartels rotations from May 2011 to May 2017 in the energy range from 1 to 50 GeV. For the ... ...

Abstract	We present high-statistics, precision measurements of the detailed time and energy dependence of the primary cosmic-ray electron flux and positron flux over 79 Bartels rotations from May 2011 to May 2017 in the energy range from 1 to 50 GeV. For the first time, the charge-sign dependent modulation during solar maximum has been investigated in detail by leptons alone. Based on 23.5×10^{6} events, we report the observation of short-term structures on the timescale of months coincident in both the electron flux and the positron flux. These structures are not visible in the e^{+}/e^{-} flux ratio. The precision measurements across the solar polarity reversal show that the ratio exhibits a smooth transition over 830±30 days from one value to another. The midpoint of the transition shows an energy dependent delay relative to the reversal and changes by 260±30 days from 1 to 6 GeV.
Language	English
Publishing date	2018-08-13
Publishing country	United States
Document type	Journal Article
ZDB-ID	208853-8
ISSN	1079-7114 ; 0031-9007
ISSN (online)	1079-7114
ISSN	0031-9007
DOI	10.1103/PhysRevLett.121.051102
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In stock of ZB MED Bonn / Germany

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In stock of ZB MED Bonn / Germany

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Inter-library loan at ZB MED