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2. Modeling of GERDA Phase II data

Author

GERDA collaboration, Agostini, Matteo, Bakalyarov, Alexander M., Balata, Marco, Barabanov, Igor, Baudis, Laura, Bauer, Christian, Bellotti, Enrico, Belogurov, Sergej, Bettini, Alessandro, Bezrukov, Leonid, Borowicz, Dariusz, Bossio, Elisabetta, Bothe, Vikas, Brudanin, Victor, Brugnera, Riccardo, Caldwell, Allen, Cattadori, Carla, Chernogorov, Andrey, Comellato, Tommaso, D'Andrea, Valerio, Demidova, Elena V., Di Marco, Natalia, Domula, Alexander, Doroshkevich, Evgenyi, Egorov, Viacheslav, Fischer, Felix, Fomina, Maria, Gangapshev, Albert, Garfagnini, Alberto, Gooch, Chris, Grabmayr, Peter, Gurentsov, Valery, Gusev, Konstantin, Hakenmüller, Janina, Hemmer, Sabine, Hiller, Roman, Hofmann, Werner, Hult, Mikael, Inzhechik, Lev V., Csáthy, Jozsef Janicskó, Jochum, Josef, Junker, Matthias, Kazalov, Vladimir, Kermaïdic, Yoann, Kihm, Thomas, Kirpichnikov, Igor V., Klimenko, Alexander, Kneißl, Raphael, Knöpfle, Karl T., Kochetov, Oleg, Kornoukhov, Vasily N., Krause, Patrick, Kuzminov, Valery V., Laubenstein, Matthias, Lazzaro, Andrea, Lindner, Manfred, Lippi, Ivano, Lubashevskiy, Alexey, Lubsandorzhiev, Bayarto, Lutter, Guillaume, Macolino, Carla, Majorovits, Bela, Maneschg, Werner, Miloradovic, Michael, Mingazheva, Rizalina, Misiaszek, Marcin, Moseev, Pavel, Nemchenok, Igor, Panas, Krysztof, Pandola, Luciano, Pelczar, Krysztof, Pertoldi, Luigi, Piseri, Paolo, Pullia, Alberto, Ransom, Chloe, Riboldi, Stefano, Rumyantseva, Nadezda, Sada, Cinzia, Salamida, Francesco, Schönert, Stefan, Schreiner, Jochen, Schütt, Mario, Schütz, Ann-Katrin, Schulz, Oliver, Schwarz, Mario, Schwingenheuer, Bernhard, Selivanenko, Oleg, Shevchik, Egor, Shirchenko, Mark, Simgen, Hardy, Smolnikov, Anatoly, Stukov, Danila, Vanhoefer, Laura, Vasenko, Andrey A., Veresnikova, Anna, Vignoli, Chiara, von Sturm, Katharina, Wester, Thomas, Wiesinger, Christoph, Wojcik, Marcin, Yanovich, Evgeny, Zatschler, Birgit, Zhitnikov, Igor, Zhukov, Sergey V., Zinatulina, Daniya, Zschocke, Andreas, Zsigmond, Anna J., Zuber, Kai, and Zuzel, Grzegorz

Subjects
Nuclear Experiment, Physics - Instrumentation and Detectors
Abstract

The GERmanium Detector Array (GERDA) experiment at the Gran Sasso underground laboratory (LNGS) of INFN is searching for neutrinoless double-beta ($0\nu\beta\beta$) decay of $^{76}$Ge. The technological challenge of GERDA is to operate in a "background-free" regime in the region of interest (ROI) after analysis cuts for the full 100$\,$kg$\cdot$yr target exposure of the experiment. A careful modeling and decomposition of the full-range energy spectrum is essential to predict the shape and composition of events in the ROI around $Q_{\beta\beta}$ for the $0\nu\beta\beta$ search, to extract a precise measurement of the half-life of the double-beta decay mode with neutrinos ($2\nu\beta\beta$) and in order to identify the location of residual impurities. The latter will permit future experiments to build strategies in order to further lower the background and achieve even better sensitivities. In this article the background decomposition prior to analysis cuts is presented for GERDA Phase II. The background model fit yields a flat spectrum in the ROI with a background index (BI) of $16.04^{+0.78}_{-0.85} \cdot 10^{-3}\,$cts/(kg$\cdot$keV$\cdot$yr) for the enriched BEGe data set and $14.68^{+0.47}_{-0.52} \cdot 10^{-3}\,$cts/(kg$\cdot$keV$\cdot$yr) for the enriched coaxial data set. These values are similar to the one of Gerda Phase I despite a much larger number of detectors and hence radioactive hardware components.

Published
2019
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3. Low energy neutron background in deep underground laboratories

Author

Best, Andreas, Gorres, Joachim, Junker, Matthias, Kratz, Karl-Ludwig, Laubenstein, Matthias, Long, Alexander, Nisi, Stefano, Smith, Karl, and Wiescher, Michael

Subjects
Physics - Instrumentation and Detectors, Nuclear Experiment
Abstract

The natural neutron background influences the maximum achievable sensitivity in most deep underground nuclear, astroparticle and double-beta decay physics experiments. Reliable neutron flux numbers are an important ingredient in the design of the shielding of new large-scale experiments as well as in the analysis of experimental data. Using a portable setup of He-3 counters we measured the thermal neutron flux at the Kimballton Underground Research Facility, the Soudan Underground Laboratory, on the 4100 ft and the 4850 ft levels of the Sanford Underground Research Facility, at the Waste Isolation Pilot Plant and at the Gran Sasso National Laboratory. Absolute neutron fluxes at these laboratories are presented., Comment: Preparation version for submission

Published
2015
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6. Shades

Author

Rapagnani David, Ananna Chemseddine, Di Leva Antonino, Imbriani Gianluca, Junker Matthias, Pignatari Marco, and Best Andreas

Subjects
Physics, QC1-999
Abstract

Neutron capture reactions are the main contributors to the synthesis of the heavy elements through the s-process. Together with 13C(α, n)16O, which has recently been measured by the LUNA collaboration in an energy region inside the Gamow peak, 22Ne(α, n)25Mg is the other main neutron source in stars. Its cross section is mostly unknown in the relevant stellar energy (450 keV < Ecm < 750 keV), where only upper limits from direct experiments and highly uncertain estimates from indirect sources exist. The ERC project SHADES (UniNa/INFN) aims to provide for the first time direct cross section data in this region and to reduce the uncertainties of higher energy resonance parameters. High sensitivity measurements will be performed with the new LUNA-MV accelerator at the INFN-LNGS laboratory in Italy: the energy sensitivity of the SHADES hybrid neutron detector, together with the low background environment of the LNGS and the high beam current of the new accelerator promises to improve the sensitivity by over 2 orders of magnitude over the state of the art, allowing to finally probe the unexplored low-energy cross section. Here we present an overview of the project and first results on the setup characterization.

Published
2022
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10. Shades: 22Ne(α, n)25Mg reaction rate in the Gamow window.

Author

Rapagnani, David, Ananna, Chemseddine, Di Leva, Antonino, Imbriani, Gianluca, Junker, Matthias, Pignatari, Marco, and Best, Andreas

Subjects
NEUTRON capture, NUCLEAR physics, ELECTRON accelerators, ACCELERATOR physicists, LABORATORIES
Abstract

Neutron capture reactions are the main contributors to the synthesis of the heavy elements through the s-process. Together with 13C(α, n)16O, which has recently been measured by the LUNA collaboration in an energy region inside the Gamow peak, 22Ne(α, n)25Mg is the other main neutron source in stars. Its cross section is mostly unknown in the relevant stellar energy (450 keV < Ecm < 750 keV), where only upper limits from direct experiments and highly uncertain estimates from indirect sources exist. The ERC project SHADES (UniNa/INFN) aims to provide for the first time direct cross section data in this region and to reduce the uncertainties of higher energy resonance parameters. High sensitivity measurements will be performed with the new LUNA-MV accelerator at the INFN-LNGS laboratory in Italy: the energy sensitivity of the SHADES hybrid neutron detector, together with the low background environment of the LNGS and the high beam current of the new accelerator promises to improve the sensitivity by over 2 orders of magnitude over the state of the art, allowing to finally probe the unexplored low-energy cross section. Here we present an overview of the project and first results on the setup characterization. [ABSTRACT FROM AUTHOR]

Published
2022
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11. 23Na(p,γ)24Mg Cross Section Measurements

Author

Boeltzig Axel, Best Andreas, deBoer Richard J., DiLeva Antonino, Imbriani Gianluca, Junker Matthias, and Wiescher Michael

Subjects
Physics, QC1-999
Abstract

As a link between the NeNa and MgAl cycles in stellar burning, the reaction 23Na(p,γ)24Mg is of interest for various astrophysical scenarios, such as AGB stars. A combined effort at the Laboratory for Underground Nuclear Astrophysics (LUNA) and the Nuclear Science Laboratory (NSL) at the University of Notre Dame aims at a cross section determination for the this reaction, to constrain the astrophysical reaction rate by improving the knowledge of the resonance strengths and the non-resonant component. Experiments at LUNA benefit from the underground location at the Gran Sasso National Laboratory which allows for the measurement of resonances at low energies with high sensitivity in a low background environment. Measurements at the University of Notre Dame pursue a determination of the non-resonant cross section at higher energies. We present the two experiments and the status of the data analysis.

Published
2017
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12. Visual palatability of food in patients with eating disorders and dieting women

Author

Bossert, Sabine, Laessle, Reinhold G., Meiller, Caroline, Junker, Matthias, Ellgring, Heiner, and Pirke, Karl-Martin

Subjects
Eating disorders -- Psychological aspects, Food -- Caloric content, Dieters -- Psychological aspects, Psychology and mental health
Abstract

Summary--The effects of 19 meals of different caloric content on slides on palatability and hypothetical duration of consumption were investigated in 7 patients with anorexia nervosa, 17 patients with bulimia nervosa at the beginning and after 8 weeks of hospital treatment. Nine healthy females served as controls. At the beginning of treatment, palatability of low caloric food was significantly higher and hypothetical duration of consumption of high caloric food was significantly longer in patients when compared to controls. After 8 weeks, in the patients palatability of low caloric food had decreased. Dislike for high caloric food remained stable in anorexics.

Published
1991

13. Improved astrophysical rate for the 18O(p,α)15N reaction by underground measurements

Author

Bruno, Carlo C.G., Aliotta, Marialuisa, Descouvemont, Pierre, Best, Andreas, Davinson, Thomas, Bemmerer, Daniel, Boeltzig, Axel, Broggini, Carlo, Caciolli, Antonio, Cavanna, Francesca, Chillery, Thomas, Ciani, Giacomo G.F., Corvisiero, Pietro, Depalo, Rosanna, Di Leva, Antonino, Elekes, Zoltán, Ferraro, Federico, Formicola, Alba, Fulop, Zsolt, Gervino, Gianpiero, Guglielmetti, Alessandra, Gustavino, Carlo, Gyurky, Gy, Imbriani, Gianluca, Junker, Matthias, Lugaro, Maria, Marigo, Paola, Menegazzo, Roberto, Mossa, Viviana, Pantaleo, Felice F.R., Piatti, D., Prati, Paolo, Stöckel, Klaus, Straniero, Oscar, Strieder, Frank, Szücs, Tamás, Takács, Marcell M.P., Trezzi, Davide, Bruno, Carlo C.G., Aliotta, Marialuisa, Descouvemont, Pierre, Best, Andreas, Davinson, Thomas, Bemmerer, Daniel, Boeltzig, Axel, Broggini, Carlo, Caciolli, Antonio, Cavanna, Francesca, Chillery, Thomas, Ciani, Giacomo G.F., Corvisiero, Pietro, Depalo, Rosanna, Di Leva, Antonino, Elekes, Zoltán, Ferraro, Federico, Formicola, Alba, Fulop, Zsolt, Gervino, Gianpiero, Guglielmetti, Alessandra, Gustavino, Carlo, Gyurky, Gy, Imbriani, Gianluca, Junker, Matthias, Lugaro, Maria, Marigo, Paola, Menegazzo, Roberto, Mossa, Viviana, Pantaleo, Felice F.R., Piatti, D., Prati, Paolo, Stöckel, Klaus, Straniero, Oscar, Strieder, Frank, Szücs, Tamás, Takács, Marcell M.P., and Trezzi, Davide

Abstract

The 18O(p,α)15N reaction affects the synthesis of 15N, 18O and 19F isotopes, whose abundances can be used to probe the nucleosynthesis and mixing processes occurring deep inside asymptotic giant branch (AGB) stars. We performed a low-background direct measurement of the 18O(p,α)15N reaction cross-section at the Laboratory for Underground Nuclear Astrophysics (LUNA) from center of mass energy Ec.m.=340 keV down to Ec.m.=55 keV, the lowest energy measured to date corresponding to a cross-section of less than 1 picobarn/sr. The strength of a key resonance at center of mass energy Er=90 keV was found to be a factor of 10 higher than previously reported. A multi-channel R-matrix analysis of our and other data available in the literature was performed. Over a wide temperature range, T=0.01–1.00 GK, our new astrophysical rate is both more accurate and precise than recent evaluations. Stronger constraints can now be placed on the physical processes controlling nucleosynthesis in AGB stars with interesting consequences on the abundance of 18O in these stars and in stardust grains, specifically on the production sites of oxygen-rich Group II grains., SCOPUS: ar.j, info:eu-repo/semantics/published

Published
2019

16. 23Na(p,γ)24Mg Cross Section Measurements.

Author

deBoer, Richard J., Wiescher, Michael, Boeltzig, Axel, Best, Andreas, DiLeva, Antonino, Imbriani, Gianluca, and Junker, Matthias

Subjects
NUCLEAR cross sections, SODIUM compounds, MAGNESIUM isotopes, NUCLEAR reactions, ASYMPTOTIC giant branch stars, ASTROPHYSICS
Abstract

As a link between the NeNa and MgAl cycles in stellar burning, the reaction 23Na(p,γ)24Mg is of interest for various astrophysical scenarios, such as AGB stars. A combined effort at the Laboratory for Underground Nuclear Astrophysics (LUNA) and the Nuclear Science Laboratory (NSL) at the University of Notre Dame aims at a cross section determination for the this reaction, to constrain the astrophysical reaction rate by improving the knowledge of the resonance strengths and the non-resonant component. Experiments at LUNA benefit from the underground location at the Gran Sasso National Laboratory which allows for the measurement of resonances at low energies with high sensitivity in a low background environment. Measurements at the University of Notre Dame pursue a determination of the non-resonant cross section at higher energies. We present the two experiments and the status of the data analysis. [ABSTRACT FROM AUTHOR]

Published
2017
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17. S-factor of 14N(p,Y)15O at astrophysical energies

Author

Imbriana, G., Costantini, H., Formicola, A., Vomiero, A., Angulo Perez, Carmen, Bemmerer, D., Bonetti, R., Broggini, C., Confortola, F., Corvisiero, P., Cruz, J., Descouvemont, Pierre, Fulop, Zsolt, Gervino, G., Guglielmetti, A., Gustavino, C., Gyurky, Gy, Jesus, A. P., Junker, Matthias, Klug, J. N., Lemut, A., Menegazzo, R., Prati, R., Roca, V., Rolfs, Claus, Romano, M., lvarez, C., Schümann, F., Schürmann, D., Somorjai, Endre, Straniero, O., Strieder, Frank, Terrasi, F., Trauvetter, H. P., Imbriana, G., Costantini, H., Formicola, A., Vomiero, A., Angulo Perez, Carmen, Bemmerer, D., Bonetti, R., Broggini, C., Confortola, F., Corvisiero, P., Cruz, J., Descouvemont, Pierre, Fulop, Zsolt, Gervino, G., Guglielmetti, A., Gustavino, C., Gyurky, Gy, Jesus, A. P., Junker, Matthias, Klug, J. N., Lemut, A., Menegazzo, R., Prati, R., Roca, V., Rolfs, Claus, Romano, M., lvarez, C., Schümann, F., Schürmann, D., Somorjai, Endre, Straniero, O., Strieder, Frank, Terrasi, F., and Trauvetter, H. P.

Abstract

info:eu-repo/semantics/published

Published
2005

18. Astrophysical S-factor of 14N(p,)15O

Author

Formicola, A., Imbriana, G., Costantini, H., Angulo Perez, Carmen, Bemmerer, D., Bonetti, R., Broggini, C., Corvisiero, P., Cruz, J., Descouvemont, Pierre, Fulop, Zsolt, Gervino, G., Guglielmetti, A., Gustavino, C., Gyurky, Gy, Jesus, A. P., Junker, Matthias, Lemut, A., Menegazzo, R., Prati, P., Roca, V., Rolfs, Claus, Romano, M., Alvarez, C., Schumann, F., Somorjai, Endre, Straniero, O., Strieder, Frank, Terrasi, F., Trautvetter, H. P., Vomiero, A., Zavatarelli, Sandra, Formicola, A., Imbriana, G., Costantini, H., Angulo Perez, Carmen, Bemmerer, D., Bonetti, R., Broggini, C., Corvisiero, P., Cruz, J., Descouvemont, Pierre, Fulop, Zsolt, Gervino, G., Guglielmetti, A., Gustavino, C., Gyurky, Gy, Jesus, A. P., Junker, Matthias, Lemut, A., Menegazzo, R., Prati, P., Roca, V., Rolfs, Claus, Romano, M., Alvarez, C., Schumann, F., Somorjai, Endre, Straniero, O., Strieder, Frank, Terrasi, F., Trautvetter, H. P., Vomiero, A., and Zavatarelli, Sandra

Abstract

We report on a new measurement of the 14N(p,γ) 15O capture cross section at Ep=140 to 400 keV using the 400 kV LUNA accelerator facility at the Laboratori Nazionali del Gran Sasso (LNGS). The uncertainties have been reduced with respect to previous measurements and their analysis. We have analyzed the data using the R-matrix method and we find that the ground state transition accounts for about 15% of the total S-factor. The main contribution to the S-factor is given by the transition to the 6.79 MeV state. We find a total S(0)=1.7±0.2 keVb, in agreement with recent extrapolations. The result has important consequences for the solar neutrino spectrum as well as for the age of globular clusters. © 2004 Elsevier B.V. All rights reserved., info:eu-repo/semantics/published

Published
2004

19. Study of the BBN reaction $D(\alpha ,\gamma )^{6}$Li deep underground at LUNA

Author

Erhard, Martin, primary, Anders, Michael, additional, Bellini, Alessandro, additional, Bemmerer, Daniel, additional, Broggini, Carlo, additional, Caciolli, Antonio, additional, Corvisiero, Pietro, additional, Costantini, Heide, additional, Elekes, Zoltan, additional, Formicola, Alba, additional, Fülöp, Zsolt, additional, Gervino, Giampiero, additional, Guglielmetti, Alessandra, additional, Gustavino, Carlo, additional, Gyürky, György, additional, Imbriani, Gianluca, additional, Junker, Matthias, additional, Laubenstein, Matthias, additional, Lemut, Alberto, additional, Marta, Michele, additional, Mazzocchi, Chiara, additional, Menegazzo, Roberto, additional, Prati, Paolo, additional, Rocca, Vincenzo, additional, Rolfs, Claus, additional, Rossi Alvarez, Carlos, additional, Somorjai, Endre, additional, Straniero, Oscar, additional, Strieder, Frank, additional, Szücs, Tamás, additional, Terrasi, Filippe, additional, and Trautvetter, Hans-Peter, additional

Published
2011
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21. Spectroscopic performances of the GERDA cryogenic Charge Sensitive Amplifier based on JFET-CMOS ASIC, coupled to germanium detectors

Author

D'Andragora, Alessio, primary, Cattadori, Carla M., additional, di Vacri, Assunta, additional, Junker, Matthias, additional, Pandola, Luciano, additional, Pullia, Alberto, additional, Riboldi, Stefano, additional, Zocca, Francesca, additional, Heider, Marik Barnabe, additional, Budjas, Dusan, additional, Kiko, Jurgen, additional, Schonert, Stefan, additional, Gusev, Konstantin, additional, and Majorovits, Bela, additional

Published
2009
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23. Cross section measurments of nuclear reactions relevant to the astrophysical p-process

Author

Somorjai, Endre, Fulop, Zsolt, Kiss, A.Z., Rolfs, Claus, Trautvetter, H. P., Greife, Uwe, Junker, Matthias, Rauscher, Thomas, Oberhummer, Heinz, Arnould, Marcel, Rayet, Marc, Goriely, Stéphane, Somorjai, Endre, Fulop, Zsolt, Kiss, A.Z., Rolfs, Claus, Trautvetter, H. P., Greife, Uwe, Junker, Matthias, Rauscher, Thomas, Oberhummer, Heinz, Arnould, Marcel, Rayet, Marc, and Goriely, Stéphane

Abstract

info:eu-repo/semantics/published

Published
1998

24. Radiative capture experiments for the p-process and comparison to statistical calculations

Author

Somorjai, Endre, Fulop, Zsolt, Kiss, A.Z., Rolfs, C.E., Trautvetter, H. P., Greife, Uwe, Junker, Matthias, Arnould, Marcel, Rayet, Marc, Goriely, Stéphane, Rauscher, Thomas, Oberhummer, Heinz, Mohr, Peter, Somorjai, Endre, Fulop, Zsolt, Kiss, A.Z., Rolfs, C.E., Trautvetter, H. P., Greife, Uwe, Junker, Matthias, Arnould, Marcel, Rayet, Marc, Goriely, Stéphane, Rauscher, Thomas, Oberhummer, Heinz, and Mohr, Peter

Abstract

info:eu-repo/semantics/published

Published
1998

25. LUNA: An underground accelerator facility for nuclear astrophysics.

Author

Junker, Matthias

Subjects
*NUCLEAR astrophysics, *ACCELERATOR mass spectrometry
Abstract

The contribution focuses on the 400 kV accelerator which will be installed in the underground laboratory of the Laboratori Nazionali del Gran Sasso (Italy) in the year 2000. Special emphasis will bes put on the properties of the accelerator and the gamma detector systems giving high detection efficiency and low background. © 2000 American Institute of Physics. [ABSTRACT FROM AUTHOR]

Published
2000

29. Fission Properties Relevant for GW170817

Author

Mumpower, M. R., Vassh, N., Sprouse, T., Jaffke, P., Kawano, T., Holmbeck, E., Zhu, Y. L., Surman, R., McLaughlin, G. C., Möller, P., Formicola, Alba, editor, Junker, Matthias, editor, Gialanella, Lucio, editor, and Imbriani, Gianluca, editor

Published
2019
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31. Nuclear Astrophysics Underground: Status and Future

Author

Strieder, Frank, Robertson, Daniel, Boeltzig, Axel, Borgwardt, Tyler, Couder, Manoel, Frentz, Bryce, Greife, Uwe, Goerres, Joachim, Hanhardt, Mark, Kadlecek, Thomas, Wiescher, Michael, Formicola, Alba, editor, Junker, Matthias, editor, Gialanella, Lucio, editor, and Imbriani, Gianluca, editor

Published
2019
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34. Investigation of Neutron-Induced Reaction at the Goethe University Frankfurt

Author

Reifarth, René, Bott, Lukas, Brückner, Benjamin, Dogan, Ozan, Dworac, Markus, Endres, Anne, Erbacher, Philipp, Fiebiger, Stefan, Gernhäuser, Roman, Göbel, Kathrin, Hebermehl, Fabian, Heftrich, Tanja, Langer, Christoph, Kausch, Tanja, Klapper, Nadine, Khasawneh, Kafa, Köppchen, Christoph, Krasilovskaja, Sabina, Kurtulgil, Deniz, Reich, Markus, Schöffler, Markus S., Schmidt, Lothar Ph. H., Schwarz, Christian, Slavkovská, Zuzana, Stiebing, Kurt E., Thomas, Benedikt, Volknandt, Meiko, Weigand, Mario, Wiescher, Michael, Ziel, Patric, Formicola, Alba, editor, Junker, Matthias, editor, Gialanella, Lucio, editor, and Imbriani, Gianluca, editor

Published
2019
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39. Experimental Study of the Reaction in Classical Novae

Author

Meyer, A., de Séréville, N., Hammache, F., Adsley, P., Parikh, A., Assié, M., Assunção, M., Bastin, B., Beaumel, D., Béroff, K., Coc, Alain, D’Agata, G., Delafosse, C., De Oliveira, F., Flavigny, F., Fox, S. P., Georgiadou, A., Gottardo, A., Grassi, L., Guillot, J., Guimaräes, V., Hubbard, N., Id Barkach, T., Kiener, J., Laird, A. M., Lara, A. L., MacCormick, M., Matea, I., Olivier, L., Oulebsir, N., Perrot, L., Portail, C., Riley, J., Benítez, Á. M. Sánchez, Stefan, I., Tatischeff, V., Formicola, Alba, editor, Junker, Matthias, editor, Gialanella, Lucio, editor, and Imbriani, Gianluca, editor

Published
2019
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47. Neutrinos from Presupernova Stars

Author

Yoshida, Takashi, Takahashi, Koh, Umeda, Hideyuki, Ishidoshiro, Koji, Formicola, Alba, editor, Junker, Matthias, editor, Gialanella, Lucio, editor, and Imbriani, Gianluca, editor

Published
2019
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50. Axions and the Final Fate of Stars

Author

Domínguez, I., Straniero, Oscar, Giannotti, M., Mirizzi, A., Formicola, Alba, editor, Junker, Matthias, editor, Gialanella, Lucio, editor, and Imbriani, Gianluca, editor

Published
2019
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