S. Palmerini - List of publications at the Cyclotron Institute, Texas A&M University

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First name(s):	S.
Last name(s):	Palmerini

Authors associated with the Cyclotron Institute are underlined, and those associated with Center of Excellence in Nuclear Training And University-based Research (CENTAUR) have a ^* next to their name.

Neutron enhancement from laser interaction with a critical fluid, H. J. Quevedo, G. Zhang, A. Bonasera^*, M. Donovan, G. Dyer, E. Gaul, G. L. Guardo, M. Gulino, M. La Cognata, D. Lattuada, S. Palmerini, R. G. Pizzone, S. Romano, H. Smith, O. Trippella, A. Anzalone, C. Spitaleri and T. Ditmire, Physics Letters A 382, 94--98 (2018)

pub id: 785 [DOI] [URL]

Range of plasma ions in cold cluster gases near the critical point, G. Zhang, H. J. Quevedo, A. Bonasera^*, M. Donovan, G. Dyer, E. Gaul, G. L. Guardo, M. Gulino, M. La Cognata, D. Lattuada, S. Palmerini, R. G. Pizzone, S. Romano, H. Smith, O. Trippella, A. Anzalone, C. Spitaleri and T. Ditmire, Physics Letters A 381, 1682 - 1686 (2017)

pub id: 643 [DOI] [URL]

Updated THM Astrophysical Factor of the $^{19}\mathrm{F}(p,\alpha)^{16}\mathrm{O}$ Reaction and Influence of New Direct Data at Astrophysical Energies, M. La Cognata, S. Palmerini, C. Spitaleri, I. Indelicato, A. M. Mukhamedzhanov^*, I. Lombardo and O. Trippella, The Astrophysical Journal 805, 128 (2015)

pub id: 186 [DOI] [URL]

Progress on nuclear reaction rates affecting the stellar production of $^{26}\mathrm{Al}$, A. M. Laird, M. Lugaro, A. Kankainen, P. Adsley^*, D. W. Bardayan, H. E. Brinkman, B. Côté, C. M. Deibel, R. Diehl, F. Hammache, J. W. den Hartogh, J. José, D. Kurtulgil, C. Lederer-Woods, G. Lotay, G. Meynet, S. Palmerini, M. Pignatari, R. Reifarth, N. de Séréville, A. Sieverding, R. J. Stancliffe, T. C. L. Trueman, T. Lawson, J. S. Vink, C. Massimi and A. Mengoni, Journal of Physics G: Nuclear and Particle Physics 50, 033002 (2023)

pub id: 1298 [DOI] [URL]

Radioisotope production using lasers: From basic science to applications, M. R. D. Rodrigues, A. Bonasera^*, M. Scisciò, J. A. Pérez-Hernández, M. Ehret, F. Filippi, P. L. Andreoli, M. Huault, H. Larreur, D. Singappuli, D. Molloy, D. Raffestin, M. Alonzo, G. G. Rapisarda, D. Lattuada, G. L. Guardo, C. Verona, Fe. Consoli, G. Petringa, A. McNamee, M. La Cognata, S. Palmerini, T. Carriere, M. Cipriani, G. Di Giorgio, G. Cristofari, R. De Angelis, G. A. P. Cirrone, D. Margarone, L. Giuffrida, D. Batani, P. Nicolai, K. Batani, R. Lera, L. Volpe, D. Giulietti, S. Agarwal, M. Krupka, S. Singh and Fa. Consoli, Matter and Radiation at Extremes 9, 037203 (2024)

pub id: 1360 [DOI] [URL]

Searching for resonance states in $^{22}\mathrm{Ne}(p,\gamma)^{23}\mathrm{Na}$, D. P. Carrasco-Rojas, M. Williams, P. Adsley^*, L. Lamia, B. Bastin, T. Faestermann, C. Fougères, F. Hammache, D. S. Harrouz, R. Hertenberger, M. La Cognata, A. Meyer, F. de Oliveira Santos, S. Palmerini, R. G. Pizzone, S. Romano, N. de Séréville, A. Tumino and H. -F. Wirth, Phys. Rev. C 108, 045802 (2023)

pub id: 1350 [DOI] [URL]

Experimental study of the $^{30}\mathrm{Si}(^3\mathrm{He},d)^{31}\mathrm{P}$ reaction and thermonuclear reaction rate of $^{30}\mathrm{Si}(p,\gamma)^{31}\mathrm{P}$, D. S. Harrouz, N. de Séréville, P. Adsley^*, F. Hammache, R. Longland, B. Bastin, T. Faestermann, R. Hertenberger, M. La Cognata, L. Lamia, A. Meyer, S. Palmerini, R. G. Pizzone, S. Romano, A. Tumino and H. -F. Wirth, Phys. Rev. C 105, 015805 (2022)

pub id: 1195 [DOI] [URL]

Indirect determination of the astrophysical $S$ factor for the $^6\mathrm{Li}(p,\gamma)^7\mathrm{Be}$ reaction using the asymptotic normalization coefficient method, G. G. Kiss, M. La Cognata, R. Yarmukhamedov, K. I. Tursunmakhatov, I. Wiedenhöver^*, L. T. Baby, S. Cherubini, A. Cvetinović, G. D'Agata, P. Figuera, G. L. Guardo, M. Gulino, S. Hayakawa, I. Indelicato, L. Lamia, M. Lattuada, F. Mudò, S. Palmerini, R. G. Pizzone, G. G. Rapisarda, S. Romano, M. L. Sergi, R. Spartá, C. Spitaleri, O. Trippella, A. Tumino, M. Anastasiou, S. A. Kuvin, N. Rijal, B. Schmidt, S. B. Igamov, S. B. Sakuta, Zs. Fülöp, Gy. Gyürky, T. Szücs, Z. Halász, E. Somorjai, Z. Hons, J. Mrazek, R. E. Tribble and A. M. Mukhamedzhanov^*, Phys. Rev. C 104, 015807 (2021)

pub id: 1142 [DOI] [URL]

Experimental Determination of $\alpha$ Widths of $^{21}\mathrm{Ne}$ Levels in the Region of Astrophysical Interest: New $^{17}\mathrm{O}+\alpha$ Reaction Rates and Impact on the Weak $s$ Process, F. Hammache, P. Adsley^*, L. Lamia, D. S. Harrouz, N. de Séréville, B. Bastin, A. Choplin, T. Faestermann, C. Fougères, R. Hertenberger, R. Hirschi, M. La Cognata, A. Meyer, S. Palmerini, R. G. Pizzone, F. de Oliveira Santos, S. Romano, A. Tumino and H. -F. Wirth, Phys. Rev. Lett. 132, 182701 (2024)

pub id: 1379 [DOI] [URL]

Exploring the astrophysical energy range of the $^{27}\mathrm{Al}(p,\alpha)^{24}\mathrm{Mg}$ reaction: A new recommended reaction rate, M. La Cognata, S. Palmerini, P. Adsley^*, F. Hammache, A. Di Pietro, P. Figuera, R. Alba, S. Cherubini, F. Dell'Agli, G. L. Guardo, M. Gulino, L. Lamia, D. Lattuada, C. Maiolino, A. Oliva, R. G. Pizzone, P. M. Prajapati, S. Romano, D. Santonocito, R. Spartá, M. L. Sergi and A. Tumino, Physics Letters B 826, 136917 (2022)

pub id: 1207 [DOI] [URL]

Astrophysical $S$-factor for the $^3\mathrm{He}(\alpha,\gamma)^7\mathrm{Be}$ reaction via the asymptotic normalization coefficient ({ANC}) method, G. G. Kiss, M. La Cognata, C. Spitaleri, R. Yarmukhamedov, I. Wiedenhöver^*, L. T. Baby, S. Cherubini, A. Cvetinović, G. D'Agata, P. Figuera, G. L. Guardo, M. Gulino, S. Hayakawa, I. Indelicato, L. Lamia, M. Lattuada, F. Mudò, S. Palmerini, R. G. Pizzone, G. G. Rapisarda, S. Romano, M. L. Sergi, R. Spartá, O. Trippella, A. Tumino, M. Anastasiou, S. A. Kuvin, N. Rijal, B. Schmidt, S. B. Igamov, S. B. Sakuta, K. I. Tursunmakhatov, Zs. Fülöp, Gy. Gyürky, T. Szücs, Z. Halász, E. Somorjai, Z. Hons, J. Mrazek, R. E. Tribble and A. M. Mukhamedzhanov^*, Physics Letters B 807, 135606 (2020)

pub id: 1040 [DOI] [URL]

A New Reaction Rate of the $^{27}\mathrm{Al}(p/\alpha)^{24}\mathrm{Mg}$ Reaction Based on Indirect Measurements at Astrophysical Energies and Implications for $^{27}\mathrm{Al}$ Yields of Intermediate-mass Stars, M. La Cognata, S. Palmerini, P. Adsley^*, F. Hammache, A. Di Pietro, P. Figuera, F. Dell'Agli, R. Alba, S. Cherubini, G. L. Guardo, M. Gulino, L. Lamia, D. Lattuada, C. Maiolino, A. Oliva, R. G. Pizzone, P. M. Prajapati, G. G. Rapisarda, S. Romano, D. Santonocito, R. Spartá, M. L. Sergi, A. Tumino and P. Ventura, The Astrophysical Journal 941, 96 (2022)

pub id: 1307 [DOI] [URL]

Determination of the astrophysical factor of the $^3\mathrm{He}(\alpha,\gamma)^7\mathrm{Be}$ down to zero energy using the asymptotic normalization coefficient method, M. La Cognata, G. G. Kiss, R. Yarmukhamedov, K. I. Tursunmakhatov, I. Wiedenhöver^*, L. T. Baby, S. Cherubini, A. Cvetinović, G. D'Agata, P. Figuera, G. L. Guardo, M. Gulino, S. Hayakawa, I. Indelicato, L. Lamia, M. Lattuada, F. Mudò, S. Palmerini, R. G. Pizzone, G. G. Rapisarda, S. Romano, M. L. Sergi, R. Spartá, C. Spitaleri, O. Trippella, A. Tumino, M. Anastasiou, S. A. Kuvin, N. Rijal, B. Schmidt, S. B. Igamov, S. B. Sakuta, Zs. Fülöp, Gy. Gyürky, T. Szücs, Z. Halász, E. Somorjai, Z. Hons, J. Mrazek, R. E. Tribble and A. M. Mukhamedzhanov^*, in: 28th International Nuclear Physics Conference (INPC 2022), Journal of Physics: Conference Series 2586, Cape Town South Africa, pages 012093, {IOP} Publishing, 2023

pub id: 1337 [DOI] [URL]

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