P. Figuera - List of publications at the Cyclotron Institute, Texas A&M University

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First name(s):	P.
Last name(s):	Figuera

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.

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]

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]

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]

Strong Resonances at High Excitation Energy in $^{17}\mathrm{O}+$ Alpha Resonance Scattering, D. K. Nauruzbayev, A. K. Nurmukhanbetova, V. Z. Goldberg, M. La Cognata, A. Di Pietro, P. Figuera, S. Cherubini, M. Gulino, L. Lamia, R. G. Pizzone, R. Spartá, A. Tumino, A. Serikov and E. M. Gazeeva, in: LXIX Nucleus 2019: Fundamental Problems of Nuclear Physics, Nuclei at Borders of Nucleon Stability, High Technologies, Physics of Atomic Nuclei 83, Dubna, Russia, pages 520--522, Pleiades Publishing Ltd, 2020

pub id: 1161 [DOI] [URL]

$^{19}\mathrm{F}$ spectroscopy and implications for astrophysics, M. La Cognata, M. Fisichella, A. Di Pietro, P. Figuera, V. Z. Goldberg, S. Cherubini, J. P. Fernández Garcia, M. Gulino, L. Lamia, D. Lattuada, M. Lattuada, R. G. Pizzone, G. G. Rapisarda, S. Romano, R. Spartá, C. Spitaleri, D. Torresi, A. Tumino and M. Zadro, in: Nuclear Physics in Astrophysics IX, Journal of Physics: Conference Series 1668, Frankfurt, Germany, pages 012023, {IOP} Publishing, 2020

pub id: 1159 [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]

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]

Observation of $^{15}\mathrm{N}+\alpha$ resonant structures in $^{19}\mathrm{F}$ using the thick target in inverse kinematics scattering method, M. La Cognata, M. Fisichella, A. Pietro Di, P. Figuera, V. Z. Goldberg, S. Cherubini, J. P. Fernández Garcia, M. Gulino, L. Lamia, D. Lattuada, M. Lattuada, R. G. Pizzone, G. G. Rapisarda, S. Romano, R. Spartá, C. Spitaleri, D. Torresi, A. Tumino and M. Zadro, Phys. Rev. C 99, 034301 (2019)

pub id: 927 [DOI] [URL]

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