G. G. Kiss - List of publications at the Cyclotron Institute, Texas A&M University

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First name(s):	G. G.
Last name(s):	Kiss
Institute:	Istituto Nazionale di Fisica Nucleare

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.

Measurement of the $-3~\mathrm{keV}$ Resonance in the Reaction $^{13}\mathrm{C}(\alpha,n)^{16}\mathrm{O}$ of Importance in the $s$-Process, M. La Cognata, C. Spitaleri, O. Trippella, G. G. Kiss, G. V. Rogachev^*, A. M. Mukhamedzhanov^*, M. Avila, G. L. Guardo, E. Koshchiy, A. Kuchera, L. Lamia, S. M. R. Puglia, S. Romano, D. Santiago and R. Spartá, Phys. Rev. Lett. 109, 232701 (2012)

pub id: 327 [DOI] [URL]

Measurement of the $^{13}\mathrm{C}(\alpha, n)^{16}\mathrm{O}$ reaction at astrophysical energies using the Trojan Horse Method. Focus on the $-3~\mathrm{keV}$ sub-threshold resonance, M. La Cognata, C. Spitaleri, O. Trippella, G. G. Kiss, G. V. Rogachev^*, A. M. Mukhamedzhanov^*, M. L. Avila, G. L. Guardo, E. Koshchiy, A. N. Kuchera, L. Lamia, S. M. R. Puglia, S. Romano, D. Santiago-Gonzalez and R. Spartá, in: INPC 2013 – International Nuclear Physics Conference, EPJ Web of Conferences 66, EDP Sciences, Firenze, Italy, pages 07010, 2014

pub id: 155 [DOI] [URL]

Measurement of the 20 and 90~keV Resonances in the $^{18}\mathrm{O}(p,\alpha)^{15}\mathrm{N}$ Reaction via the Trojan Horse Method, M. La Cognata, C. Spitaleri, A. M. Mukhamedzhanov^*, B. Irgaziev, R. E. Tribble, A. Banu, S. Cherubini, A. Coc, V. Crucillà, V. Z. Goldberg, M. Gulino, G. G. Kiss, L. Lamia, J. Mrazek, R. G. Pizzone, S. M. R. Puglia, G. G. Rapisarda, S. Romano, M. L. Sergi, G. Tabacaru, L. Trache, W. Trzaska and A. Tumino, Phys. Rev. Lett. 101, 152501 (2008)

pub id: 82 [DOI] [URL]

On the Measurement of the $^{13}\mathrm{C}(\alpha, n)^{16}\mathrm{O}$ ${S}$-factor at Negative Energies and its Influence on the $s$-process, M. La Cognata, C. Spitaleri, O. Trippella, G. G. Kiss, G. V. Rogachev^*, A. M. Mukhamedzhanov^*, M. Avila, G. L. Guardo, E. Koshchiy, A. Kuchera, L. Lamia, S. M. R. Puglia, S. Romano, D. Santiago and R. Spartá, The Astrophysical Journal 777, 143 (2013)

pub id: 316 [DOI] [URL]

Reaction rate of the $^{13}\mathrm{C}(\alpha,n)^{16}\mathrm{O}$ neutron source using the ANC of the $-3~\mathrm{keV}$ resonance measured with the THM, M. La Cognata, C. Spitaleri, O. Trippella, G. G. Kiss, G. V. Rogachev^*, A. M. Mukhamedzhanov^*, M. Avila, G. L. Guardo, E. Koshchiy, A. Kuchera, L. Lamia, S. M. R. Puglia, S. Romano, D. Santiago and R. Spartá, in: Nuclear Physics in Astrophysics VI (NPA6), Journal of Physics: Conference Series 665, Lisbon, Portugal, pages 012013, 2016

pub id: 516 [DOI] [URL]

THM determination of the 65~keV resonance strength intervening in the $^{17}\mathrm{O}(p,\alpha)^{14}\mathrm{N}$ reaction rate, M. L. Sergi, C. Spitaleri, S. V. Burjan, S. Cherubini, A. Coc, M. Gulino, F. Hammache, Z. Hons, B. Irgaziev, G. G. Kiss, V. Kroha, M. La Cognata, L. Lamia, A. M. Mukhamedzhanov^*, R. G. Pizzone, S. M. R. Puglia, G. G. Rapisarda, S. Romano, N. de Séréville, E. Somorjai and A. Tumino, in: Exotic Nuclei and Nuclear/Particle Astrophysics (V). from Nuclei to Stars: Carpathian Summer School of Physics 2014, AIP Conference Proceedings 1645, Sinaia, Romania, pages 392-396, 2015

pub id: 188 [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]

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]

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]

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