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51. Massa 2022 - Book of Abstracts

Author

Di Francesco, G., Croce, M., Vincenti, F., Montesano, C., Sergi, M., and Curini, R.

Subjects
Suspect Screening, Novel Psychoactive Substances, Mass Spectrometry, Suspect Screening, Novel Psychoactive Substances, Mass Spectrometry
Published
2022

56. Study of the neutron-induced reaction 17O(n,α)14C at astrophysical energies via the Trojan Horse method

Author

Oliva A. A., Guardo G. L., Lamia L., Cherubini S., Cvetinovic A., D'Agata G., de Sereville N., Di Pietro A., Figuera P., Gulino M., Hammache F., Hayakawa S., Indelicato I., la Cognata M., la Commara M., Lattuada D., Lattuada M., Manico G., Mazzocco M., Messina S., Palmerini S., Pizzone R. G., Pumo M. L., Rapisarda G. G., Romano S., Sergi M. L., Soic N., Sparta R., Spitaleri C., Tumino A., Oliva, A. A., Guardo, G. L., Lamia, L., Cherubini, S., Cvetinovic, A., D'Agata, G., de Sereville, N., Di Pietro, A., Figuera, P., Gulino, M., Hammache, F., Hayakawa, S., Indelicato, I., la Cognata, M., la Commara, M., Lattuada, D., Lattuada, M., Manico, G., Mazzocco, M., Messina, S., Palmerini, S., Pizzone, R. G., Pumo, M. L., Rapisarda, G. G., Romano, S., Sergi, M. L., Soic, N., Sparta, R., Spitaleri, C., and Tumino, A.

Abstract

Stellar nucleosynthesis processes are of vital importance for nuclear physics: all the heavy elements are created by neutron capture reactions that take place in stars. To correctly study such reactions the neutron abundance available in the environment must be known, which means that also the so-called “neutron poisons” must be considered. The present work will focus on the reaction 17O(n,α)14C which removes neutrons from the stellar environment during the s-process. Even though the study of such reactions is of high interest, it still presents several technological problems regarding both the creation and characterization of the neutron beam and the radioprotection of the facility. Therefore, the Trojan Horse Method, an indirect method, has been chosen to study the 17O(n, α)14C reaction in the energy region of astrophysical interest, from 300 keV in the center-of-mass frame down to zero. In the present work, after briefly recalling the main features of the method and reporting on the state of the art for the reaction cross-section measurements, the latest THM experiment will be presented.

Published
2020

57. Indirect measurement of the 3He (n,p) 3H reaction cross section at Big Bang energies

Author

Pizzone R. G., Spampinato C., Sparta R., Couder M., Tan W., Burjan V., D'Agata G., Guardo G. L., La Cognata M., Lamia L., Mrazek J., Palmerini S., Typel S., Tumino A., Wiescher M., Anguilar S., Bardayan D., Blankstein D., Boccioli L., Callahan L., Cha S. M., Chae K. Y., Clark A. M., Frentz B., Hall M. R., Gula A., Henderson S., Kelmar R., Kwag M. S., Indelicato I., La Commara M., Lattuada D., Liu Q., Long J., Mazzocco M., Majumdar A., McGuinness S., Nelson A., Oliva A. A., O'Malley P., Prajapati P. M., Rapisarda G. G., Romano S., Sergi M. L., Seymour C., Skulski M., Spitaleri C., Wilkinson J., Pizzone, R. G., Spampinato, C., Sparta, R., Couder, M., Tan, W., Burjan, V., D'Agata, G., Guardo, G. L., La Cognata, M., Lamia, L., Mrazek, J., Palmerini, S., Typel, S., Tumino, A., Wiescher, M., Anguilar, S., Bardayan, D., Blankstein, D., Boccioli, L., Callahan, L., Cha, S. M., Chae, K. Y., Clark, A. M., Frentz, B., Hall, M. R., Gula, A., Henderson, S., Kelmar, R., Kwag, M. S., Indelicato, I., La Commara, M., Lattuada, D., Liu, Q., Long, J., Mazzocco, M., Majumdar, A., Mcguinness, S., Nelson, A., Oliva, A. A., O'Malley, P., Prajapati, P. M., Rapisarda, G. G., Romano, S., Sergi, M. L., Seymour, C., Skulski, M., Spitaleri, C., and Wilkinson, J.

Abstract

Nuclear reactions play a key role in the framework of the Big Bang Nucleosynthesis. A network of 12 principal reactions has been identified as the main path that drove the elemental nucleosynthesis in the first 20 min of the history of the Universe. Among them an important role is played by neutron-induced reactions, which, from an experimental point of view, are usually a difficult task to be measured directly. Nevertheless big efforts in the last decades have led to a better understanding of their role in the primordial nucleosynthesis network. In this work we apply the Trojan Horse Method to extract the cross section at astrophysical energies for the 3He (n,p)3H reaction after a detailed study of the 2H (3He ,pt)H three-body process. Data extracted from the present measurement are compared with other published sets.

Published
2020

58. The $$^{27}\hbox {Al}(\hbox {p},\alpha )^{24}\hbox {Mg}$$ reaction at astrophysical energies studied by means of the Trojan Horse Method applied to the $$^2\hbox {H}(^{27}\hbox {Al},\alpha ^{24}\hbox {Mg})\hbox {n}$$ reaction

Author

Palmerini, S., primary, La Cognata, M., additional, Hammache, F., additional, Acosta, L., additional, Alba, R., additional, Burjan, V., additional, Chávez, E., additional, Cherubini, S., additional, Cvetinović, A., additional, D’Agata, G., additional, de Séréville, N., additional, Di Pietro, A., additional, Figuera, P., additional, Fülöp, Z., additional, Gaitán De Los Rios, K., additional, Guardo, G. L., additional, Gulino, M., additional, Hayakawa, S., additional, Kiss, G. G., additional, La Commara, M., additional, Lamia, L., additional, Maiolino, C., additional, Manicó, G., additional, Matei, C., additional, Mazzocco, M., additional, Mrazek, J., additional, Parascandolo, T., additional, Petruse, T., additional, Pierroutsakou, D., additional, Pizzone, R. G., additional, Rapisarda, G. G., additional, Romano, S., additional, Santonocito, D., additional, Sergi, M. L., additional, Spartà, R., additional, Tumino, A., additional, and Yamaguchi, H., additional

Published
2021
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60. Nuclear reactions in AGB nucleosynthesis: the 19F(α, p)22Ne at energies of astrophysical relevance

Author

D’Agata G., Pizzone R. G., La Cognata M., Indelicato I., Spitaleri C., Blagus S., Cherubini S., Figuera P., Grassi L., Guardo G. L., Gulino M., Hayakawa S., Kshetri R., Lamia L., Lattuada M., Mijatović T., Milin M., Miljanić Ð., Prepolec L., Rapisarda G. G., Romano S., Sergi M. L., Soić N., Tokić V., Tumino A., and Uroić M.

Subjects
Physics, QC1-999
Abstract

The abundance of 19F in the universe is strictly related to standard and extra-mixing processes taking place inside AGB-stars, that are considered to be the most important sites for its production. Nevertheless the way in which it is destroyed is far from being well understood. For this reason we studied the 19F(α,p)22Ne reaction, that is supposed to be the main destruction channel in the Helium-rich part of the star. In this experiment, the reaction has been studied in the energy range of relevance for astrophysics (0÷1 MeV) via the Trojan Horse Method (THM), using the three-body reaction 6Li(19F,p22Ne)d.

Published
2017
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61. The Trojan Horse Method application on the 10B(p,α0)7Be reaction cross section measurements

Author

Cvetinović A., Spitaleri C., Spartá R., Rapisarda G. G., Puglia S. M., La Cognata M., Cherubini S., Guardo G. L., Gulino M., Lamia L., Pizzone R. G., Romano S., and Sergi M. L.

Subjects
Physics, QC1-999
Abstract

The 10B(p,α0)7Be reaction cross section has been measured in an wide energy range from 2.2 MeV down to 3 keV in a single experiment applying THM. Optimized experimental set-up ensured good energy resolution leading to a good separation of α0 and α1 contributions to the cross section coming from the 7Be ground and first excited state, respectively.

Published
2017
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63. Indirect determination of the astrophysical S factor for the Li6 ( p,γ)Be7 reaction using the asymptotic normalization coefficient method

Author

Kiss, G. G., primary, La Cognata, M., additional, Yarmukhamedov, R., additional, Tursunmakhatov, K. I., additional, Wiedenhöver, I., additional, Baby, L. T., additional, Cherubini, S., additional, Cvetinović, A., additional, D'Agata, G., additional, Figuera, P., additional, Guardo, G. L., additional, Gulino, M., additional, Hayakawa, S., additional, Indelicato, I., additional, Lamia, L., additional, Lattuada, M., additional, Mudò, F., additional, Palmerini, S., additional, Pizzone, R. G., additional, Rapisarda, G. G., additional, Romano, S., additional, Sergi, M. L., additional, Spartà, R., additional, Spitaleri, C., additional, Trippella, O., additional, Tumino, A., additional, Anastasiou, M., additional, Kuvin, S. A., additional, Rijal, N., additional, Schmidt, B., additional, Igamov, S. B., additional, Sakuta, S. B., additional, Fülöp, Zs., additional, Gyürky, Gy., additional, Szücs, T., additional, Halász, Z., additional, Somorjai, E., additional, Hons, Z., additional, Mrázek, J., additional, Tribble, R. E., additional, and Mukhamedzhanov, A. M., additional

Published
2021
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64. $$^{10}$$B(n,$$\alpha _{0}$$)$$^{7}$$Li and $$^{10}$$B(n,$$\alpha _{1}$$)$$^{7}$$Li reactions measured via Trojan Horse Method

Author

Spartà, R., primary, Lamia, L., additional, La Cognata, M., additional, Spitaleri, C., additional, Rapisarda, G. G., additional, Guardo, G. L., additional, Cherubini, S., additional, D’Agata, G., additional, Di Pietro, A., additional, Figuera, P., additional, Gulino, M., additional, Lattuada, D., additional, Lattuada, M., additional, Palmerini, S., additional, Pizzone, R. G., additional, Romano, S., additional, Sergi, M. L., additional, Tumino, A., additional, and Typel, S., additional

Published
2021
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65. The 27Al (p , α) 24Mg reaction at astrophysical energies studied by means of the Trojan Horse Method applied to the 2H (27Al , α24Mg) n reaction

Author

Palmerini, S., La Cognata, M., Hammache, F., Acosta, L., Alba, R., Burjan, V., Chavez, E., Cherubini, S., Cvetinovic, A., D'Agata, G., de Sereville, N., Di Pietro, A., Figuera, P., Fulop, Z., Gaitan De Los Rios, K., Guardo, G. L., Gulino, M., Hayakawa, S., Kiss, G. G., La Commara, M., Lamia, L., Maiolino, C., Manico, G., Matei, C., Mazzocco, M., Mrazek, J., Parascandolo, T., Petruse, T., Pierroutsakou, D., Pizzone, R. G., Rapisarda, G. G., Romano, S., Santonocito, D., Sergi, M. L., Sparta, R., Tumino, A., and Yamaguchi, H.

Published
2021

67. The Al-27(p, alpha)Mg-24 reaction at astrophysical energies studied by means of the Trojan Horse Method applied to the H-2(Al-27, alpha Mg-24)n reaction

Author

Palmerini, S., La Cognata, M., Hammache, F., Acosta, L., Alba, R., Burjan, V., Chávez, E., Cherubini, S., Cvetinović, A., D’Agata, G., de Séréville, N., Di Pietro, A., Figuera, P., Fülöp, Z., Gaitán De Los Rios, K., Guardo, G. L., Gulino, M., Hayakawa, S., Kiss, G. G., La Commara, M., Lamia, L., Maiolino, C., Manicó, G., Matei, C., Mazzocco, M., Mrazek, J., Parascandolo, T., Petruse, T., Pierroutsakou, D., Pizzone, R. G., Rapisarda, G. G., Romano, S., Santonocito, D., Sergi, M. L., Spartà, R., Tumino, A., and Yamaguchi, H.

Published
2021

68. Indirect determination of the astrophysical factor for the ( reaction using the asymptotic normalization coefficient method

Author

Kiss, G. G., La Cognata, M., Yarmukhamedov, R., Tursunmakhatov, K. I., Wiedenhover, I., Baby, L. T., Cherubini, S., Cvetinovic, A., D'Agata, G., Figuera, P., Guardo, G. L., Gulino, M., Hayakawa, S., Indelicato, I., Lamia, L., Lattuada, M., Mudo, F., Palmerini, S., Pizzone, R. G., Rapisarda, G. G., Romano, S., Sergi, M. L., Sparta, R., Spitaleri, C., Trippella, O., Tumino, A., Anastasiou, M., Kuvin, S. A., Rijal, N., Schmidt, B., Igamov, S. B., Sakuta, S. B., Fulop, Zs., Gyurky, Gy., Szucs, T., Halasz, Z., Somorjai, E., Hons, Z., Mrazek, J., Tribble, R. E., and Mukhamedzhanov, A. M.

Published
2021

70. Indirect determination of the astrophysical S factor for the 6Li(p,γ)7Be reaction using the asymptotic normalization coefficient method

Author

Kiss, G. G., La Cognata, M., Yarmukhamedov, R., Tursunmakhatov, K. I., Wiedenhover, I., Baby, L. T., Cherubini, S., Cvetinovic, A., D'Agata, G., Figuera, P., Guardo, G. L., Gulino, M., Hayakawa, S., Indelicato, I., Lamia, L., Lattuada, M., Mudo, F., Palmerini, S., Pizzone, R. G., Rapisarda, G. G., Romano, S., Sergi, M. L., Sparta, R., Spitaleri, C., Trippella, O., Tumino, A., Anastasiou, M., Kuvin, S. A., Rijal, N., Schmidt, B., Igamov, S. B., Sakuta, S. B., Fulop, Zs., Gyurky, Gy., Szucs, T., Halasz, Z., Somorjai, E., Hons, Z., Mrazek, J., Tribble, R. E., and Mukhamedzhanov, A. M.

Subjects
Nucleon induced nuclear reactions, Big bang nucleosynthesis, Radiative capture, Big bang nucleosynthesis, Nuclear astrophysics, Nuclear reactions, Nucleon induced nuclear reactions, Radiative capture, Nuclear astrophysics, Nuclear reactions
Published
2021

75. Proton-proton elastic scattering via the Trojan horse method

Author

Tumino, A., Spitaleri, C., Mukhamedzhanov, A., Rapisarda, G. G., Blagus, S., Bogovać, M., Cherubini, S., Crucillá, V., Elekes, Z., Fülöp, Z., Gulino, M., Gyürky, G., Kiss, G., Miljanić, Dj., Milin, M., La Cognata, M., Lamia, L., Pizzone, R. G., Rendić, D., Romano, S., Sergi, M. L., and Somorjai, E.

Published
2008
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77. Oligopeptides as mimic of acetylcholinesterase: from the rational design to the application in solid-phase extraction for pesticides

Author

Mascini, M., Sergi, M., Monti, D., Del Carlo, M., and Compagnone, D.

Subjects
Pesticides -- Properties, Oligopeptides -- Properties, Extraction (Chemistry) -- Methods, Acetylcholinesterase -- Properties, Chemistry
Abstract

Three different peptides (His-Glu-Pro-Ser, His-Gly-Ser-Ala and Glu-Pro-Ser-Ala) were selected and tested to be used as affinity binding receptors for organophosphate and carbamate pesticides. The peptides were rationally designed by mimicking acetylcholinesterase active site. The simulated binding energy of the three tetrapeptides versus one model of organophosphate (paraoxon) and one of carbamate (carbaryl) pesticide was calculated; a good correlation between shape designed and binding score was obtained. The binding properties of the peptide-pesticide interaction were studied following the variation of UV-visible spectra in different solvents. The binding constants in water, which were nicely correlated with computational data, ranged from 506 ([+ or -]115) to 36([+ or -]2) [M.sup.-1]. All the peptides had a 5-fold decrease in binding by changing solvent, going from water to less polar ethanol. The binding affinity suggested the use of these ligands as a preanalytical tool in extraction cartridges. The tetrapeptides efficiency was tested linking the peptides to two different supports. The cartridges prepared using His-Glu-Pro-Ser sequence was, as predicted, able to bind paraoxon and carbaryl with recovery values in the 72-88% range at pH 4.5. Intercolumn, interday RSD was in the 4-7% range. The columns were used for 80 cycles before losing retention ability.

Published
2008

80. Si26(p,γ)P27 direct proton capture by means of the asymptotic normalization coefficients method for mirror nuclei

Author

D'Agata, G., primary, Kilic, A. I., additional, Burjan, V., additional, Mrazek, J., additional, Glagolev, V., additional, Kroha, V., additional, Guardo, G. L., additional, La Cognata, M., additional, Lamia, L., additional, Palmerini, S., additional, Pizzone, R. G., additional, Rapisarda, G. G., additional, Romano, S., additional, Sergi, M. L., additional, Spartà, R., additional, Spitaleri, C., additional, Siváček, I., additional, and Tumino, A., additional

Published
2021
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83. The effect of the recent 17O(p,α)14N and 18O(p,α)15N fusion cross section measurements in the nucleosynthesis of AGB stars

Author

Palmerini S., Sergi M. L., La Cognata M., Lamia L., Pizzone R. G., and Spitaleri C.

Subjects
Physics, QC1-999
Abstract

The Trojan Horse Method (THM) has been used to investigate the low-energy cross sections of the 17O(p,α)14N and 18O(p,α)15N fusion reactions and to extract the strengths of the resonances that more contribute to the reaction rates at astrophysical energies. Moreover, the strength of the 65 keV resonance in the 17O(p,α)14N reaction, measured by means of the THM, has been used to renormalize the corresponding resonance strength in the 17O + p radiative capture channel. Since, proton-induced fusion reactions on 17O and 18O belong to the CNO cycle network for H-burning in stars, the new estimates of the cross sections have been introduced into calculations of Asymptotic giant branch (AGB) star nucleosynthesis to determine their impact on astrophysical environments. Results of nucleosynthesis calculations have been compared with geochemical analysis of ”presolar” grains. These solids form in the cold and dusty envelopes that surround AGB stars and once that have been ejected by stellar winds, come to us as inclusions in meteorites providing invaluable benchmarks and constraints for our knowledge of fusion reactions in astrophysical environments.

Published
2015
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86. Indirect measurement of the $$^3\hbox {He}$$(n,p)$$^3\hbox {H}$$ reaction cross section at Big Bang energies

Author

Pizzone, R. G., primary, Spampinato, C., additional, Spartá, R., additional, Couder, M., additional, Tan, W., additional, Burjan, V., additional, D’Agata, G., additional, Guardo, G. L., additional, La Cognata, M., additional, Lamia, L., additional, Mrazek, J., additional, Palmerini, S., additional, Typel, S., additional, Tumino, A., additional, Wiescher, M., additional, Anguilar, S., additional, Bardayan, D., additional, Blankstein, D., additional, Boccioli, L., additional, Callahan, L., additional, Cha, S. M., additional, Chae, K. Y., additional, Clark, A. M., additional, Frentz, B., additional, Hall, M. R., additional, Gula, A., additional, Henderson, S., additional, Kelmar, R., additional, Kwag, M. S., additional, Indelicato, I., additional, La Commara, M., additional, Lattuada, D., additional, Liu, Q., additional, Long, J., additional, Mazzocco, M., additional, Majumdar, A., additional, McGuinness, S., additional, Nelson, A., additional, Oliva, A. A., additional, O’Malley, P., additional, Prajapati, P. M., additional, Rapisarda, G. G., additional, Romano, S., additional, Sergi, M. L., additional, Seymour, C., additional, Skulski, M., additional, Spitaleri, C., additional, and Wilkinson, J., additional

Published
2020
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88. Fluorine Destruction in Stellar Environments

Author

Pizzone, R. G., primary, D’Agata, G., additional, Indelicato, I., additional, La Cognata, M., additional, Figuera, P., additional, Guardo, G. L., additional, Hayakawa, S., additional, Lamia, L., additional, Lattuada, M., additional, Milin, M., additional, Rapisarda, G. G., additional, Romano, S., additional, Sergi, M. L., additional, Skukan, N., additional, Soic̀, N., additional, Spitaleri, C., additional, and Tumino, A., additional

Published
2020
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89. Resonant C-Burning at Astrophysical Energies

Author

Tumino, A., primary, Spitaleri, C., additional, La Cognata, M., additional, Cherubini, S., additional, Guardo, G. L., additional, Gulino, M., additional, Hayakawa, S., additional, Indelicato, I., additional, Lamia, L., additional, Petrascu, H., additional, Pizzone, R. G., additional, Puglia, S. M. R., additional, Rapisarda, G. G., additional, Romano, S., additional, Sergi, M. L., additional, Spartà, R., additional, and Trache, L., additional

Published
2020
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90. Fluorine Destruction in Stars Studied via Trojan Horse Method

Author

Pizzone, R. G., primary, D’Agata, G., additional, Indelicato, I., additional, La Cognata, M., additional, Figuera, P., additional, Guardo, G. L., additional, Hayakawa, S., additional, Lamia, L., additional, Lattuada, M., additional, Milin, M., additional, Rapisarda, G. G., additional, Romano, S., additional, Sergi, M. L., additional, Skukan, N., additional, Soic̀, N., additional, Spitaleri, C., additional, and Tumino, A., additional

Published
2020
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95. The19F(α,p) Ne and23Na(p,α20 Ne Reactions at Energies of Astrophysical Interest via the Trojan Horse Method

Author

Da€™Agata, G., Pizzone, R. G., Indelicato, I., La Cognata, M., Spitaleri, C., Burjan, V., Cherubini, S., Di Pietro, A., Figuera, P., Guardo, G. L., Gulino, M., La Commara, M., Lamia, L., Lattuada, M., Mazzocco, M., Mrazek, J., Milin, M., Palmerini, S., Parascandolo, C., Pierroutsakou, D., Rapisarda, G. G., Romano, S., Sergi, M. L., SoicI€, N., Sparta¡, R., Trippella, O., and Tumino, A.

Published
2019

96. The 19F(α,p)22Ne and 23Na(p,α)20Ne Reactions at Energies of Astrophysical Interest via the Trojan Horse Method

Author

Da€™Agata, G., Pizzone, R. G., Indelicato, I., La Cognata, M., Spitaleri, C., Burjan, V., Cherubini, S., Di Pietro, A., Figuera, P., Guardo, G. L., Gulino, M., La Commara, M., Lamia, L., Lattuada, M., Mazzocco, M., Mrazek, J., Milin, M., Palmerini, S., Parascandolo, C., Pierroutsakou, D., Rapisarda, G. G., Romano, S., Sergi, M. L., SoicI€, N., Sparta¡, R., Trippella, O., and Tumino, A.

Published
2019

98. Posters

Author

Cerny, V., Zivny, P., Dostal, P., Parizkova, R., Zabka, L., Hodgson, R. E., Bosenberg, A. T., Hadley, G. P., Spapen, H., Diltoer, M., Suys, E., Borremans, M., Ramet, J., Huyghens, L., Afessa, B., Murphy, R., Hogans, L., Meyers, B., Mentec, H., Gruchet, P., Squara, P., De Jonghe, B., Peillon, I., Sollet, J. P., Bleichner, G., Zivkovic, Z., Mihailovic, S., Jakovljevic, M., Ryan, D. W., Weldon, O. G. W., Gower, S. N., Whiteley, S. M., Bodenham, A., De Robertis, E., Liu, J. M., Svantesson, C., Oahm, P. L., Thöme, J., Blomquist, S., Jonson, B., Pelagatti, C., Barattini, M., Poli, C., Ricupero, L., Olmastroni, M., Pieraccioni, P., Padelletti, M. B., Romagnoli, P., Masi, A., Rossi, G. F., Kurz-Müller, K., Tryba, M., Pelosi, P., Chiumello, D., Croci, M., Gattinoni, L., Kofings, G., Kyriakidis, M., Betrosian, A., Georgiou, L., Toufouzas, P., Lim, C. M., Choi, J. E., Kon, Y., Lee, S. D., Kim, W. S., Park, P. H., Kim, D. S., Kim, W. D., Koh, Y., Jung, B. H., Kim, W. S., Mazzi, S., Petrucci, N., Agostini, F., Vischi, F., Mitic-Milikic, M., Vukcevic, M., Obradovic, Lj. Nagomi, Sekulic, S., Peláez, J., Asensio, M. J., Jiménez, M., Sisón, M., Yus, S., Cerdeño, V., Nishizuka, K., Tashiro, K., Matsumoto, Y., Kobayashi, T., Suzuki, Y., De Blasio, E., De Sio, A., Golia, D., Papa, A., Giurbino, M., Paulone, G., Evangelista, V., Imhoff, M., Greive, H., Lehner, J. H., Löhlein, D., Kelly, K. P., Busch, T., Loge, K., Gerlach, H., Falke, K. J., Rossaint, R., Herreo, S., Suarez, T., Mosácula, J., Lacort, M., Lapuerta, J. A., Guerra, J., Benini, A., Borelli, M., Lampati, L., Acciaro, M., Pesenti, A., Verweij, M., Marcolin, R., Bombino, M., Patroniti, N., Sordi, A., Tsareva, M., Petkoy, I., Kishen, R., Bowles, B. J. M., Thomas, A. N., Geraghty, I. F., Goodall, J., Grasso, S., Giuliani, R., Puntillo, F., Mascia, L., Fiore, T., Brienza, N., Ranieri, V. M., Pavlou, E., Zevla, E., Stavropoulou, M., Papazacharias, Ch., Loannidou, E., González F. 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Published
1996
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99. Measurement of the cross-section for e+e− → hadrons near the nucleon-antinucleon threshold by the FENICE experiment

Author

Antonelli, A., Baldini, R., Bertani, M., Biagini, M. E., Bidoli, V., Bini, C., Bressani, T., Calabrese, R., Cardarelli, R., Carlin, R., Casari, C., Cugusi, L., Dalpiaz, P., De Zorzi, G., Feliciello, A., Ferrer, M. L., Ferretti, P., Gauzzi, P., Gianotti, P., Iazzi, F., Luppi, E., Marcello, S., Masoni, A., Messi, R., Morandin, M., Paoluzi, L., Pasqualucci, E., Pauli, G., Perlotto, N., Petrucci, F., Posocco, M., Preger, M., Puddu, G., Reale, M., Santi, L., Santonico, R., Sartori, P., Savrié, M., Serci, S., Sergi, M. T., Spinetti, M., Tessaro, S., Voci, C., Zuin, F., and The FENICE Collaboration

Published
1994
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100. Understanding the Underlying Principles of the Short Film

Author

Batty, C, Berry, M, Dooley, K, Frankham, B, Kerrigan, S, Sergi, M, Batty, C, Berry, M, Dooley, K, Frankham, B, Kerrigan, S, and Sergi, M

Abstract

This chapter explores the types of story possible within short films, and how often there can be confusion and uncertainty, particularly amongst student filmmakers, about what a short film really is. In order to better understand this, this chapter outlines a series of underlying principles about short film story design that, we argue, are integral to the initial stages of conceiving such films. Before script development takes place, we argue that realistic thinking about what the short film can deliver in terms of story, characters, scope and dramatic question, will result in a screen work that is not only feasible for student filmmakers to produce, but is also more likely to increase an audience’s emotional engagement with the film. Drawing on a range of multi-award-winning contemporary short films to illustrate these principles, we discuss the relationship between content and form in this genre, leading to a better understanding of the parameters within which a student filmmaker might work. While not presenting these parameters as strict and unbreakable, we argue that knowing what has worked well for others, and what audiences expect from the short film form, provides a solid basis from which to begin conceptualising a short film.

Published
2019

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