TY  - JOUR
AU  - Agostini, F.
AU  - Maouloud, S. E. M. Ahmed
AU  - Althueser, L.
AU  - Amaro, F.
AU  - Antunović, Biljana
AU  - Aprile, E.
AU  - Baudis, L.
AU  - Baur, D.
AU  - Biondi, Y.
AU  - Bismark, A.
AU  - Breur, P. A.
AU  - Brown, A.
AU  - Bruno, G.
AU  - Budnik, R.
AU  - Capelli, C.
AU  - Cardoso, J.
AU  - Cichon, D.
AU  - Clark, M.
AU  - Colijn, A. P.
AU  - Cuenca-García, J. J.
AU  - Cussonneau, J. P.
AU  - Decowski, M. P.
AU  - Depoian, A.
AU  - Dierle, J.
AU  - Gangi, P. Di
AU  - Giovanni, A. Di
AU  - Diglio, S.
AU  - Santos, J. M. F. dos
AU  - Drexlin, G.
AU  - Eitel, K.
AU  - Engel, R.
AU  - Ferella, A. D.
AU  - Fischer, H.
AU  - Galloway, M.
AU  - Gao, F.
AU  - Girard, F.
AU  - Glück, F.
AU  - Grandi, L.
AU  - Größle, R.
AU  - Gumbsheimer, R.
AU  - Hansmann-Menzemer, S.
AU  - Jörg, F.
AU  - Khundzakishvili, G.
AU  - Kopec, A.
AU  - Kuger, F.
AU  - Krauss, L. M.
AU  - Landsman, H.
AU  - Lang, R. F.
AU  - Lindemann, S.
AU  - Lindner, M.
AU  - Lopes, J. a. M.
AU  - Villalpando, A. Loya
AU  - Macolino, C.
AU  - Manfredini, A.
AU  - Undagoitia, T. Marrodán
AU  - Masbou, J.
AU  - Masson, E.
AU  - Meinhardt, P.
AU  - Milutinović, Slobodan
AU  - Molinario, A.
AU  - Monteiro, C. M. B.
AU  - Murra, M.
AU  - Oberlack, U. G.
AU  - Pandurović, Mila
AU  - Peres, R.
AU  - Pienaar, J.
AU  - Pierre, M.
AU  - Pizzella, V.
AU  - Qin, J.
AU  - García, D. Ramírez
AU  - Reichard, S.
AU  - Rupp, N.
AU  - Sanchez-Lucas, P.
AU  - Sartorelli, G.
AU  - Schulte, D.
AU  - Schumann, M.
AU  - Lavina, L. Scotto
AU  - Selvi, M.
AU  - Silva, M.
AU  - Simgen, H.
AU  - Steidl, M.
AU  - Terliuk, A.
AU  - Therreau, C.
AU  - Thers, D.
AU  - Thieme, K.
AU  - Trotta, R.
AU  - Tunnell, C. D.
AU  - Valerius, K.
AU  - Volta, G.
AU  - Vorkapić, D.
AU  - Weinheimer, C.
AU  - Wittweg, C.
AU  - Wolf, J.
AU  - Zopounidis, J. P.
AU  - Zuber, K.
PY  - 2020
UR  - https://vinar.vin.bg.ac.rs/handle/123456789/9633
AB  - The DARWIN observatory is a proposed next-generation experiment to search for particle dark matter and for the neutrinoless double beta decay of $$^{136}$$ 136 Xe. Out of its 50 t total natural xenon inventory, 40 t will be the active target of a time projection chamber which thus contains about 3.6 t of $$^{136}$$ 136 Xe. Here, we show that its projected half-life sensitivity is $$2.4\times {10}^{27}\,{\hbox {year}}$$ 2.4 × 10 27 year , using a fiducial volume of 5 t of natural xenon and 10 year of operation with a background rate of less than 0.2 events/(t $$\cdot $$ · year) in the energy region of interest. This sensitivity is based on a detailed Monte Carlo simulation study of the background and event topologies in the large, homogeneous target. DARWIN will be comparable in its science reach to dedicated double beta decay experiments using xenon enriched in $$^{136}$$ 136 Xe.
T2  - European Physical Journal C. Particles and Fields
T1  - Sensitivity of the DARWIN observatory to the neutrinoless double beta decay of 136 Xe
VL  - 80
IS  - 9
SP  - 1
EP  - 11
DO  - 10.1140/epjc/s10052-020-8196-z
ER  - 

@article{
author = "Agostini, F. and Maouloud, S. E. M. Ahmed and Althueser, L. and Amaro, F. and Antunović, Biljana and Aprile, E. and Baudis, L. and Baur, D. and Biondi, Y. and Bismark, A. and Breur, P. A. and Brown, A. and Bruno, G. and Budnik, R. and Capelli, C. and Cardoso, J. and Cichon, D. and Clark, M. and Colijn, A. P. and Cuenca-García, J. J. and Cussonneau, J. P. and Decowski, M. P. and Depoian, A. and Dierle, J. and Gangi, P. Di and Giovanni, A. Di and Diglio, S. and Santos, J. M. F. dos and Drexlin, G. and Eitel, K. and Engel, R. and Ferella, A. D. and Fischer, H. and Galloway, M. and Gao, F. and Girard, F. and Glück, F. and Grandi, L. and Größle, R. and Gumbsheimer, R. and Hansmann-Menzemer, S. and Jörg, F. and Khundzakishvili, G. and Kopec, A. and Kuger, F. and Krauss, L. M. and Landsman, H. and Lang, R. F. and Lindemann, S. and Lindner, M. and Lopes, J. a. M. and Villalpando, A. Loya and Macolino, C. and Manfredini, A. and Undagoitia, T. Marrodán and Masbou, J. and Masson, E. and Meinhardt, P. and Milutinović, Slobodan and Molinario, A. and Monteiro, C. M. B. and Murra, M. and Oberlack, U. G. and Pandurović, Mila and Peres, R. and Pienaar, J. and Pierre, M. and Pizzella, V. and Qin, J. and García, D. Ramírez and Reichard, S. and Rupp, N. and Sanchez-Lucas, P. and Sartorelli, G. and Schulte, D. and Schumann, M. and Lavina, L. Scotto and Selvi, M. and Silva, M. and Simgen, H. and Steidl, M. and Terliuk, A. and Therreau, C. and Thers, D. and Thieme, K. and Trotta, R. and Tunnell, C. D. and Valerius, K. and Volta, G. and Vorkapić, D. and Weinheimer, C. and Wittweg, C. and Wolf, J. and Zopounidis, J. P. and Zuber, K.",
year = "2020",
abstract = "The DARWIN observatory is a proposed next-generation experiment to search for particle dark matter and for the neutrinoless double beta decay of $$^{136}$$ 136 Xe. Out of its 50 t total natural xenon inventory, 40 t will be the active target of a time projection chamber which thus contains about 3.6 t of $$^{136}$$ 136 Xe. Here, we show that its projected half-life sensitivity is $$2.4\times {10}^{27}\,{\hbox {year}}$$ 2.4 × 10 27 year , using a fiducial volume of 5 t of natural xenon and 10 year of operation with a background rate of less than 0.2 events/(t $$\cdot $$ · year) in the energy region of interest. This sensitivity is based on a detailed Monte Carlo simulation study of the background and event topologies in the large, homogeneous target. DARWIN will be comparable in its science reach to dedicated double beta decay experiments using xenon enriched in $$^{136}$$ 136 Xe.",
journal = "European Physical Journal C. Particles and Fields",
title = "Sensitivity of the DARWIN observatory to the neutrinoless double beta decay of 136 Xe",
volume = "80",
number = "9",
pages = "1-11",
doi = "10.1140/epjc/s10052-020-8196-z"
}

Agostini, F., Maouloud, S. E. M. A., Althueser, L., Amaro, F., Antunović, B., Aprile, E., Baudis, L., Baur, D., Biondi, Y., Bismark, A., Breur, P. A., Brown, A., Bruno, G., Budnik, R., Capelli, C., Cardoso, J., Cichon, D., Clark, M., Colijn, A. P., Cuenca-García, J. J., Cussonneau, J. P., Decowski, M. P., Depoian, A., Dierle, J., Gangi, P. D., Giovanni, A. D., Diglio, S., Santos, J. M. F. d., Drexlin, G., Eitel, K., Engel, R., Ferella, A. D., Fischer, H., Galloway, M., Gao, F., Girard, F., Glück, F., Grandi, L., Größle, R., Gumbsheimer, R., Hansmann-Menzemer, S., Jörg, F., Khundzakishvili, G., Kopec, A., Kuger, F., Krauss, L. M., Landsman, H., Lang, R. F., Lindemann, S., Lindner, M., Lopes, J. a. M., Villalpando, A. L., Macolino, C., Manfredini, A., Undagoitia, T. M., Masbou, J., Masson, E., Meinhardt, P., Milutinović, S., Molinario, A., Monteiro, C. M. B., Murra, M., Oberlack, U. G., Pandurović, M., Peres, R., Pienaar, J., Pierre, M., Pizzella, V., Qin, J., García, D. R., Reichard, S., Rupp, N., Sanchez-Lucas, P., Sartorelli, G., Schulte, D., Schumann, M., Lavina, L. S., Selvi, M., Silva, M., Simgen, H., Steidl, M., Terliuk, A., Therreau, C., Thers, D., Thieme, K., Trotta, R., Tunnell, C. D., Valerius, K., Volta, G., Vorkapić, D., Weinheimer, C., Wittweg, C., Wolf, J., Zopounidis, J. P.,& Zuber, K.. (2020). Sensitivity of the DARWIN observatory to the neutrinoless double beta decay of 136 Xe. in European Physical Journal C. Particles and Fields, 80(9), 1-11.
https://doi.org/10.1140/epjc/s10052-020-8196-z

Agostini F, Maouloud SEMA, Althueser L, Amaro F, Antunović B, Aprile E, Baudis L, Baur D, Biondi Y, Bismark A, Breur PA, Brown A, Bruno G, Budnik R, Capelli C, Cardoso J, Cichon D, Clark M, Colijn AP, Cuenca-García JJ, Cussonneau JP, Decowski MP, Depoian A, Dierle J, Gangi PD, Giovanni AD, Diglio S, Santos JMFD, Drexlin G, Eitel K, Engel R, Ferella AD, Fischer H, Galloway M, Gao F, Girard F, Glück F, Grandi L, Größle R, Gumbsheimer R, Hansmann-Menzemer S, Jörg F, Khundzakishvili G, Kopec A, Kuger F, Krauss LM, Landsman H, Lang RF, Lindemann S, Lindner M, Lopes JAM, Villalpando AL, Macolino C, Manfredini A, Undagoitia TM, Masbou J, Masson E, Meinhardt P, Milutinović S, Molinario A, Monteiro CMB, Murra M, Oberlack UG, Pandurović M, Peres R, Pienaar J, Pierre M, Pizzella V, Qin J, García DR, Reichard S, Rupp N, Sanchez-Lucas P, Sartorelli G, Schulte D, Schumann M, Lavina LS, Selvi M, Silva M, Simgen H, Steidl M, Terliuk A, Therreau C, Thers D, Thieme K, Trotta R, Tunnell CD, Valerius K, Volta G, Vorkapić D, Weinheimer C, Wittweg C, Wolf J, Zopounidis JP, Zuber K. Sensitivity of the DARWIN observatory to the neutrinoless double beta decay of 136 Xe. in European Physical Journal C. Particles and Fields. 2020;80(9):1-11.
doi:10.1140/epjc/s10052-020-8196-z .

Agostini, F., Maouloud, S. E. M. Ahmed, Althueser, L., Amaro, F., Antunović, Biljana, Aprile, E., Baudis, L., Baur, D., Biondi, Y., Bismark, A., Breur, P. A., Brown, A., Bruno, G., Budnik, R., Capelli, C., Cardoso, J., Cichon, D., Clark, M., Colijn, A. P., Cuenca-García, J. J., Cussonneau, J. P., Decowski, M. P., Depoian, A., Dierle, J., Gangi, P. Di, Giovanni, A. Di, Diglio, S., Santos, J. M. F. dos, Drexlin, G., Eitel, K., Engel, R., Ferella, A. D., Fischer, H., Galloway, M., Gao, F., Girard, F., Glück, F., Grandi, L., Größle, R., Gumbsheimer, R., Hansmann-Menzemer, S., Jörg, F., Khundzakishvili, G., Kopec, A., Kuger, F., Krauss, L. M., Landsman, H., Lang, R. F., Lindemann, S., Lindner, M., Lopes, J. a. M., Villalpando, A. Loya, Macolino, C., Manfredini, A., Undagoitia, T. Marrodán, Masbou, J., Masson, E., Meinhardt, P., Milutinović, Slobodan, Molinario, A., Monteiro, C. M. B., Murra, M., Oberlack, U. G., Pandurović, Mila, Peres, R., Pienaar, J., Pierre, M., Pizzella, V., Qin, J., García, D. Ramírez, Reichard, S., Rupp, N., Sanchez-Lucas, P., Sartorelli, G., Schulte, D., Schumann, M., Lavina, L. Scotto, Selvi, M., Silva, M., Simgen, H., Steidl, M., Terliuk, A., Therreau, C., Thers, D., Thieme, K., Trotta, R., Tunnell, C. D., Valerius, K., Volta, G., Vorkapić, D., Weinheimer, C., Wittweg, C., Wolf, J., Zopounidis, J. P., Zuber, K., "Sensitivity of the DARWIN observatory to the neutrinoless double beta decay of 136 Xe" in European Physical Journal C. Particles and Fields, 80, no. 9 (2020):1-11,
https://doi.org/10.1140/epjc/s10052-020-8196-z . .

TY  - JOUR
AU  - Aalbers, J.
AU  - Agostini, F.
AU  - Maouloud, S.
AU  - Alfonsi, M.
AU  - Althueser, L.
AU  - Antunović, Biljana
AU  - Milošević, B.
AU  - Milutinović, Slobodan
AU  - Obradović, M.
AU  - Pandurović, Mila
AU  - Subotić, D.
AU  - Vorkapić, D.
PY  - 2020
UR  - https://vinar.vin.bg.ac.rs/handle/123456789/9773
AB  - We detail the sensitivity of the proposed liquid xenon DARWIN observatory to solar neutrinos via elastic electron scattering. We find that DARWIN will have the potential to measure the fluxes of five solar neutrino components: pp,  $$^7$$     7    Be,  $$^{13}$$     13    N,  $$^{15}$$     15    O and pep. The precision of the  $$^{13}$$     13    N,  $$^{15}$$     15    O and pep components is hindered by the double-beta decay of  $$^{136}$$     136    Xe and, thus, would benefit from a depleted target. A high-statistics observation of pp neutrinos would allow us to infer the values of the electroweak mixing angle,  $$\sin ^2\theta _w$$     sin 2   θ w     , and the electron-type neutrino survival probability,  $$P_{ee}$$    P  ee     , in the electron recoil energy region from a few keV up to 200 keV for the first time, with relative precision of 5% and 4%, respectively, with 10 live years of data and a 30 tonne fiducial volume. An observation of pp and  $$^7$$     7    Be neutrinos would constrain the neutrino-inferred solar luminosity down to 0.2%. A combination of all flux measurements would distinguish between the high- (GS98) and low-metallicity (AGS09) solar models with 2.1–2.5 $$\sigma $$   σ    significance, independent of external measurements from other experiments or a measurement of  $$^8$$     8    B neutrinos through coherent elastic neutrino-nucleus scattering in DARWIN. Finally, we demonstrate that with a depleted target DARWIN may be sensitive to the neutrino capture process of  $$^{131}$$     131    Xe.
T2  - European Physical Journal C. Particles and Fields
T1  - Solar neutrino detection sensitivity in DARWIN via electron scattering
VL  - 80
IS  - 12
SP  - 1133
DO  - 10.1140/epjc/s10052-020-08602-7
ER  - 

@article{
author = "Aalbers, J. and Agostini, F. and Maouloud, S. and Alfonsi, M. and Althueser, L. and Antunović, Biljana and Milošević, B. and Milutinović, Slobodan and Obradović, M. and Pandurović, Mila and Subotić, D. and Vorkapić, D.",
year = "2020",
abstract = "We detail the sensitivity of the proposed liquid xenon DARWIN observatory to solar neutrinos via elastic electron scattering. We find that DARWIN will have the potential to measure the fluxes of five solar neutrino components: pp,  $$^7$$     7    Be,  $$^{13}$$     13    N,  $$^{15}$$     15    O and pep. The precision of the  $$^{13}$$     13    N,  $$^{15}$$     15    O and pep components is hindered by the double-beta decay of  $$^{136}$$     136    Xe and, thus, would benefit from a depleted target. A high-statistics observation of pp neutrinos would allow us to infer the values of the electroweak mixing angle,  $$\sin ^2\theta _w$$     sin 2   θ w     , and the electron-type neutrino survival probability,  $$P_{ee}$$    P  ee     , in the electron recoil energy region from a few keV up to 200 keV for the first time, with relative precision of 5% and 4%, respectively, with 10 live years of data and a 30 tonne fiducial volume. An observation of pp and  $$^7$$     7    Be neutrinos would constrain the neutrino-inferred solar luminosity down to 0.2%. A combination of all flux measurements would distinguish between the high- (GS98) and low-metallicity (AGS09) solar models with 2.1–2.5 $$\sigma $$   σ    significance, independent of external measurements from other experiments or a measurement of  $$^8$$     8    B neutrinos through coherent elastic neutrino-nucleus scattering in DARWIN. Finally, we demonstrate that with a depleted target DARWIN may be sensitive to the neutrino capture process of  $$^{131}$$     131    Xe.",
journal = "European Physical Journal C. Particles and Fields",
title = "Solar neutrino detection sensitivity in DARWIN via electron scattering",
volume = "80",
number = "12",
pages = "1133",
doi = "10.1140/epjc/s10052-020-08602-7"
}

Aalbers, J., Agostini, F., Maouloud, S., Alfonsi, M., Althueser, L., Antunović, B., Milošević, B., Milutinović, S., Obradović, M., Pandurović, M., Subotić, D.,& Vorkapić, D.. (2020). Solar neutrino detection sensitivity in DARWIN via electron scattering. in European Physical Journal C. Particles and Fields, 80(12), 1133.
https://doi.org/10.1140/epjc/s10052-020-08602-7

Aalbers J, Agostini F, Maouloud S, Alfonsi M, Althueser L, Antunović B, Milošević B, Milutinović S, Obradović M, Pandurović M, Subotić D, Vorkapić D. Solar neutrino detection sensitivity in DARWIN via electron scattering. in European Physical Journal C. Particles and Fields. 2020;80(12):1133.
doi:10.1140/epjc/s10052-020-08602-7 .

Aalbers, J., Agostini, F., Maouloud, S., Alfonsi, M., Althueser, L., Antunović, Biljana, Milošević, B., Milutinović, Slobodan, Obradović, M., Pandurović, Mila, Subotić, D., Vorkapić, D., "Solar neutrino detection sensitivity in DARWIN via electron scattering" in European Physical Journal C. Particles and Fields, 80, no. 12 (2020):1133,
https://doi.org/10.1140/epjc/s10052-020-08602-7 . .

TY  - JOUR
AU  - Kelic, A
AU  - Itkis, IM
AU  - Pokrovsky, IV
AU  - Prokhorova, EV
AU  - Benoit, B
AU  - Costa, G
AU  - Donadille, L
AU  - Dorvaux, O
AU  - Brennand, ED
AU  - Guillaume, G
AU  - Hanappe, F
AU  - Heusch, B
AU  - Huck, A
AU  - Itkis, MG
AU  - Jokić, Stevan
AU  - Kondratiev, NA
AU  - Kozulin, EM
AU  - Oganessian, YT
AU  - Rudolf, G
AU  - Rusanov, AY
AU  - Stuttge, L
AU  - Vorkapić, D.
AU  - Yuasa-Nakagawa, K
PY  - 1999
UR  - https://vinar.vin.bg.ac.rs/handle/123456789/2272
AB  - The neutron spectra associated to the two fission modes of Th-226 have been measured in coincidence with the fragment yields of the O-18 + Pb-208 reaction at E-lab = 78 MeV. The pre- and post-fission multiplicities and temperatures have been extracted. Surprisingly, the prefission neutron multiplicities associated with the asymmetric mode are larger than those associated with the symmetric mode.
T2  - Europhysics Letters / EPL
T1  - Prefission neutron multiplicities and the fission modes of Th-226
VL  - 47
IS  - 5
SP  - 552
EP  - 555
DO  - 10.1209/epl/i1999-00424-4
ER  - 

@article{
author = "Kelic, A and Itkis, IM and Pokrovsky, IV and Prokhorova, EV and Benoit, B and Costa, G and Donadille, L and Dorvaux, O and Brennand, ED and Guillaume, G and Hanappe, F and Heusch, B and Huck, A and Itkis, MG and Jokić, Stevan and Kondratiev, NA and Kozulin, EM and Oganessian, YT and Rudolf, G and Rusanov, AY and Stuttge, L and Vorkapić, D. and Yuasa-Nakagawa, K",
year = "1999",
abstract = "The neutron spectra associated to the two fission modes of Th-226 have been measured in coincidence with the fragment yields of the O-18 + Pb-208 reaction at E-lab = 78 MeV. The pre- and post-fission multiplicities and temperatures have been extracted. Surprisingly, the prefission neutron multiplicities associated with the asymmetric mode are larger than those associated with the symmetric mode.",
journal = "Europhysics Letters / EPL",
title = "Prefission neutron multiplicities and the fission modes of Th-226",
volume = "47",
number = "5",
pages = "552-555",
doi = "10.1209/epl/i1999-00424-4"
}

Kelic, A., Itkis, I., Pokrovsky, I., Prokhorova, E., Benoit, B., Costa, G., Donadille, L., Dorvaux, O., Brennand, E., Guillaume, G., Hanappe, F., Heusch, B., Huck, A., Itkis, M., Jokić, S., Kondratiev, N., Kozulin, E., Oganessian, Y., Rudolf, G., Rusanov, A., Stuttge, L., Vorkapić, D.,& Yuasa-Nakagawa, K.. (1999). Prefission neutron multiplicities and the fission modes of Th-226. in Europhysics Letters / EPL, 47(5), 552-555.
https://doi.org/10.1209/epl/i1999-00424-4

Kelic A, Itkis I, Pokrovsky I, Prokhorova E, Benoit B, Costa G, Donadille L, Dorvaux O, Brennand E, Guillaume G, Hanappe F, Heusch B, Huck A, Itkis M, Jokić S, Kondratiev N, Kozulin E, Oganessian Y, Rudolf G, Rusanov A, Stuttge L, Vorkapić D, Yuasa-Nakagawa K. Prefission neutron multiplicities and the fission modes of Th-226. in Europhysics Letters / EPL. 1999;47(5):552-555.
doi:10.1209/epl/i1999-00424-4 .

Kelic, A, Itkis, IM, Pokrovsky, IV, Prokhorova, EV, Benoit, B, Costa, G, Donadille, L, Dorvaux, O, Brennand, ED, Guillaume, G, Hanappe, F, Heusch, B, Huck, A, Itkis, MG, Jokić, Stevan, Kondratiev, NA, Kozulin, EM, Oganessian, YT, Rudolf, G, Rusanov, AY, Stuttge, L, Vorkapić, D., Yuasa-Nakagawa, K, "Prefission neutron multiplicities and the fission modes of Th-226" in Europhysics Letters / EPL, 47, no. 5 (1999):552-555,
https://doi.org/10.1209/epl/i1999-00424-4 . .

TY  - JOUR
AU  - Vorkapić, D.
AU  - Ivanišević, B.
PY  - 1997
UR  - https://vinar.vin.bg.ac.rs/handle/123456789/2069
AB  - It is shown that K-equilibration fission can explain the decrease of mass resolved fission fragment anisotropy at larger mass asymmetries. Two competing mechanisms contribute to the anisotropy. The effective moment of inertia and K-0(2) decreases with the increase of mass asymmetry and contribute to the increase of anisotropy. On the other hand, for larger asymmetries, the barriers are higher and lifetimes are longer. Such systems are more K equilibrated and will have smaller anisotropy.
T2  - Physical Review C
T1  - Mass resolved angular distribution of fission fragments for near-barrier fusion-fission reactions
VL  - 55
IS  - 5
SP  - 2711
EP  - 2714
DO  - 10.1103/PhysRevC.55.2711
ER  - 

@article{
author = "Vorkapić, D. and Ivanišević, B.",
year = "1997",
abstract = "It is shown that K-equilibration fission can explain the decrease of mass resolved fission fragment anisotropy at larger mass asymmetries. Two competing mechanisms contribute to the anisotropy. The effective moment of inertia and K-0(2) decreases with the increase of mass asymmetry and contribute to the increase of anisotropy. On the other hand, for larger asymmetries, the barriers are higher and lifetimes are longer. Such systems are more K equilibrated and will have smaller anisotropy.",
journal = "Physical Review C",
title = "Mass resolved angular distribution of fission fragments for near-barrier fusion-fission reactions",
volume = "55",
number = "5",
pages = "2711-2714",
doi = "10.1103/PhysRevC.55.2711"
}

Vorkapić, D.,& Ivanišević, B.. (1997). Mass resolved angular distribution of fission fragments for near-barrier fusion-fission reactions. in Physical Review C, 55(5), 2711-2714.
https://doi.org/10.1103/PhysRevC.55.2711

Vorkapić D, Ivanišević B. Mass resolved angular distribution of fission fragments for near-barrier fusion-fission reactions. in Physical Review C. 1997;55(5):2711-2714.
doi:10.1103/PhysRevC.55.2711 .

Vorkapić, D., Ivanišević, B., "Mass resolved angular distribution of fission fragments for near-barrier fusion-fission reactions" in Physical Review C, 55, no. 5 (1997):2711-2714,
https://doi.org/10.1103/PhysRevC.55.2711 . .