Bayangin kita jalan ngelewatin udara, terus ngelewatin air, dan ngelewatin pasir. Lama-lama pasti jadi makin susah. Tapi ada partikel aneh super-kecil dan super-ringan yang bisa jalan nembus segalanya: mulai dari jendela kamar kita sampe planet-planet di luar angkasa. Namanya: Neutrino. Salah satu partikel yang jadi bahan dasar pembentuk alam semesta. Dan gilanya, ternyata neutrino bisa aja megang kunci misteri yang udah ngebingungin kita dan banyak pemikir sebelum kita: kenapa alam semesta… bisa ada? Gimana ceritanya?
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References:
Adams, D. Q, et al. (2020). Improved Limit on Neutrinoless Double-Beta Decay in Te130 with CUORE. Physical Review Letters, 124(12).
Arns, R. G. (2001). Detecting the Neutrino. Physics in Perspective, 3(3), 314–334.
A Science Odyssey: Atom Builder: Elementary Particles. (2019). PBS.
A. Alessandrello, et al. (1991). Measurements on radioactivity of ancient roman lead to be used as shield in searches for rare events. Nuclear Instruments and Methods in Physics Research Section B: Beam Interactions with Materials and Atoms, 61(1), 106–117.
BBC Earth Science. (2024, April 14). Exploring a $100m Underground Neutrino Detector | Science’s Greatest Mysteries | BBC Earth Science. YouTube.
Becker, Adam. (2022, April 6). CUORE Team Places New Limits on the Bizarre Behavior of Neutrinos - Berkeley Lab. Berkeley Lab News Center.
Bilenky, S. M. (2020). Neutrinos: Majorana or Dirac? Universe, 6(9), 134–134.
Birth of Neutrinos | Physics. (n.d.). CERN. (2006, September 6). Ray Davis: indefatigable neutrino pioneer – CERN Courier. CERN Courier. CERN. (2019, April 8). The Standard Model. Home.cern; CERN. Cooper, K. (2022, September 21). What are neutrinos? Space.com. Cooper, K. (2022, September 10). What is the Standard Model? Space.com. Cowan, C. L. Jr.; Reines, F.; Harrison, F. B.; Kruse, H. W.; McGuire, A. D. (1956). "Detection of the Free Neutrino: a Confirmation". Science. 124 (3212): 103–104. Bibcode:1956Sci...124..103C.
Drewes, M., Garbrecht, B., Gueter, D., & Juraj Klarić. (2016). Leptogenesis from oscillations of heavy neutrinos with large mixing angles. Journal of High Energy Physics, 2016(12).
Enz, Charles; Meyenn, Karl von (1994). "Wolfgang Pauli, A Biographical Introduction". Writings on Physics and Philosophy. Springer-Verlag: 19.
Higgs for Waldegrave. (2025). Ucl.ac.uk. History of Neutrino. (n.d.). Super-Kamiokande Official Webiste. Koberlein, B. (2020, April 17). Why was there more matter than antimatter in the Universe? Neutrinos might give us the answer. Universetoday.com. McGrayne, S.B., Trefil, J., Bertsch, G.F. (2025, April 21). atom. Encyclopedia Britannica.
Neutrinoless Double Beta Decay. (2015). Argonne National Laboratory. Neutrino invention. (2007, March). Symmetry Magazine. Office of Science. (n.d.). DOE Explains...Beta Decay. Energy.gov. O’Keefe, M. (n.d.). 1956. IceCube. Parlati, S. (2025). Cuore. Laboratori Nazionali Del Gran Sasso.
Physics | CUORE. (2016). Infn.it.
Plataforma SINC. (2013, November 29). Controversy over the use of Roman ingots to investigate dark matter and neutrinos. Phys.org. Raymond Davis Jr. (2024). The Linda Hall Library. REINES, F., & COWANjun., C. L. (1956). The Neutrino. Nature, 178(4531), 446–449.
Roman ingots to shield particle detector. (2010, April 15). Scientific American. Sterile neutrinos | All Things Neutrino. (n.d.). Sutton, C. (2025, April 7). standard model. Encyclopedia Britannica. Ultracold detector probes neutrinoless double beta decay. (2022). Physics Today, 2022(1), 0414a.
Understanding the Origin of Matter with the CUORE Experiment. (2023). Energy.gov. Venkataraman, R. (2020). Semiconductor detectors. Elsevier EBooks, 409–491.
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