Eminyakeni yamuva nje, ama-grastitational wave aqaphelayo amasiginali abhalisiwe adalwe "inhlekelele ye-cosmic ehlukile - ukuhlanganisa izimbobo ezimnyama, amabhangqa we-neutron izinkanyezi, kanye nezimbobo ezimnyama nezinkanyezi ze-neutron. Izinhlelo ezinje "ezimbi kakhulu" zingenzeka ngezindlela ezihlukile. Okokuqala, izimbobo ezimnyama ne-neutron izinkanyezi kungenzeka ngezikhathi ezithile, zihamba ngezinto ezifanayo "ezinabile" zendawo yendawo yesikhala. Okwesibili, bayakwazi ukwakha ukusondelana komunye nomunye.
Eqinisweni, zombili izimbobo ezimnyama, nezinkanyezi ze-neutron - izigaba zakamuva zokuvela kwezinkanyezi ezinkulu, ezisele ngemuva kokuqhuma kweSupernovae. Ngakho-ke, izinkanyezi ezimbalwa ezimbalwa zingavela ku "inkanyezi yenkanyezi", ngemuva kwalokho enye emva kokukhanya, kuguqukela emgodini omnyama noma i-neutron star. Futhi uhlelo olunjalo lungatholwa ngokweqiniso ngisho nangaphambi kokuba kwenzeke umfutho oyinhlekelele. Mayelana naleli qembu ososayensi baseChina abaholwa ngu-GAO ubhala esihlokweni esishicilelwe ezincwadini ze-Astrophysical Astrographs.
Uma ukuqhuma kweSupernova kuzokwenzeka emnyango ongezansi emgodini omnyama sekuvele kwakhiwa, kuzoholela ezinguquko ezitholakele. Imvamisa, ukuqubuka okunjalo kukhula ngokushesha okukhulu, phakathi nezinsuku, emva kwalokho ukukhanya kuncipha kancane. Kodwa-ke, uma umgodi omnyama useduze, khona-ke ingxenye ethile ye-supernova ephonswe kuyo izowela kuwo. Le nqubo iholela kumandla ongezekile wamandla nomsebe, okumele aguqule ijika lekristalu ngeSupernova.
Uhlobo oluthile lwalezi zinguquko luxhomekeka ngobuningi bezimo nezici zohlelo oluphindwe kabili. Kodwa-ke, yena nozakwabo bakholelwa ukuthi ezinye zezinhlelo ezifanayo eziphindwe kabili zingabonakala ku-glossnova ebengenziwanga. Mhlawumbe esikhathini esizayo, umsebenzi onjalo uzokwenziwa futhi uzokuvumela ukuthi usungule ukuthi ukwakheka kabili, ukulungele ukuhlangana nomuntu omusha oyinhlekelele, kwakha amaza adonsela phansi anamandla.
Umthombo: Isayensi Enqunu