是他1952年在一篇廣播稿中開玩笑地創(chuàng)造了大爆炸這個(gè)名字。他指出,我們?cè)诶斫馕锢韺W(xué)的時(shí)候,怎么也解釋不了為什么一切會(huì)聚合成一點(diǎn),然后又突然戲劇性地開始膨脹。
Hoyle favored a steady-state theory in which the universe was constantly expanding andcontinually creating new matter as it went. Hoyle also realized that if stars imploded they wouldliberate huge amounts of heat—100 million degrees or more, enough to begin to generate theheavier elements in a process known as nucleosynthesis. In 1957, working with others, Hoyleshowed how the heavier elements were formed in supernova explosions. For this work, W. A.Fowler, one of his collaborators, received a Nobel Prize. Hoyle, shamefully, did not.
霍伊爾贊成恒穩(wěn)態(tài)學(xué)說(shuō),該學(xué)說(shuō)認(rèn)為宇宙在不斷膨脹,在此過(guò)程中不斷創(chuàng)造新的物質(zhì)?;粢翣栠€意識(shí)到,要是恒星發(fā)生爆聚,便會(huì)釋放出大量熱量--溫度在1億攝氏度以上,足以在被稱之為核合成的過(guò)程中產(chǎn)生較重的元素。1957年,霍伊爾和別人一起,展示重元素是如何在超新星的爆炸中形成的。由于這項(xiàng)工作,他的合作者W.A.福勒獲得了諾貝爾獎(jiǎng)?;粢翣杽t沒有,很難為情。
According to Hoyle's theory, an exploding star would generate enough heat to create all thenew elements and spray them into the cosmos where they would form gaseous clouds—theinterstellar medium as it is known—that could eventually coalesce into new solar systems.With the new theories it became possible at last to construct plausible scenarios for how wegot here. What we now think we know is this.
根據(jù)霍伊爾的理論,一顆爆炸中的恒星會(huì)釋放出足夠的熱量來(lái)產(chǎn)生所有的新元素,并把它們?yōu)⒃谟钪胬?。這些元素會(huì)形成氣云--就是所謂的星際媒介--最終聚合成新的太陽(yáng)系。有了這些理論,我們終于可以為我們?cè)趺磿?huì)來(lái)到這個(gè)世界的問(wèn)題構(gòu)筑一個(gè)貌似有理的設(shè)想。我們現(xiàn)在認(rèn)為自己知道的情況如下。