以The modification of the Newtonian dynamics來探究星系距離

完整後設資料紀錄

DC 欄位	值	語言
dc.contributor.author	謝玉真	en_US
dc.contributor.author	Hsieh Yu Chen	en_US
dc.contributor.author	高文芳	en_US
dc.contributor.author	W.F.Gore	en_US
dc.date.accessioned	2014-12-12T02:09:09Z	-
dc.date.available	2014-12-12T02:09:09Z	-
dc.date.issued	2004	en_US
dc.identifier.uri	http://140.113.39.130/cdrfb3/record/nctu/#GT009127520	en_US
dc.identifier.uri	http://hdl.handle.net/11536/55824	-
dc.description.abstract	『修正的牛頓力學』（Modified Newtonian Dynamics）是一個新的物理理論, 企圖改變牛頓運動力學以解釋星系自轉的速度問題。於1983年由Mordehai Milgrom提出，在以沒有暗物質的假設前提下，計算出與觀測現象相符的星系盤上的自轉曲線(rotation curve)。而這MOND的理論，將可以幫助我們從已知的星系自轉速度的分布，與目前觀測到星系的表面亮度的分布(surface brightness)，去反推算出星系所在的距離。	zh_TW
dc.description.abstract	The modified Newtonian dynamics is a new physical theory which attempts to explain the rotation curve problem of galaxies by changing Newton's law of motion. MOND was proposed by Mordehai Milgrom in 1983. The new theory can explain well why the galaxies rotation curve is "flat " and don't need to take account of "Dark Matter".	en_US
dc.language.iso	zh_TW	en_US
dc.subject	修正牛頓力學	zh_TW
dc.subject	NGC3198	zh_TW
dc.subject	NGC2903	zh_TW
dc.subject	星系的距離	zh_TW
dc.subject	自轉速度	zh_TW
dc.subject	MOND	en_US
dc.subject	NGC3198	en_US
dc.subject	NGC2903	en_US
dc.subject	distance of galaxy	en_US
dc.subject	rotation curve	en_US
dc.subject	Milgrom	en_US
dc.title	以The modification of the Newtonian dynamics來探究星系距離	zh_TW
dc.title	To Calibrate Galaxy's Distance By The Modification of The Newtonian Dynamics	en_US
dc.type	Thesis	en_US
dc.contributor.department	物理研究所	zh_TW
顯示於類別：	畢業論文

文件中的檔案：

752001.pdf

若為 zip 檔案，請下載檔案解壓縮後，用瀏覽器開啟資料夾中的 index.html 瀏覽全文。