| ²é¿´: 1031 | »Ø¸´: 2 | ||
| µ±Ç°Ö»ÏÔʾÂú×ãÖ¸¶¨Ìõ¼þµÄ»ØÌû£¬µã»÷ÕâÀï²é¿´±¾»°ÌâµÄËùÓлØÌû | ||
qpalzmasdͳæ (³õÈëÎÄ̳)
|
[ÇóÖú]
ÔõÑù¼ÆËãÌÓÍѹ²Õñ·ý»ñ¸ÅÂÊ
|
|
|
ÔÚH×÷Âý»¯ÎïÖÊ£¬²¢ÇÒÓë¡°1/V¡±ÎüÊÕ¼Á¾ùÔÈ»ìºÏ£¨Ç°ÕßÓëºóÕßÔ×Ó¸öÊý±ÈΪ100:1£©µÄÇé¿öÏ£¬ÒÑÖªÔÚ0.025eVʱ£¬ÎüÊÕ¼ÁµÄ΢¹ÛÎüÊÕ½ØÃæÊÇ760b£¬ÔõÑùÇó100keVµÄÖÐ×ÓÔ´·¢Éä³öµÄÖÐ×ÓÔÚ1eVµÄÌÓÍѹ²Õñ·ý»ñ¸ÅÂÊ£¿£¨²»¿¼ÂÇÎüÊÕ¼ÁµÄÉ¢É䣩Õâ¸öÎÊÌâÍêÈ«²»ÖªµÀ¸ÃÔõô´ð¡£¡£¡£»¹Çë´óÉñ¸øÐ¡µÜÉÏÉϿΡ£ Ϊ·ÀÖ¹ÎÒ·ÒëÓÐÎó£¬ÔÌâÈçÏ£º Calculate the resonance escape probability at energy 1eV for neutrons emitted at 100 keV in a mixture of hydrogen and a "1/v" absorber with a microscopic absorption cross-section of 760b at 0.025eV. The mixture contains 100 atoms of hydrogen per absorber atom. You may neglect scattering by the absorber. |
» ²ÂÄãϲ»¶
Ò»Ö¾Ô¸ÎäÀí085500»úеרҵ×Ü·Ö300Çóµ÷¼Á
ÒѾÓÐ6È˻ظ´
²ÄÁÏѧÇóµ÷¼Á
ÒѾÓÐ5È˻ظ´
¿¼Ñе÷¼Á
ÒѾÓÐ4È˻ظ´
281Çóµ÷¼Á
ÒѾÓÐ4È˻ظ´
0805 316Çóµ÷¼Á
ÒѾÓÐ6È˻ظ´
085601Çóµ÷¼Á×Ü·Ö293Ó¢Ò»Êý¶þ
ÒѾÓÐ3È˻ظ´
08¹¤Ñ§µ÷¼Á
ÒѾÓÐ17È˻ظ´
340Çóµ÷¼Á
ÒѾÓÐ4È˻ظ´
311Çóµ÷¼Á
ÒѾÓÐ3È˻ظ´
ʳƷר˶ һ־Ը˫һÁ÷ 328
ÒѾÓÐ4È˻ظ´
blueskyqw8816
ͳæ (СÓÐÃûÆø)
- Ó¦Öú: 0 (Ó×¶ùÔ°)
- ½ð±Ò: 137.1
- É¢½ð: 2
- Ìû×Ó: 55
- ÔÚÏß: 19.5Сʱ
- ³æºÅ: 529759
- ×¢²á: 2008-03-20
- ÐÔ±ð: GG
- רҵ: ºË¼¼Êõ¼°ÆäÓ¦ÓÃ
3Â¥2013-12-11 00:39:19
blueskyqw8816
ͳæ (СÓÐÃûÆø)
- Ó¦Öú: 0 (Ó×¶ùÔ°)
- ½ð±Ò: 137.1
- É¢½ð: 2
- Ìû×Ó: 55
- ÔÚÏß: 19.5Сʱ
- ³æºÅ: 529759
- ×¢²á: 2008-03-20
- ÐÔ±ð: GG
- רҵ: ºË¼¼Êõ¼°ÆäÓ¦ÓÃ
2Â¥2013-12-11 00:19:25













»Ø¸´´ËÂ¥