²é¿´: 480  |  »Ø¸´: 2
µ±Ç°Ö»ÏÔʾÂú×ãÖ¸¶¨Ìõ¼þµÄ»ØÌû£¬µã»÷ÕâÀï²é¿´±¾»°ÌâµÄËùÓлØÌû

liddrr

Í­³æ (СÓÐÃûÆø)

[ÇóÖú] Abinit ÄÜÓÃmodified Becke johnson potential ¼ÆËã´øÏ¶Âð£¿

ÇëÎÊAbinit ÄÜÓÃmodified Becke johnson potential ¼ÆËã´øÏ¶Âð£¿
СµÜÏÈл¹ý´ó¼ÒÁË£¡
»Ø¸´´ËÂ¥

» ²ÂÄãϲ»¶

» ±¾Ö÷ÌâÏà¹Ø¼ÛÖµÌùÍÆ¼ö£¬¶ÔÄúͬÑùÓаïÖú:

ÒÑÔÄ   »Ø¸´´ËÂ¥   ¹Ø×¢TA ¸øTA·¢ÏûÏ¢ ËÍTAºì»¨ TAµÄ»ØÌû

ÈñÀûµÄË鯬

ľ³æ (ÕýʽдÊÖ)

star watcher

¡¾´ð°¸¡¿Ó¦Öú»ØÌû

¡ï
¸Ðл²ÎÓ룬ӦÖúÖ¸Êý +1
liliangfang(½ð±Ò+1): ¶àлָ½Ì 2012-01-01 11:52:06
liddrr(½ð±Ò+3): 2012-01-01 17:37:12
Õâ¸öÊÇÒ»ÖÖmetagga,libxcÀïÓÐ,Ô­ÔòÉÏabinit¿ÉÒÔ.
elk×î½üÒ²¼ÓÈëÁËmetagga,²»¹ýelk×÷Õß˵ËûÃǵÄʵÏÖ²»Äܾ«È·µÃµ½wien2kµÄ½á¹û.
"Also to note for meta-GGA is that the spin-averaged kinetic energy
density, tau, is always used, even for magnetic systems. The
spin-resolved tau should be used in principle, but we cannot make it
consistent with non-collinear magnetism in this case.

Finally please note that the Tran-Blaha functional [Phys. Rev. Lett.
102, 226401 (2009)] does not produce exactly the same gaps as in the
article with Wien2k. We're not sure why this is and are still investigating."
3Â¥2012-01-01 10:51:19
ÒÑÔÄ   »Ø¸´´ËÂ¥   ¹Ø×¢TA ¸øTA·¢ÏûÏ¢ ËÍTAºì»¨ TAµÄ»ØÌû
²é¿´È«²¿ 3 ¸ö»Ø´ð

mailoliver

½ð³æ (СÓÐÃûÆø)

¡¾´ð°¸¡¿Ó¦Öú»ØÌû

¡ï
¸Ðл²ÎÓ룬ӦÖúÖ¸Êý +1
liliangfang(½ð±Ò+1): ллÌáʾ 2012-01-01 08:59:09
liddrr(½ð±Ò+1): 2012-01-01 17:36:59
Ô­ÔòÉÏ¿ÉÒÔ¡£µ«ÊÇÄãµÃÏÈÔì³öº¬ÓÐÕâÖÖ½»»»¹ØÁªµÄØÍÊÆ£¬ÓÃPAW£¬½Ì³ÌÖÐÓнÌÔõôÔ죬µ«Êǹý³ÌºÜÍ´¿à¡£
2Â¥2012-01-01 08:32:50
ÒÑÔÄ   »Ø¸´´ËÂ¥   ¹Ø×¢TA ¸øTA·¢ÏûÏ¢ ËÍTAºì»¨ TAµÄ»ØÌû
ÐÅÏ¢Ìáʾ
ÇëÌî´¦ÀíÒâ¼û