Complex magnetic states of heavy fermion compound CeGe

The intermetallic compound CeGe exhibits unusual magnetic behavior due to the interplay between the Kondo
 and the antiferromagnetic coupling. This particular system is interesting because the Kondo temperature is close to
 the Néel temperature, resulting in a close competition betwe...

Повний опис

Збережено в:
Бібліографічні деталі
Опубліковано в: :Физика низких температур
Дата:2012
Автори: Haines, C.R.S., Marcano, N., Smith, R.P., Aviani, I., Espeso, J.I., Gómez Sal, J.C., Saxena, S.S.
Формат: Стаття
Мова:Англійська
Опубліковано: Фізико-технічний інститут низьких температур ім. Б.І. Вєркіна НАН України 2012
Теми:
Онлайн доступ:https://nasplib.isofts.kiev.ua/handle/123456789/117273
Теги: Додати тег
Немає тегів, Будьте першим, хто поставить тег для цього запису!
Назва журналу:Digital Library of Periodicals of National Academy of Sciences of Ukraine
Цитувати:Complex magnetic states of heavy fermion
 compound CeGe / C.R.S. Haines, N. Marcano, R.P. Smith, I. Aviani, J.I. Espeso, J.C. Gómez Sal, S.S. Saxena // Физика низких температур. — 2012. — Т. 38, № 7. — С. 821-827. — Бібліогр.: 12 назв. — англ.

Репозитарії

Digital Library of Periodicals of National Academy of Sciences of Ukraine
Опис
Резюме:The intermetallic compound CeGe exhibits unusual magnetic behavior due to the interplay between the Kondo
 and the antiferromagnetic coupling. This particular system is interesting because the Kondo temperature is close to
 the Néel temperature, resulting in a close competition between the low-temperature interactions, which can be
 tuned by means of varying external parameters such as pressure and applied magnetic field. Interestingly, magnetization
 measurements up to 12 kbar reveal that the Néel temperature is not affected by pressure. Measurements of
 the electrical resistivity, however, show that the sharp upturn appearing below TN is sensitive to pressures up to
 15 kbar. This suggests that pressure may change the complex antiferromagnetic spin structure. The validity of an
 explanation based on the magnetic superzones seen in the rare earths is discussed here.
ISSN:0132-6414