TY - JOUR
T1 - Dependence of magnetic properties on the growth conditions of MnGaN grown by rf N plasma molecular beam epitaxy
AU - Haider, Muhammad B.
AU - Constantin, Costel
AU - Al-Brithen, Hamad
AU - Caruntu, Gabriel
AU - O'Connor, Charles J.
AU - Smith, Arthur R.
PY - 2005/5
Y1 - 2005/5
N2 - MnGaN has been grown by radio frequency N plasma-assisted molecular beam epitaxy. MnGaN samples were grown on MOCVD GaN(0001)/sapphire(0001) at substrate temperature of 550°C under different Ga/N flux ratios leading to 4 different growth regimes: N-rich, slight metal-rich, metal-rich, and Ga-rich. It is found that in the case of MnGaN, Mn incorporation and hence magnetic properties clearly depend on the growth conditions. Briefly, it is found that the N-rich conditions give a sample with much larger magnetization compared to the other samples. Slight metal-rich and metal-rich grown samples have very little magnetization. Finally, Ga-rich grown samples have intermediate level of magnetization. Possible origins of the magnetization are discussed. Ga-rich magnetization is attributed to accumulates, but N-rich magnetization is attributed to carrier-mediated ferromagnetism and/or ferromagnetism due to clusters.
AB - MnGaN has been grown by radio frequency N plasma-assisted molecular beam epitaxy. MnGaN samples were grown on MOCVD GaN(0001)/sapphire(0001) at substrate temperature of 550°C under different Ga/N flux ratios leading to 4 different growth regimes: N-rich, slight metal-rich, metal-rich, and Ga-rich. It is found that in the case of MnGaN, Mn incorporation and hence magnetic properties clearly depend on the growth conditions. Briefly, it is found that the N-rich conditions give a sample with much larger magnetization compared to the other samples. Slight metal-rich and metal-rich grown samples have very little magnetization. Finally, Ga-rich grown samples have intermediate level of magnetization. Possible origins of the magnetization are discussed. Ga-rich magnetization is attributed to accumulates, but N-rich magnetization is attributed to carrier-mediated ferromagnetism and/or ferromagnetism due to clusters.
UR - http://www.scopus.com/inward/record.url?scp=25444494155&partnerID=8YFLogxK
U2 - 10.1002/pssa.200420004
DO - 10.1002/pssa.200420004
M3 - Article
AN - SCOPUS:25444494155
SN - 1862-6300
VL - 202
SP - 1135
EP - 1144
JO - Physica Status Solidi (A) Applications and Materials Science
JF - Physica Status Solidi (A) Applications and Materials Science
IS - 6
ER -