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Relating Magnetic Properties and High Hyperthermia Performance of Iron Oxide Nanoflowers
Universidad de Cantabria, Spain.
DTU Technical University of Denmark, Denmark.
DTU Technical University of Denmark, Denmark.
DTU Technical University of Denmark, Denmark.
Vise andre og tillknytning
2018 (engelsk)Inngår i: The Journal of Physical Chemistry C, ISSN 1932-7447, E-ISSN 1932-7455, Vol. 122, nr 5, s. 3068-3077Artikkel i tidsskrift (Fagfellevurdert) Published
Abstract [en]

We investigated, in depth, the interrelations among structure, magnetic properties, relaxation dynamics and magnetic hyperthermia performance of magnetic nanoflowers. The nanoflowers are about 39 nm in size, and consist of densely packed iron oxide cores. They display a remanent magnetization, which we explain by the exchange coupling between the cores, but we observe indications for internal spin disorder. By polarized small-angle neutron scattering, we unambiguously confirm that, on average, the nano flowers are preferentially magnetized along one direction. The extracted discrete relaxation time distribution of the colloidally dispersed particles indicates the presence of three distinct relaxation contributions. We can explain the two slower processes by Brownian and classical Neel relaxation, respectively. The additionally observed very fast relaxation contributions are attributed by us to the relaxation of disordered spins within the nanoflowers. Finally, we show that the intrinsic loss power (ILP, magnetic hyperthermia performance) of the nanoflowers measured in colloidal dispersion at high frequency is comparatively large and independent of the viscosity of the surrounding medium. This concurs with our assumption that the observed relaxation in the high frequency range is primarily a result of internal spin relaxation, and possibly connected to the disordered spins within the individual nanoflowers.

sted, utgiver, år, opplag, sider
2018. Vol. 122, nr 5, s. 3068-3077
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Identifikatorer
URN: urn:nbn:se:ri:diva-33372DOI: 10.1021/acs.jpcc.7b11255Scopus ID: 2-s2.0-85042146321OAI: oai:DiVA.org:ri-33372DiVA, id: diva2:1187732
Tilgjengelig fra: 2018-03-05 Laget: 2018-03-05 Sist oppdatert: 2019-01-10bibliografisk kontrollert

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