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Planar Hall-Effect Bridge Sensor With NiFeX (X = Cu, Ag, and Au) Sensing Layer
KTH, School of Information and Communication Technology (ICT), Materials- and Nano Physics, Material Physics, MF.
KTH, School of Information and Communication Technology (ICT), Materials- and Nano Physics, Material Physics, MF.ORCID iD: 0000-0003-3605-8872
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2015 (English)In: IEEE transactions on magnetics, ISSN 0018-9464, E-ISSN 1941-0069, Vol. 51, no 11, 4005404Article in journal (Refereed) PublishedText
Abstract [en]

This paper presents a new material alloy for planar Hall-effect bridge (PHEB) sensors and the accurate analysis of the resistance and sensitivity of these materials. The sensing layer is based on NiFeX (X = Cu, Ag, and Au). These alloys have a lower resistance without a significant loss of sensitivity. The presented PHEB sensors with NiFeX sensing layer show a coercivity of 1.7 Oe, lower than that of PHEB sensors with NiFe sensing layers, which have coercivities of 2.2 Oe.

Place, publisher, year, edition, pages
IEEE Press, 2015. Vol. 51, no 11, 4005404
Keyword [en]
Anisotropic magnetoresistance (AMR), antiferromagnetic (AFM), ferromagnetic (FM), magnetic anisotropy, magnetic sensor planar Hall effect
National Category
Other Materials Engineering
Identifiers
URN: urn:nbn:se:kth:diva-179169DOI: 10.1109/TMAG.2015.2451216ISI: 000364770500327ScopusID: 2-s2.0-84946121921OAI: oai:DiVA.org:kth-179169DiVA: diva2:882279
Conference
IEEE International Magnetics Conference (Intermag), MAY 11-15, 2015, Beijing, PEOPLES R CHINA
Note

QC 20151214

Available from: 2015-12-14 Created: 2015-12-11 Last updated: 2016-05-19Bibliographically approved
In thesis
1. Fabrication and Characterization of magnetometer for space applications
Open this publication in new window or tab >>Fabrication and Characterization of magnetometer for space applications
2016 (English)Doctoral thesis, comprehensive summary (Other academic)
Abstract [en]

The present rapid increase in the number of space missions demands a decrease in the cost of satellite equipment, but also requires the development of instruments that have low power consumption, low weight, and small size.Anisotropic magnetoresistance (AMR) sensors can answer these needs on account of their small size, weight, and power consumption. AMR sensors also produce lower noise than either giant magnetoresistance (GMR) or tunnel magnetoresistance (TMR) devices and are thus more suitable for space applications.The type of AMR sensor developed in this study was a Planar Hall EffectBridge (PHEB) sensor. The FM layer was also coupled with an AFM layer in order to fix the internal magnetization of the FM layer.One technique that was employed in order to meet the low-noise requirement was to make the FM layer thicker than has previously been attempted.In doing so, the exchange bias field between the AFM layer and the FMlayer is no longer high enough to bias the thicker FM layer, so in order to correct this unwanted effect, the material stack was upgraded to two AFM–FM interfaces. With this configuration, it became possible to increase the exchange field by up to 60%. Stronger exchange bias leads to a thicker FMlayer and so to lower noise in the device performance. Another strategy that was used to lower the resistance of the device was to implement an NiFeX alloy instead of the standard NiFe. NiFeX consists of an alloy of NiFe andCu, Ag, or Au; the last of these is known to have very low resistivity.This solution leads to a significant lowering of the device’s resistance. A recent technological advance used to fabricate devices with lower resistance is to deposit a multilayer of AFM–FM.

Place, publisher, year, edition, pages
Stockholm: KTH Royal Institute of Technology, 2016. 73 p.
Series
TRITA-ICT, 2016:15
Keyword
AMR, Magnetic sensor, Ferromagnetic, Antiferromagnetic, NiFe, IrMn, exchange bias.
National Category
Condensed Matter Physics
Research subject
Physics; Materials Science and Engineering
Identifiers
urn:nbn:se:kth:diva-187237 (URN)ISBN 978-91-7595-982-5 (ISBN)
Public defence
2016-06-10, Sal C, Isafjordsgatan 26, Kista, 13:01 (English)
Opponent
Supervisors
Available from: 2016-05-19 Created: 2016-05-18 Last updated: 2016-05-19Bibliographically approved

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