Magnetism of isolated Mn12 single-molecule magnets detected by magnetic circular dichroism: Observation of spin tunneling with a magneto-optical technique

We report magnetic and magneto-optical measurements of two Mn12 single-molecule magnet derivatives isolated in organic glasses. Field-dependent magnetic circular dichroism (MCD) intensity curves (hysteresis cycles) are found to be essentially identical to superconducting quantum interference device magnetization results and provide experimental evidence for the potential of the optical technique for magnetic characterization. Optical observation of magnetic tunneling has been achieved by studying the decay of the MCD signal at weak applied magnetic field

Observation of phonon-induced magnetic deflagration in manganites

Very fast magnetic avalanches in (La, Pr)-based manganites are the signature of a phase transition from an insulating blocked charge-ordered antiferromagnetic state to a charge-delocalized ferromagnetic (CD-FM) state. We report here the experimental observation that this transition does not occur either simultaneously or randomly in the whole sample but there is instead a spatial propagation with a velocity of the order of tens of m/s. Our results show that avalanches originate from the inside of the sample, move to the outside, and occur at values of the applied magnetic field that depend on the CD-FM fraction in the sample. Moreover, upon application of surface acoustic waves at constant magnetic fields, we are able to trigger avalanches at very well-determined values of the temperature and magnetic field. Due to the interaction with the acoustic waves, the number of isolated ferromagnetic clusters in La0.225Pr0.40Ca0.375MnO3 starts to grow across the entire sample in the same way as if it were a magnetic deflagration.

Topological magnetic irreversibility in superconducting Pb samples of various shapes

The magnetic-field dependence of the magnetization of cylinders, disks, and spheres of pure type-I superconducting lead was investigated by means of isothermal measurements of first magnetization curves and hysteresis cycles. Depending on the geometry of the sample and the direction and intensity of the applied magnetic field, the intermediate state exhibits different irreversible features that become particularly highlighted in minor hysteresis cycles. The irreversibility is noticeably observed in cylinders and disks only when the magnetic field is parallel to the axis of revolution and is very subtle in spheres. When the magnetic field decreases from the normal state, the irreversibility appears at a temperature-dependent value whose distance to the thermodynamic critical field depends on the sample geometry. The irreversible features in the disks are altered when they are submitted to an annealing process. These results agree well with very recent high-resolution magneto-optical experiments in similar materials that were interpreted in terms of transitions between different topological structures for the flux configuration in the intermediate state. A discussion of the relative role of geometrical barriers for flux entry and exit and pinning effects as responsible for the magnetic irreversibility is given.

Magnetic and processability studies on rubber ferrite composites based on natural rubber and mixed ferrite

Polycrystalline single phasic mixed ferrites belonging to the series Ni1−xZnxFe2O4 for various values of x have been prepared by conventional ceramic techniques. Pre-characterized nickel zinc ferrites were then incorporated into a natural rubber matrix according to a specific recipe for various loadings. The processability and cure parameters were then determined. The magnetic properties of the ceramic filler as well as the ferrite loaded rubber ferrite composites (RFC) were evaluated and compared. A general equation for predicting the magnetic properties was also formulated. The validity of these equations were then checked and correlated with the experimental data. The coercivity of the RFCs almost resemble that of the ceramic component in the RFC. Percolation threshold is not reached for a maximum loading of 120 phr (parts per hundred rubber by weight) of the filler. These studies indicate that flexible magnets can be made with appropriate magnetic properties namely saturation magnetisation (Ms) and magnetic field strength (Hc) by a judicious choice of x and a corresponding loading. These studies also suggest that there is no possible interaction between the filler and the matrix at least at the macroscopic level. The formulated equation will aid in synthesizing RFCs with predetermined magnetic

On the Growth Mechanism of Nickel and Cobalt Nanowires and Comparison of Their Magnetic Properties

Magnetic nanowires (NWs) are ideal materials for the fabrication of various multifunctional nanostructures which can be manipulated by an external magnetic fi eld. Highly crystalline and textured nanowires of nickel (Ni NWs) and cobalt (Co NWs) with high aspect ratio (~330) and high coercivity have been synthesized by electrodeposition using nickel sulphate hexahydrate (NiSO4·6H2O) and cobalt sulphate heptahydrate (CoSO4·7H2O) respectively on nanoporous alumina membranes. They exhibit a preferential growth along〈110〉. A general mobility assisted growth mechanism for the formation of Ni and Co NWs is proposed. The role of the hydration layer on the resulting one-dimensional geometry in the case of potentiostatic electrodeposition is verified. A very high interwire interaction resulting from magnetostatic dipolar interactions between the nanowires is observed. An unusual low-temperature magnetisation switching for fi eld parallel to the wire axis is evident from the peculiar high fi eld M(T) curve

Near fifty percent sodium substituted lanthanum manganites—A potential magnetic refrigerant for room temperature applications

Nearly half of lanthanum sites in lanthanum manganites were substituted with monovalent ion-sodium and the compound possessed distorted orthorhombic structure. Ferromagnetic ordering at 300K and the magnetic isotherms at different temperature ranges were analyzed for estimating magnetic entropy variation. Magnetic entropy change of 1.5 J kg 1 K 1 was observed near 300 K. An appreciable magnetocaloric effect was also observed for a wide range of temperatures near 300K for small magnetic field variation. Heat capacity was measured for temperatures lower than 300K and the adiabatic temperature change increases with increase in temperature with a maximum of 0.62K at 280 K

Protein Folding Simulations: Confinement, External Fields and Sequence Design

The present Thesis looks at the problem of protein folding using Monte Carlo and Langevin simulations, three topics in protein folding have been studied: 1) the effect of confining potential barriers, 2) the effect of a static external field and 3) the design of amino acid sequences which fold in a short time and which have a stable native state (global minimum). Regarding the first topic, we studied the confinement of a small protein of 16 amino acids known as 1NJ0 (PDB code) which has a beta-sheet structure as a native state. The confinement of proteins occurs frequently in the cell environment. Some molecules called Chaperones, present in the cytoplasm, capture the unfolded proteins in their interior and avoid the formation of aggregates and misfolded proteins. This mechanism of confinement mediated by Chaperones is not yet well understood. In the present work we considered two kinds of potential barriers which try to mimic the confinement induced by a Chaperon molecule. The first kind of potential was a purely repulsive barrier whose only effect is to create a cavity where the protein folds up correctly. The second kind of potential was a barrier which includes both attractive and repulsive effects. We performed Wang-Landau simulations to calculate the thermodynamical properties of 1NJ0. From the free energy landscape plot we found that 1NJ0 has two intermediate states in the bulk (without confinement) which are clearly separated from the native and the unfolded states. For the case of the purely repulsive barrier we found that the intermediate states get closer to each other in the free energy landscape plot and eventually they collapse into a single intermediate state. The unfolded state is more compact, compared to that in the bulk, as the size of the barrier decreases. For an attractive barrier modifications of the states (native, unfolded and intermediates) are observed depending on the degree of attraction between the protein and the walls of the barrier. The strength of the attraction is measured by the parameter $\epsilon$. A purely repulsive barrier is obtained for $\epsilon=0$ and a purely attractive barrier for $\epsilon=1$. The states are changed slightly for magnitudes of the attraction up to $\epsilon=0.4$. The disappearance of the intermediate states of 1NJ0 is already observed for $\epsilon =0.6$. A very high attractive barrier ($\epsilon \sim 1.0$) produces a completely denatured state. In the second topic of this Thesis we dealt with the interaction of a protein with an external electric field. We demonstrated by means of computer simulations, specifically by using the Wang-Landau algorithm, that the folded, unfolded, and intermediate states can be modified by means of a field. We have found that an external field can induce several modifications in the thermodynamics of these states: for relatively low magnitudes of the field ($<2.06 \times 10^8$ V/m) no major changes in the states are observed. However, for higher magnitudes than ($6.19 \times 10^8$ V/m) one observes the appearance of a new native state which exhibits a helix-like structure. In contrast, the original native state is a $\beta$-sheet structure. In the new native state all the dipoles in the backbone structure are aligned parallel to the field. The design of amino acid sequences constitutes the third topic of the present work. We have tested the Rate of Convergence criterion proposed by D. Gridnev and M. Garcia ({\it work unpublished}). We applied it to the study of off-lattice models. The Rate of Convergence criterion is used to decide if a certain sequence will fold up correctly within a relatively short time. Before the present work, the common way to decide if a certain sequence was a good/bad folder was by performing the whole dynamics until the sequence got its native state (if it existed), or by studying the curvature of the potential energy surface. There are some difficulties in the last two approaches. In the first approach, performing the complete dynamics for hundreds of sequences is a rather challenging task because of the CPU time needed. In the second approach, calculating the curvature of the potential energy surface is possible only for very smooth surfaces. The Rate of Convergence criterion seems to avoid the previous difficulties. With this criterion one does not need to perform the complete dynamics to find the good and bad sequences. Also, the criterion does not depend on the kind of force field used and therefore it can be used even for very rugged energy surfaces.

Magneto-optische Oberflächenplasmonresonanzeffekte in austauschverschobenen Dünnschichtsystemen

Die Wechselwirkungen zwischen Biomolekülen spielen eine zentrale Rolle in der biochemischen und pharmazeutischen Forschung. In der biomolekularen Interaktionsanalyse sind dabei Biosensoren auf Basis des Oberflächenplasmonresonanzeffekts (SPR-Effekt) weitverbreitet. Seit Einführung der ersten kommerziellen SPR-Biosensoren Anfang der 1990er Jahre wurden verschiedenste Messanordnungen sowie Materialsysteme mit dem Ziel einer möglichst hohen Empfindlichkeit getestet. Eine Möglichkeit zur Steigerung der Empfindlichkeit klassischer SPR-Systeme bieten sogenannte magneto-optische SPR-Biosensoren (MOSPR-Biosensoren). Grundlage der Empfindlichkeitssteigerung ist die gleichzeitige Messung des SPR-Effekts und des transversalen magneto-optischen KERR-Effekts (tMOKE). Bisherige Untersuchungen haben sich meist auf den Einfluss der Magnetisierung freier ferromagnetischer Schichten beschränkt. Im Rahmen dieser Arbeit wurden erstmals austauschverschobene Dünnschichtsysteme (EB-Systeme), eine Kombination aus Ferromagnet und Antiferromagnet, hinsichtlich ihrer Eignung für SPR- und MOSPR-basierte biosensorische Anwendungen untersucht. Aufgrund der remanenten Magnetisierung der ferromagnetischen Schicht und ihrer magnetischen Strukturierbarkeit sind EB-Systeme eine hochinteressante Plattform zur Realisierung neuer Biosensorkonzepte. Zur Reduzierung der stark dämpfendenden Wirkung magnetischer Materialien wurde das hier betrachtete IrMn/Co EB-System zwischen zwei Goldschichten eingebettet. Eine Gegenüberstellung optimierter Au/ IrMn/Co/Au-Systeme mit einem reinen Au-System, wie es typischerweise in kommerziellen SPR-basierten Biosensoren eingesetzt wird, demonstriert, dass mit den entwickelten EB-Systemen vergleichbare Empfindlichkeiten in SPR-Sensor-Anwendungen erreicht werden können. Die magneto-optische Aktivität der untersuchten Dünnschichtsysteme liegt im Bereich der Literaturwerte für Au/Co/Au-Systeme, mit denen erhöhte Empfindlichkeiten gegenüber Standard-SPR-Biosensoren realisiert wurden. Auf Grundlage magnetisch strukturierter Au/IrMn/Co/Au-Systeme wurden neue Biosensorkonzepte entwickelt und getestet. Erste Experimente belegen, dass mit diesen Schichtsystemen eine gleichzeitige Detektion der magnetisierungsabhängigen Reflektivitäten in ortsauflösenden MOSPR-Messungen möglich ist. Eine solche Messanordnung profitiert von der erhöhten Empfindlichkeit MOSPR-basierter Biosensoren, hohen Messgeschwindigkeiten und einem verbesserten Signal-Rausch-Verhältnis. Weiterhin wurde der domänenwandassistierte Transport (DOWMAT) superparamagnetischer Partikel über der Oberfläche eines exemplarischen EB-Systems, zur Sensorintegration von Misch-, Reinigungs- und Aufkonzentrationsfunktionen erfolgreich getestet. Die Ergebnisse demonstrieren, dass ein Transport von Partikelreihen mit hohen Geschwindigkeiten bei moderaten externen Magnetfeldern über den entwickelten Schichtsystemen möglich ist. Die Agglomeration der Partikel wird dabei intrinsisch vermieden. Diese Beobachtungen verdeutlichen die Vorzüge des DOWMAT-Mechanismus für biosensorische Anwendungen. Die präsentierten Untersuchungen bilden die Grundlage auf dem Weg zur Umsetzung neuer vielversprechender Biosensorkonzepte, die eine Schlüsselfunktion in der medizinischen point-of-care-Diagnostik bei der Detektion kleinster Konzentrationen krankheitsrelevanter Biomarker einnehmen können.

Bestimmung der magnetischen Streufeldstärke von künstlichen magnetischen Domänen austauschverschobener Dünnschichtsysteme und deren Einfluss auf die Selbstassemblierung organischer Moleküle

Die lokale Anlagerung molekularer Substanzen auf Oberflächen ist technologisch von großem Interesse. Die Beeinflussung selbstassemblierender Materialien bietet dabei große Vorteile, da sie kostengünstig und großflächig angewendet werden kann. Untersuchungen einer solchen Beeinflussung mithilfe von magnetischen Feldern wurden bisher jedoch noch nicht durchgeführt. Ursache hierfür ist das, insbesondere bei der Verwendung von diamagnetischen Substanzen, geringe induzierte magnetische Moment und die daraus resultierenden geringen magnetischen Kräfte. In der vorliegenden Arbeit wurde untersucht, ob es möglich ist, die lokale Anlagerung von selbstassemblierenden, diamagnetischen Substanzen durch die Verwendung von magnetischen Streufeldern zu beeinflussen und somit ein Schichtwachstum bevorzugt in gewünschten Bereichen eines Substrats zu erreichen. Es wurde ein austauschverschobenes Dünnschichtsystem über das Verfahren der ionenbeschuss-induzierten magnetischen Strukturierung mit einem künstlichen Domänenmuster in streifenförmiger Anordnung im Mikrometermaßstab erzeugt. Über experimentelle Untersuchungen wurden die aus diesem Schichtsystem austretenden magnetischen Streufelder erstmals quantifiziert. Die experimentell unvermeidbaren Mittelungen und technischen Limitierungen wurden mithilfe eines theoretischen Modells herausgerechnet, sodass letztlich die resultierende Magnetfeldlandschaft in allen drei Dimensionen über der Probenoberfläche erhalten wurde. Durch die Bestimmung der magnetischen Suszeptibilitäten der hier verwendeten thioethersubstituierten Subphthalocyanin-Derivate konnte somit die Berechnung der induzierten magnetischen Kräfte erfolgen, deren Vergleich mit Literaturwerten eine erfolgreiche Beeinflussung der Anlagerung dieser Substanzen erhoffen ließ. Aufgrund der Kombination diverser, anspruchsvoller Nachweisverfahren konnte der experimentelle Beweis für die erfolgreiche Positionierung der molekularen Substanzen durch die magnetischen Streufelder des Dünnschichtsystems erbracht werden. Zunächst wurde nachgewiesen, dass sich die Subphthalocyanin-Derivate auf der Probenoberfläche befinden und in einer mit der Periode der magnetischen Domänenstruktur korrelierenden Geometrie anlagern. Über Untersuchungen an Synchrotronstrahlungsquellen konnte die magnetische Streifenstruktur mit der Struktur der angelagerten Moleküle überlagert werden, sodass bekannt wurde, dass sich die Moleküle bevorzugt in den magnetisch begünstigten Bereichen anlagern. Um mögliche Einflüsse einer eventuell durch den magnetischen Strukturierungsprozess lokal modifizierten Substratoberfläche als Ursache für die lokale Molekülanlagerung ausschließen zu können, wurden zusätzliche Referenzmessungen durchgeführt. Alle Untersuchungen zeigen, dass die Molekülpositionierung auf der Wechselwirkung der diamagnetischen Substanzen mit den Streufeldern des Substrats zurückzuführen ist. Der im Rahmen dieser Arbeit entwickelte Mechanismus der magnetischen Beeinflussung der lokalen Molekülanlagerung besagt dabei, dass insbesondere die Oberflächendiffusion der selbstassemblierenden Substanz durch die in-plane-Magnetfeldkomponente beeinflusst wird und vermutlich die Nukleationsphase der Selbstassemblierung entscheidend für die lokale Materialabscheidung ist. Es konnte in dieser Arbeit somit gezeigt werden, dass eine Beeinflussung der Selbstassemblierung von diamagnetischen Subphthalocyanin-Derivaten und somit eine lokal bevorzugte Anlagerung dieser Substanzen durch magnetische Streufelder von magnetisch strukturierten austauschverschobenen Dünnschichtsystemen erreicht werden kann. Es resultiert somit eine neue Möglichkeit die technologisch wichtigen Selbstassemblierungsprozesse nun auch über magnetische Streufelder beeinflussen und kontrollieren zu können. Durch die hohe Flexibilität bei den Strukturierungsmöglichkeiten der magnetischen Domänengeometrien der hier verwendeten austauschverschobenen Dünnschichtsysteme resultieren aus den hier gezeigten Ergebnissen vielfältige Anwendungsmöglichkeiten im Bereich der Beschichtungstechnik.

The expected imprint of flux rope geometry on suprathermal electrons in magnetic clouds

Magnetic clouds are a subset of interplanetary coronal mass ejections characterized by a smooth rotation in the magnetic field direction, which is interpreted as a signature of a magnetic flux rope. Suprathermal electron observations indicate that one or both ends of a magnetic cloud typically remain connected to the Sun as it moves out through the heliosphere. With distance from the axis of the flux rope, out toward its edge, the magnetic field winds more tightly about the axis and electrons must traverse longer magnetic field lines to reach the same heliocentric distance. This increased time of flight allows greater pitch-angle scattering to occur, meaning suprathermal electron pitch-angle distributions should be systematically broader at the edges of the flux rope than at the axis. We model this effect with an analytical magnetic flux rope model and a numerical scheme for suprathermal electron pitch-angle scattering and find that the signature of a magnetic flux rope should be observable with the typical pitch-angle resolution of suprathermal electron data provided ACE's SWEPAM instrument. Evidence of this signature in the observations, however, is weak, possibly because reconnection of magnetic fields within the flux rope acts to intermix flux tubes.

The accuracy of using the Ulysses result of the spatial invariance of the radial heliospheric field to compute the open solar flux

We survey observations of the radial magnetic field in the heliosphere as a function of position, sunspot number, and sunspot cycle phase. We show that most of the differences between pairs of simultaneous observations, normalized using the square of the heliocentric distance and averaged over solar rotations, are consistent with the kinematic "flux excess" effect whereby the radial component of the frozen-in heliospheric field is increased by longitudinal solar wind speed structure. In particular, the survey shows that, as expected, the flux excess effect at high latitudes is almost completely absent during sunspot minimum but is almost the same as within the streamer belt at sunspot maximum. We study the uncertainty inherent in the use of the Ulysses result that the radial field is independent of heliographic latitude in the computation of the total open solar flux: we show that after the kinematic correction for the excess flux effect has been made it causes errors that are smaller than 4.5%, with a most likely value of 2.5%. The importance of this result for understanding temporal evolution of the open solar flux is reviewed.

Coronal mass ejections and magnetic flux buildup in the heliosphere

To test for magnetic flux buildup in the heliosphere from coronal mass ejections (CMEs), we simulate heliospheric flux as a constant background open flux with a time-varying interplanetary CME (ICME) contribution. As flux carried by ejecta can only contribute to the heliospheric flux budget while it remains closed, the ICME flux opening rate is an important factor. Two separate forms for the ICME flux opening rate are considered: (1) constant and (2) exponentially decaying with time. Coronagraph observations are used to determine the CME occurrence rates, while in situ observations are used to estimate the magnetic flux content of a typical ICME. Both static equilibrium and dynamic simulations, using the constant and exponential ICME flux opening models, require flux opening timescales of ∼50 days in order to match the observed doubling in the magnetic field intensity at 1 AU over the solar cycle. Such timescales are equivalent to a change in the ICME closed flux of only ∼7–12% between 1 and 5 AU, consistent with CSE signatures; no flux buildup results. The dynamic simulation yields a solar cycle flux variation with high variability that matches the overall variability of the observed magnetic field intensity remarkably well, including the double peak forming the Gnevyshev gap.

A kinematically distorted flux rope model for magnetic clouds

Constant-α force-free magnetic flux rope models have proven to be a valuable first step toward understanding the global context of in situ observations of magnetic clouds. However, cylindrical symmetry is necessarily assumed when using such models, and it is apparent from both observations and modeling that magnetic clouds have highly noncircular cross sections. A number of approaches have been adopted to relax the circular cross section approximation: frequently, the cross-sectional shape is allowed to take an arbitrarily chosen shape (usually elliptical), increasing the number of free parameters that are fit between data and model. While a better “fit” may be achieved in terms of reducing the mean square error between the model and observed magnetic field time series, it is not always clear that this translates to a more accurate reconstruction of the global structure of the magnetic cloud. We develop a new, noncircular cross section flux rope model that is constrained by observations of CMEs/ICMEs and knowledge of the physical processes acting on the magnetic cloud: The magnetic cloud is assumed to initially take the form of a force-free flux rope in the low corona but to be subsequently deformed by a combination of axis-centered self-expansion and heliocentric radial expansion. The resulting analytical solution is validated by fitting to artificial time series produced by numerical MHD simulations of magnetic clouds and shown to accurately reproduce the global structure.

Numerical simulation of the 12 May 1997 CME Event: The role of magnetic reconnection

We perform a numerical study of the evolution of a Coronal Mass Ejection (CME) and its interaction with the coronal magnetic field based on the 12 May 1997, CME event using a global MagnetoHydroDynamic (MHD) model for the solar corona. The ambient solar wind steady-state solution is driven by photospheric magnetic field data, while the solar eruption is obtained by superimposing an unstable flux rope onto the steady-state solution. During the initial stage of CME expansion, the core flux rope reconnects with the neighboring field, which facilitates lateral expansion of the CME footprint in the low corona. The flux rope field also reconnects with the oppositely orientated overlying magnetic field in the manner of the breakout model. During this stage of the eruption, the simulated CME rotates counter-clockwise to achieve an orientation that is in agreement with the interplanetary flux rope observed at 1 AU. A significant component of the CME that expands into interplanetary space comprises one of the side lobes created mainly as a result of reconnection with the overlying field. Within 3 hours, reconnection effectively modifies the CME connectivity from the initial condition where both footpoints are rooted in the active region to a situation where one footpoint is displaced into the quiet Sun, at a significant distance (≈1R ) from the original source region. The expansion and rotation due to interaction with the overlying magnetic field stops when the CME reaches the outer edge of the helmet streamer belt, where the field is organized on a global scale. The simulation thus offers a new view of the role reconnection plays in rotating a CME flux rope and transporting its footpoints while preserving its core structure.

Suprathermal electron flux peaks at stream interfaces: Signature of solar wind dynamics or tracer for open magnetic flux transport on the Sun?

The high variability of the intensity of suprathermal electron flux in the solar wind is usually ascribed to the high variability of sources on the Sun. Here we demonstrate that a substantial amount of the variability arises from peaks in stream interaction regions, where fast wind runs into slow wind and creates a pressure ridge at the interface. Superposed epoch analysis centered on stream interfaces in 26 interaction regions previously identified in Wind data reveal a twofold increase in 250 eV flux (integrated over pitch angle). Whether the peaks result from the compression there or are solar signatures of the coronal hole boundary, to which interfaces may map, is an open question. Suggestive of the latter, some cases show a displacement between the electron and magnetic field peaks at the interface. Since solar information is transmitted to 1 AU much more quickly by suprathermal electrons compared to convected plasma signatures, the displacement may imply a shift in the coronal hole boundary through transport of open magnetic flux via interchange reconnection. If so, however, the fact that displacements occur in both directions and that the electron and field peaks in the superposed epoch analysis are nearly coincident indicate that any systematic transport expected from differential solar rotation is overwhelmed by a random pattern, possibly owing to transport across a ragged coronal hole boundary.