2009 MAGNET DEVELOPMENT AND INSTRUMENTATIONMeasuring the vacuum magnetic birefring<strong>en</strong>cePreviously we reported measurem<strong>en</strong>ts of birefring<strong>en</strong>ces assmall as 10 −16 with our experim<strong>en</strong>tal apparatus. During thelast year we have worked on the optimization of the signalto noise ratio.Our activity can be divided into five main themes.Vacuum system : in order to understand the ultimate pressurethat we are able to reach and the possibly systematiceffects that can occur, we have characterized the nature ofthe residual gases in our vessel using a Residual Gas Analyzerduring the <strong>en</strong>tire pumping process. Because of theconductivity of the vacuum pipe passing through the magnetcryostat, the lower limit for the pressure that we canreach with our ionic pumps is of about 10 −8 mbar. We needa lower residual pressure. We are curr<strong>en</strong>tly studying thefeasibility of deposing inside the vacuum pipe a substratetype “getter” which acts as a distributed pumping systemall along the inner surface of the pipe. Contact with theSAS getter company, the world experts of this technique,are under way. We are confid<strong>en</strong>t to reach a vacuum betterthan 10 −11 mbar which is <strong>en</strong>ough for our experim<strong>en</strong>t.Mirror intrinsic birefring<strong>en</strong>ce : static birefring<strong>en</strong>ce interfer<strong>en</strong>tialmirrors used in Fabry-Perot cavities is a limitingfactor of the signal to noise ratio. In refer<strong>en</strong>ce [Bielsa etal., Applied Physics B 97, 457, (2009)], we reported newmeasurem<strong>en</strong>ts that confirm that mirror phase retardation inducedby mirror birefring<strong>en</strong>ce decreases wh<strong>en</strong> mirror reflectivityincreases. Our study indicates that the origin ofthe intrinsic birefring<strong>en</strong>ce can be ascribed to the reflectinglayers close to the substrate. We believe that this is animportant step forward the realization of birefring<strong>en</strong>ce-freemirrors.Perot cavity (l<strong>en</strong>gth 2.2 m) of finesse 198000 (figure 177).The linewidth of the cavity resonance (FWHM) is around350 Hz which is one of the smallest ever realized. TheLMA in Lyon is curr<strong>en</strong>tly analysing the other mirrors toimprove their performances, which will allow us to furtherimprove our cavity finesse.Figure 177: The finesse of a Fabry Perot cavity is evaluatedthanks to the lifetime of the photon in the cavity. Here, the lifetimeτ is 463 µs. The corresponding finesse is F = πcτŁ = 198000.New coil : we have built a new coil in order to reach theproject goal of 25 T. It is based on our ”X” geometry, andwe have named it the XXLCoil. Its l<strong>en</strong>gth is of about50 cm. We have tested it at the LNCMI in Toulouse andat the DHMFL in Dresd<strong>en</strong> where we have reached 31 T(figure 178) (B 2 L ≥ 300 T 2 m). This result is a big stepforward the measurem<strong>en</strong>t of the vacuum magnetic birefring<strong>en</strong>ce,since we have fulfill the project requirem<strong>en</strong>ts. In thefinal experim<strong>en</strong>t, we will use three coils like this one.Dynamical response of the Fabry Perot cavity : our Fabry-Perot cavity stores photons for an average time which isbigger than 300 µ s. The magnetic pulse duration is a fewmilliseconds. Wh<strong>en</strong> the storage time of photons approachesthe pulse duration, the effect of the cavity low-pass filtercannot anymore be neglected and the ellipticity signal is nolonger exactly proportional to the square of the magneticfield amplitude. We have observed such a behaviour, andwe have implem<strong>en</strong>ted the appropriate correction in the dataanalysis program.Very low loss cavity mirrors : we have tested four new mirrorsmade by LMA in Lyon. The mirrors curr<strong>en</strong>tly used inour cavity have losses of the order of 20 ppm. LMA mirrorlosses are expected to have losses as low as a few ppm. Ourmeasurem<strong>en</strong>ts confirm such expectations. We have measuredfor the best LMA mirror losses of about 5 ppm. As aconsequ<strong>en</strong>ce, using such a mirror, we have realized a FabryFigure 178: Magnetic field obtained with a transverse coil(XXLCoil). The relevant parameter for the magnetic vacuum birefring<strong>en</strong>cemeasurem<strong>en</strong>t is B 2 L=250 T 2 m. This factor has be<strong>en</strong>improved by a factor t<strong>en</strong> in this new configuration.P. Berceau, F. Bielsa, J. Mauchain, R. BattestiA. Dupays, M. Fouché and C. Rizzo (<strong>Laboratoire</strong> Collisions Agrégats Réactivité, Toulouse, France)125
MAGNET DEVELOPMENT AND INSTRUMENTATION 2009Special purpose NMR probe for spectroscopy of quadrupolar nuclei at 30 TAlthough Nuclear Magnetic Resonance (NMR) is a wellestablished technique, there is a continuous demand for improveds<strong>en</strong>sitivity and spectral resolution. This is the basisfor the implem<strong>en</strong>tation of NMR techniques in high magneticfields. State of the art NMR spectroscopy is based onsuperconducting magnets with field str<strong>en</strong>gths up to 23.5 T.Higher dc magnetic fields may become possible with furtherdevelopm<strong>en</strong>t of superconducting technology, but theprogress is predicted to be increm<strong>en</strong>tal and exp<strong>en</strong>sive. Asan alternative, dc fields up to 34 T produced by resistivemagnets are already available, and there is considerable interestwithin the NMR community to implem<strong>en</strong>t g<strong>en</strong>eralpurpose and in particular high resolution NMR in thesemagnets. However, until rec<strong>en</strong>tly, NMR in resistive magnetswas limited to low resolution spectroscopy due to thestrong field inhomog<strong>en</strong>eity and the limited stability of thehigh power installations. In order to overcome these intrinsicdrawbacks, the developm<strong>en</strong>t of tailored and s<strong>en</strong>sitivityoptimized NMR instrum<strong>en</strong>tation is required.In this contribution we report on the commissioning of adedicated probe for NMR spectroscopy of quadrupolar nuclei(nuclear spin I > 1/2) at 30 T. In this case high magneticfield can overcome the problem of s<strong>en</strong>sitivity andline broad<strong>en</strong>ing in NMR spectra of low-s<strong>en</strong>sitivity nucleiwith strong quadrupole interactions [O. Pauvert et al., Inorg.Chem. 48, 8709 (2009)]. In order to fully b<strong>en</strong>efit fromthe advantages of higher magnetic fields, the <strong>des</strong>ign of theNMR probe has to be optimized for this particular application.A basic origin of low s<strong>en</strong>sitivity is a low gyromagneticratio γ of the examined nucleus (like 91 Zr or 25 Mg),that cannot be comp<strong>en</strong>sated as in the case of low naturalabundance, where isotope <strong>en</strong>richm<strong>en</strong>t increases s<strong>en</strong>sitivity.For a pulsed NMR experim<strong>en</strong>t consisting of an excitation ofthe nuclear transition by a radio frequ<strong>en</strong>cy (RF) field withstr<strong>en</strong>gth B 1 , followed by a detection period, a low value ofγ induces both a low signal (∝ γ 3 ) and a small spectral excitationwidth (∝ γB 1 ). H<strong>en</strong>ce, the effici<strong>en</strong>cy of an NMRexperim<strong>en</strong>t involving low-γ nuclei is strongly reduced. Inresponse to these limiting constraints the <strong>des</strong>ign of the RFcircuit of the NMR probe has to <strong>en</strong>sure that strong RF fieldsB 1 can be applied and that electric losses are minimized.In figure 179 we pres<strong>en</strong>t our realization of a room temperatureNMR probe meeting these constraints: Its bottomtuned RF circuit consists of the sol<strong>en</strong>oid NMR RF excitationand detection coil of a giv<strong>en</strong> inductance L C that isconnected in series with a variable tuning capacitance C T .L C and C T form a tunable series resonance circuit matchedto the source impedance (50 Ω) by a variable matching inductanceL M that is connected in parallel. Since the probeis based on the concept of creating strong B 1 fields by theapplication of high RF power, the probe has to withstandhigh voltages of the order of several kV without electricbreakdown. Therefore the tuning capacitance is realized bya copper cylinder capacitor, that can be continuously filledwith an alumina tube. In addition all conducting parts arerounded to avoid sources of arcing. Low electric loss is <strong>en</strong>suredby the usage of high conducting materials (copper,brass). The available tuning range of the probe (30 to 500MHz) covers most quadrupolar nuclei up to 30 T. The outerdiameter of the probe (28 mm) leaves space for future ext<strong>en</strong>sionslike passive shimming ev<strong>en</strong> in the 34 mm narrowbore M9 magnet of LNCMI-G.In addition, the probe is equipped with a second NMR circuitthat is used to stabilize the 24 MW magnet power supplyduring the experim<strong>en</strong>t by an active, NMR based fieldstabilization (NMR spin-lock). For this purpose the 63 CuNMR signal of a CuCl refer<strong>en</strong>ce sample is continuouslyrecorded and used for the g<strong>en</strong>eration of a control signal. Inorder to avoid crosstalks betwe<strong>en</strong> the two RF circuits thespin-lock circuit is fully shielded by a metallic cap. Theactive field stabilization <strong>en</strong>ables long time averaging of theNMR signal with refer<strong>en</strong>ce drifts of less than 1 ppm.After adjustm<strong>en</strong>t and optimization the probe was proved tobe fully operational. It withstands pulsed RF power of morethan 1 kW with a B 1 effici<strong>en</strong>cy of 18 G/ √ W for a sol<strong>en</strong>oidNMR coil of 3 mm inner diameter and 5 mm l<strong>en</strong>gth. At1 kW this corresponds to B 1 field str<strong>en</strong>gths of 570 G. Subsequ<strong>en</strong>tlythe probe with the spin-lock option was usedto conduct 91 Zr NMR studies on a series of inorganic Zrcompounds at 30 T. The obtained results provide a systematicand quantitative determination of the relation betwe<strong>en</strong>structural parameters (bond l<strong>en</strong>gths, bond angles, coordinationgeometry) and NMR parameters (chemical shift andquadrupole t<strong>en</strong>sors) of Zr compounds.Figure 179: Schematic view of the RF part of NMR probe consistingof the main RF circuit (upper right) and the shielded NMRspin-lock part (lower left, shielding cut for clarity).S. Krämer, C. de Vallée, H. Stork, J. Spitznagel, M. Horvatić, C. BerthierF. Fayon, A. Rakhmatullin, O. Pauvert, C. Bessada, D. Massiot (CEMHTI-CNRS, Orléans, France)126
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LABORATOIRE NATIONAL DES CHAMPS MAG
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TABLE OF CONTENTSPreface 1Carbon Al
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Coexistence of closed orbit and qua
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2009PrefaceDear Reader,You have bef
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2009 CARBON ALLOTROPESInvestigation
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2009 CARBON ALLOTROPESPropagative L
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2009 CARBON ALLOTROPESEdge fingerpr
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2009 CARBON ALLOTROPESObservation o
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2009 CARBON ALLOTROPESImproving gra
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2009 CARBON ALLOTROPESHow perfect c
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2009 CARBON ALLOTROPESTuning the el
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2009 CARBON ALLOTROPESElectric fiel
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2009 CARBON ALLOTROPESMagnetotransp
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2009 CARBON ALLOTROPESGraphite from
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2009Two-Dimensional Electron Gas25
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TWO-DIMENSIONAL ELECTRON GAS 2009Di
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TWO-DIMENSIONAL ELECTRON GAS 2009Sp
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TWO-DIMENSIONAL ELECTRON GAS 2009Cr
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TWO-DIMENSIONAL ELECTRON GAS 2009In
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2009 SEMICONDUCTORS AND NANOSTRUCTU
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2009 SEMICONDUCTORS AND NANOSTRUCTU
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2009 SEMICONDUCTORS AND NANOSTRUCTU
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2009Metals, Superconductors and Str
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