Survey
* Your assessment is very important for improving the workof artificial intelligence, which forms the content of this project
* Your assessment is very important for improving the workof artificial intelligence, which forms the content of this project
Hydrogen atom wikipedia , lookup
Electromagnet wikipedia , lookup
Aharonov–Bohm effect wikipedia , lookup
Superconductivity wikipedia , lookup
Condensed matter physics wikipedia , lookup
Quantum electrodynamics wikipedia , lookup
Neutron magnetic moment wikipedia , lookup
Spin (physics) wikipedia , lookup
Theoretical and experimental justification for the Schrödinger equation wikipedia , lookup
Time in physics wikipedia , lookup
VOLUME 92, N UMBER 9 PHYSICA L R EVIEW LET T ERS week ending 5 MARCH 2004 Electronic g Factor of Hydrogenlike Oxygen 16 O7 J. Verdú, S. Djekić, S. Stahl, T. Valenzuela, M. Vogel, and G. Werth Institut für Physik, Johannes-Gutenberg-Universität, D-55099 Mainz, Germany T. Beier, H.-J. Kluge, and W. Quint Gesellschaft für Schwerionenforschung, D-64291 Darmstadt, Germany (Received 11 September 2003; published 5 March 2004) We present an experimental value for the g factor of the electron bound in hydrogenlike oxygen, which is found to be gexpt 2:000 047 025 4 1544. The experiment was performed on a single 16 O7 ion stored in a Penning trap. For the first time, the expected line shape of the g-factor resonance is calculated which is essential for minimizing the systematic uncertainties. The measurement agrees within 1:1 with the predicted theoretical value gtheory 2:000 047 020 2 6. It represents a stringent test of bound-state quantum electrodynamics to a 0.25% level. Assuming the validity of the underlying theory, a value for the electron mass is obtained: me 0:000 548 579 909 6 4 u. This value agrees with our earlier determination on 12 C5 and allows a combination of both values which is about 4 times more precise than the currently accepted one. DOI: 10.1103/PhysRevLett.92.093002 Quantum electrodynamics is an established theory which describes the interaction of particles with the quantized radiation field to extremely high precision. This is manifested particularly in the agreement between the calculated and measured values of the magnetic moment of the free electron to 12 digits [1]. The situation is more complex when dealing with particles bound to a nucleus of charge Z mainly because the standard method of calculation by use of a perturbation expansion is not applicable anymore: while for a free particle the expansion parameter is the fine structure constant and is thus small as compared to one, this is no longer valid for a bound particle. The additional expansion parameter Z may not be small as compared to one, especially for high nuclear charges Z. For this case, nonperturbative methods of calculation have been developed [2]. Recently, the magnetic moment of the electron bound to a carbon nucleus has been determined with great precision [3]. This has stimulated theoretical calculations, and by now values of the magnetic moment of the electron bound in different hydrogenlike ions have been calculated to a high accuracy [4]. In this contribution we report on an extension of the previous experiment to hydrogenlike oxygen 16 O7 , using a similar experimental method, however, with significant improvements. The result, as discussed below, represents a first step to confirm the Z dependence of the bound-state QED calculations. It furthermore confirms the result for the electron mass extracted from the measurement on hydrogenlike carbon and allows the increase of the accuracy of that value [5,6]. The g factor of a charged particle is defined as the proportionality constant between its angular momentum J~ and the corresponding induced magnetic moment ~. 093002-1 0031-9007=04=92(9)=093002(4)$22.50 PACS numbers: 32.10.Fn, 06.20.Jr, 12.20.–m, 31.30.Jv For the electron in the ground state of a hydrogenlike ion this relation reads e ~ g J~; (1) 2me where e represents the (positive) elementary charge and me is the mass of the electron. In the presence of an external magnetic field B~ B u~ z the Zeeman splitting of the electronic ground state is given by E1s h ~ B~ i and is proportional to the Larmor precession frequency of the electron E1s h! L . The magnetic field can be calibrated by using the cyclotron frequency of the ion !c q=mi B, with q representing its charge and mi its mass. By use of this relation and Eq. (1) the g factor can be obtained in terms of measurable quantities: q me !L g2 : (2) e mi !c The static magnetic field necessary for generating the Zeeman splitting under investigation is also responsible for the radial confinement of the ions. Additionally, an electrostatic force along the magnetic field lines is used for confinement in the axial direction. This kind of arrangement is known as a Penning trap [7]. The motion of an ion in a Penning trap is a superposition of three harmonic oscillations. The rotation around the magnetic field axes is characterized by the reduced cyclotron frequency ! . The oscillation around the electric potential minimum is given by the axial frequency !z and the drift of the ion’s orbit on the radial plane by the so-called magnetron frequency ! . In order to measure the strength of the magnetic field B we make use of the wellknown invariance theorem [8] which relates the three trapping frequencies to the cyclotron frequency !2c !2 !2z !2 . 2004 The American Physical Society 093002-1 VOLUME 92, N UMBER 9 PHYSICA L R EVIEW LET T ERS week ending 5 MARCH 2004 The details of the experimental setup have been described in [9,10]. In short, it is a stack of two fivepole cylindrical compensated orthogonal Penning traps [10,11]. The central electrode of each trap, called the ring, is set to a negative voltage with respect to the two outer end caps, which are grounded. The voltage applied to the correction electrodes, Uc , placed between the end caps and the ring, is carefully selected for achieving maximum harmonicity of the trapping potential [10]. The ring of one trap, the so-called analysis trap, is made of a ferromagnetic material which locally deforms the otherwise homogeneous magnetic field, thus creating a magnetic bottle. The curvature of the magnetic field, B2 1 @2 B 2 2! @z2 , has been measured to be B2 10 1 mT=mm . This allows the determination of the electron’s spin state by the continuous Stern-Gerlach effect [10,12] as explained below. In the other trap, the so-called precision trap, the magnetic field inhomogeneity is 3 orders of magnitude smaller: B2 8:2 0:9 T=mm2 . This permits fractional uncertainties below the ppb (parts per billion) range in the measurement of !c . Between both traps the ion can be transported without affecting the spin state of the electron [9,13]. The three frequencies of the trapped ion, ! , !z , and ! , are measured electronically: the induced mirror currents upon the trap electrodes are picked up by tuned resonance circuits, amplified and by fast Fourier transformation (FFT) observed in the frequency domain. Figure 1 shows the spectrum of the induced voltage by the reduced cyclotron motion of a single 16 O7 ion. The line is a least squares fit to a Lorentzian resonance curve. The center frequency, i.e., the reduced cyclotron frequency, is obtained with a relative uncertainty of 2 1010 . Similarly, the axial frequencies both in the precision and in the analysis trap can be measured [9,10]. The magnetron frequency is determined indirectly via mode coupling to the axial degree of freedom [14] with an uncertainty of 100 mHz which suffices to determine the magnetic field with a precision of 1010 . The Zeeman splitting amounts to roughly 105 GHz in both traps. By irradiation of microwaves of this frequency, spin flips can be induced. They are detected in the analysis trap, where the ion’s total axial potential energy is given by Uz q ~ B~ , being the electric quadrupole potential. The axial frequency is determined by the second derivative of Uz and is therefore a function of the size and orientation of ~ . Thus, depending on whether the spin is up or down, the frequency is different g B by !z up !z down m! B2 2 0:48 Hz in the z 16 7 case of O . The spin flips are detected through the observation of this small jump during the continuous measurement of !z . However, this is possible only if the frequency remains constant over the typical measurement time of several minutes. The main anharmonicity of the axial potential is caused by its octupole term, c4 4 4 @4 1 @ Uz 1 ~ @@zB4 , and is proportional to ~. 4! @z4 4! q @z4 Thus, any variation of the ion’s cyclotron energy, i.e., of its associated magnetic dipole moment, distorts the harmonicity of Uz , making !z unstable. This is compensated by automatically adjusting the applied correction voltage necessary to achieve c4 0 at the given measured value of the cyclotron energy E . The correction voltage Uc obeys a linear dependence on the cyclotron energy as shown in Fig. 2. The strong magnetic bottle makes it very sensitive to fluctuations in E . The actual measurement of the g factor takes place in the precision trap. We determine the microwave frequency !MW which maximizes the probability of inducing a spin flip. This frequency would ideally correspond to the Larmor frequency !L of the electron in 16 O7 . However, in order to obtain the g factor and according to Eq. (2) the value of the magnetic field also needs to be known. Since B fluctuates with time, a separate measurement of the Larmor and cyclotron frequencies broadens the expected resonance, thus reducing the accuracy. This is avoided by measuring the spin flip probability as a function of the frequency ratio defined through !!MW . The basic c measurement cycle is as follows: (i) The electron’s spin FIG. 1 (color online). Cyclotron resonance spectrum of a single hydrogenlike oxygen ion in the precision trap. FIG. 2 (color online). Uc as a function of the cyclotron energy in the analysis trap. The error bars are smaller than the symbols. The zero point of the energy corresponds to 4 K. 093002-2 093002-2 VOLUME 92, N UMBER 9 direction is determined in the analysis trap. (ii) The ion is transported to the precision trap. Simultaneously with the measurement of !c the ion is irradiated with microwaves of the frequency !MW thus representing a try of inducing a spin flip by the frequency ratio !MW =!c . (iii) The ion is transported back to the analysis trap and a new determination of the electron’s spin state is performed. By comparison with the previous spin direction it can be determined whether for the tried a spin flip was induced in the precision trap or not. A scan over the relevant region of the instantaneous frequency ratio yields a resonance curve of the spin flip probability as shown in Fig. 3. The uncertainty assigned to each experimental data point is calculated assuming a binomial probability distribution [9]. The value of for which the spin flip probability resonance P reaches its maximum is denoted by ^ . It is determined from a least squares fit to a Lorentzian, as is justified below. Its value is ^ 4164:376 187 8 31, where the given uncertainty is purely statistical. In a perfectly homogeneous magnetic field the spin flip probability is given by a simple Lorentzian resonance curve. However, because of the nonvanishing B2 term of the magnetic field in the precision trap, the Larmor frequency and, consequently, P are functions of the ion’s kinetic energies: !L !L E ; Ez ; E [15]. In order to measure !c the cyclotron motion has to be excited to initial energies of E0 3 eV. During the try of one and because of the interaction with the detection electronics, the cyclotron motion of the ion undergoes resistive cooling [9]. Therefore, its cyclotron energy follows an exponential cooling curve: E t E0 expt= . The cooling time constant has been measured to be 298 4 s for a single oxygen ion. The axial motion stays in thermal equilibrium with the corresponding detection electronics. Thus, the energy Ez fluctuates according to a Boltzmann distribution expEz =kB Tz . This distribution has been observed experimentally [9] and yields an axial temperature of Tz 61 7 K. The magnetron energy is constant and equals FIG. 3. Experimental spin flip probability. All data are corrected to zero cyclotron energy. 093002-3 week ending 5 MARCH 2004 PHYSICA L R EVIEW LET T ERS the magnetron cooling limit E !!z kB Tz 0:10 0:01 meV [15]. Its influence upon the spin flip resonance is very small. Inserting the known relation !L !L E ; Ez ; E into the ideal Lorentzian curve, the true spin flip probability is obtained as the sum of the probabilities for the ion to experience one spin flip for any of the energy pairs E ; Ez possible during the try of a certain . It is therefore given by Zt 1 Z1 P dEz eEz =kB Tz dt0 IEz ; t0 : (3) 2tkB Tz 0 0 The integration limit t is the measurement time of 72 s and identical to the time needed for recording a cyclotron spectrum as shown in Fig. 1. The integrand I is given by I 2 2 g0 0 E0 et = z Ez $ 2 : (4) I represents the modified Lorentzian spin flip probability for a given axial energy Ez and at a time t0 within the measurement. The parameter $ is defined as $ 2 qe mmei . The constants and z are given by BB2 m g!0 2 i and z BB2 2mi !g0 ! . For a single 16 O7 ion in the precision trap, the values 1:1 0:1 109 eV1 and z 7:5 0:8 107 eV1 result. The parameter contains the influence of the microwave 21 2 BMW B power upon the resonance, where BMW is the strength of the magnetic field component of the microwaves. Finally, g0 represents the pursued g factor, given by the ratio of the ideal unperturbed Larmor to cyclotron frequencies, as defined in Eq. (2). In Fig. 4, Eq. (3) has been used to simulate the spin flip probability resonance for four different axial temperatures. For this purpose, the theoretical value of g0 [4] is used. It shows the evolution of ^ towards the correct frequency ratio with vanishing axial temperature. In general, this is true for all ion energies, since for vanishing motion amplitudes the influence of the magnetic field inhomogeneity disappears. Thus, the frequency ratio 0 FIG. 4 (color online). Calculated spin flip resonance curves according to Eq. (3). The zero point is set at the frequency ratio corresponding to the theoretical value of g0 . 093002-3 PHYSICA L R EVIEW LET T ERS VOLUME 92, N UMBER 9 TABLE I. Systematic corrections to the frequency ratio ^ of a single 16 O7 ion. The systematic uncertainty of 0 is the quadratic sum of all systematic uncertainties. Description Value Syst. uncertainty 0 ^ with Extrap. Tz ! 0 Extrap. E ! 0 Time base FFT Zero-reference E0 Microwave purity Electrical instabilities Elec. trap anharmon. Relativistic shifts 4164.376 187 8 0:000 005 0 0 0:000 000 3 0:000 000 3 6 107 6 1011 2 107 3 107 2 107 3 108 1 108 4 109 Final result 0 4164.376 183 4 7 107 E0 corresponding to the true g factor is obtained by a multiple extrapolation of ^ to zero motional energies in all degrees of freedom. The theoretical model contained in Eq. (3) predicts a linear dependence of ^ with the cyclo@ ^ tron energy of @E 2:0 0:2 106 eV1 . This linear behavior is confirmed experimentally by a mea@ ^ sured dependence of @E 1:8 0:3 106 eV1 . In the experimental resonance curve presented in Fig. 3 all obtained for different nonvanishing cyclotron energies have been corrected to zero E . Because of the linearity of ^ ^ E the symmetry of the underlying Lorentzian shape of the spin flip probability is not affected by the cyclotron energy. In contrast, a finite value of Tz deforms this symmetry. The deviation caused by the use of a simple Lorentzian curve for obtaining ^ , as shown in Fig. 3, is smaller than the statistical uncertainty for the actual temperature of Tz 61 K. Assuming the validity of Eq. (3) all necessary remaining corrections are calculated and given in Table I together with the estimated systematic uncertainties. Using the accepted values for the electron mass me [16], the mass of the neutral oxygen atom mO [17] and the sum of the binding energies of the seven missing electrons of Ebin 1:258 66 9 106 u [18], the mass of the hydrogenlike oxygen ion is mi mO 7me Ebin 15:991 075 819 2 u. Inserting mi , me , and 0 into Eq. (2) yields the g factor of the electron bound in hydrogenlike oxygen: g0 2:000 047 025 4 15 44: (5) The first uncertainty is the quadratic sum of the statistical 093002-4 week ending 5 MARCH 2004 and systematic uncertainties in the measured frequency ratio 0 . The second one is caused by the uncertainty of the electron mass given in [16]. The combined experimental uncertainty of 4.6 ppb represents about 0.27% of the bound-state QED contributions (including recoil) to the theoretical g factor of 1715 ppb [4]. Since the uncertainty of the accepted electron mass dominates over the measurement uncertainty, the argument can be turned around and, under the assumption of the validity of the calculations presented in [4], a new mass for the electron can be obtained. It is me 0:000 548 579 909 6 4 u in agreement with the value from measurements on 12 C5 [4,5]. A combination of both values improves the current accepted CODATA [16] value by a factor of about 4 [6]. This work was supported by the European Union (HITRAP HPRI-CT-2001-50036) and the BMBF. We thank R. Ley for stimulating discussions. [1] V. M. Hughes and T. Kinoshita, Rev. Mod. Phys. 71, 133 (1999). [2] V. M. Shabaev and V. A. Yerokhin, Phys. Rev. Lett. 88, 091801 (2002). [3] H. Häffner et al., Phys. Rev. Lett. 85, 5308 (2000). [4] V. A. Yerokhin, P. Indelicato, and V. M. Shabaev, Phys. Rev. Lett. 89, 143001 (2002); Can. J. Phys. 80, 1249 (2002). [5] T. Beier et al., Phys. Rev. Lett. 88, 011603 (2002). [6] B. Taylor (private communication). [7] F. M. Penning, Physica (Utrecht) 3, 873 (1936). [8] L. S. Brown and G. Gabrielse, Phys. Rev. A 25, 2423 (1982). [9] H. Häffner et al., Eur. Phys. J. D 22, 163 (2003.) [10] G. Werth, H. Häffner, and W. Quint, Adv. At. Mol. Opt. Phys. 48, 191 (2002). [11] G. Gabrielse and F. C. MacKintosh, Int. J. Mass Spectrosc. Ion Process. 57, 1 (1984). [12] H. Dehmelt, Proc. Natl. Acad. Sci. U.S.A. 53, 2291 (1986). [13] J. Verdú et al., J. Phys. B 36, 655 (2003). [14] E. A. Cornell, R. M. Weiskoff, K. R. Boyce, and D. E. Pritchard, Phys. Rev. A 41, 312 (1990). [15] L. S. Brown and G. Gabrielse, Rev. Mod. Phys. 58, 233 (1986). [16] P. J. Mohr and B. Taylor, Rev. Mod. Phys. 72, 351 (2000). [17] G. Audi, A. H. Wapstra, and C. Thibault, Nucl. Phys. A729, 337 (2003). [18] R. L. Kelly, J. Phys. Chem. Ref. Data 16, Suppl. No. 1, 1 (1987). 093002-4