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1.
The half-life of theI,K π=2, 2? state at 1318 keV in174Yb has been measured in the173Yb(n, γ) reaction to be 0.486±0.015 ns. This half-life determines the absolute transition probabilities of the gamma-ray transitions to the ground state rotational band yielding the following hindrance factors relative to the Weisskopf estimate:F W(M 2; 2, 2?→0, 0+)=350;F W(M2; 2, 2?→2, 0+)≧77F W(M 2;2, 2?→4, 0+)>740;F W(E 1; 2, 2?→2, 0+)=4.5×106;F W(E 3; 2, 2?→2, 0+)≈0.1;F W(E 3; 2, 2?→4, 0+)≈0.4. These data are compared to analogous transitions in neighboring nuclei.  相似文献   

2.
The half-lives of the following intrinsic states in deformed odd-mass nuclei has been measured by delayed coincidences with a time-to-amplitude converter:
  1. 5/2 5/2+[642] at 86.5 keV in155Gd:T 1/2=6.7±0.3 ns, which results in the determination of theE1,ΔK=1 transition probability to the ground state 3/2 3/2?[521] and first rotational state 5/2 3/2?[521], yielding hindrance factors ofF N ≈5.5 and ≈1.8 (F W =3.1×104 and 2.3×104) respectively.
  2. (3) 5/2 5/2?[512] at 191.4 keV in169Yb:T 1/2=3.35±0.15 ns and at 122.39 keV in171Yb:T 1/2=265±20 ns which results in the determination of the transition probabilities of theE1,ΔK=1 transitions to the ground states 7/2 7/2+[633], of theK-forbiddenM1 transitions to the 5/2 and 3/2 1/2?[521] and of theE2 transitions to the 5/2, 3/2 and 1/2 1/2?[521] states in both nuclei.
TheE1 transition probabilities are compared to the transitions between the same Nilsson states in173Yb and175Hf discussing the influence of the position of the Fermi surface — obtained from recent stripping and pick-up reactions — on these transition probabilities. Additional information on the decay scheme of171Lu→171Yb is obtained by delayed coincidence measurements. For testing the used time-to-amplitude converter the well known half-lives of the 482 keV level in181Ta (T 1/2=10.4±0.3 ns) and of the 279 keV level in203Tl (T 1/2=0.285 ±0.015 ns) were measured, in good agreement with other measurements.  相似文献   

3.
The internal conversion subshell intensities of the (21.529±0.014) keV transition in151Eu and the (22.494±0.011) keV transition in149Sm have been determined in a high resolution investigation using a double-focussing iron-core spectrometer. The subshell ratios yielded unambiguousM1+E2 multipole mixtures for both transitions. δ2(E2/M1) for the 21.53 keV transition was determined to be (8.8±0.7)·10?4 and for the 22.49 keV transition to be (5.5±1.2)·10?3.  相似文献   

4.
The conversion electron spectrum of the decay of152Eu m (9.3 h) has been specially investigated forE0 transitions with the aid of a magnetic spectrometer and coincidence techniques. Besides the knownE0 transitions of 685 keV in152Sm and 615 keV in152Gd two further pureE0 transitions of 432 keV and 1048 keV have been observed. It is shown that theseE0 transitions are identical with those observed previously in the decay of152Tb. NoE0 transitions could be found from a 0+ state of 1083 keV in152Sm. The measured intensities together with the gamma spectrum measured by Barretteet al. give a consistent decay scheme of152Eu m . Furthermore the half-life of the 0+ level at 615 keV in152Gd was measured using the method of “delayed coincidences”. The result was (0.2≦t 1/2≦2.1)×10?10 s. From this theE0 transition probability for the level was derived as (0.3≦W K (E0)≦3.7)× 109 s?1 and theρ-value as 0.10≦¦ρ¦≦0.36. The results are discussed within the framework of the collective model.  相似文献   

5.
The transitional nucleus152Eu has been studied using the (n, e), (n, γ), (n res,γ), (n, γγ), (d, p), (d, t) and (p, d) reactions. The experiments have been performed at nine different laboratories. A model independent level scheme was established including 95 levels below 510 keV and nearly 900 transitions by combination of low energy transitions and reaction data. More than 20 additional levels result from gamma rays and/or charged particle reactions. The level scheme is interpreted in terms of the Nilsson model indicating that152Eu is a deformed nucleus. Seven rotational bands and Nilsson configurations are established. An additional 27 rotational bands are tentatively or speculatively assugned. Gallagher-Moszkowski splittings are discussed. The neutron binding energy was determined as 6305.2±0.5 keV. The energy of the 9.3 h 0? isomer is 45.599 keV. The lifetimes of four levels were measured. Nuclear Reactions151Eu(n,γ),E n =thermal and resonance; measuredE γ ,I γ ,E c.e.,I c.e.,γγ Coinc.,γγΔt coinc.;151Eu(d, p),E=12MeV and 14MeV;153Eu(d, t),E=12MeV;153Eu(p, d),E =18MeV; deduced level scheme of152Eu,J, π, T 1/2,cc, Nilsson configurations. Magnetic electron spectrometer, curved crystal spectrometer, Ge(Li) and Si(Li) detectors, magnetic spectrographs. Enriched targets.  相似文献   

6.
The half lives of the 5/2 5/2?[523] level at 25.7 keV in 66 161 Dy and the 5/2 5/2+[642] level in 68 163 Er, found in this work to lie at 69.2 keV, have been determined by the delayed coincidence method to be T1/2=27.8± 1.5 nsec, and T1/2=8.8± 0.5 nsec, respectively. The following hindrance factors relative to the single particle Weisskopf estimate (F W and the Nilsson estimate (FN were obtained: 66 161 Dy 5/2 5/2?[523] → 5/2 5/2+[642]:FW=(6.6± 1.3) × 103, FN=0.48± 0.10 68 163 Er 5/2 5/2+[642] → 5/2 5/2?[523]:FW=(2.4± 0.5)× 104, FN=1.8 ± 0.4 A systematic difference between transitions in odd proton nuclei and odd neutron nuclei was found: E1, ΔK=0 transitions in odd neutron nuclei have hindrance factors FN from 2.9 to 0.16, this means, these transitions are in agreement with the predictions of the Nilsson model within a factor of 10. For transitions in odd proton nuclei one has hindrance factors FN from 75 to 9.9 × 10?4. It is shown that a small difference between the deformation of the initial and the final state changes the transition probability of both, proton and neutron transitions, considerably.  相似文献   

7.
The γγ ande ? KL γ directional correlations have been measured for the (898–1836) keV cascade in88Sr following the decay of88Y. The observed correlation coefficients areA 22(γγ)=?0.0784±0.0042 andA 22(e ? KL γ)=0.0102±0.0046. The γγ experiment is consistent with a mixing ratio δ(γ)=0.009±0.005 for the 898 keV transition. Using the result of thee ? KL γ experiment the most probable value of the ratio of the penetration matrix element to the normal γ-ray matrix element was determined to be η=0.03±0.30 showing a normal conversion process. This penetration parameter agrees with a hindrance factorH W(E1)=2.1 · 10?3 for theE1 transition.  相似文献   

8.
M. G. Kozlov 《JETP Letters》2002,75(11):534-538
We calculate the nuclear spin-dependent parity-nonconserving E1 amplitudes for the optical transition 6p 1/2, F →6p 3/2, F′ and hyperfine transition 6p 1/2, F →6p 1/2, F′ in 205Tl. The experimental limit placed upon the former amplitude by Vetter et al. [PRL 74, 2658 (1995)] corresponds to the anapole moment constant κa=?0.26±0.27.  相似文献   

9.
The F2(2) ← F1(2) and F2(2) ← F1(1) transitions of the J = 7 levels of the ground state of CH4 have been observed by infrared-radio frequency double resonance using the 3.39 μ HeNe laser line. The transition frequencies are 423.02 ± 0.02 MHz and 1246.55 ± 0.02 MHz, respectively. Using these frequencies and the splitting of the E and F2 levels of the J = 2 state calculated from the molecular beam magnetic resonance spectra of Ozier, the centrifugal distortion constants are derived to be Dt = 132933 ± 10 Hz, H4t = ? 16.65 ± 0.2 Hz, and H6t = 10 ± 1 Hz. The J = 15 E(1)E(2) microwave transition is predicted as 14150 ± 9 MHz.  相似文献   

10.
The nuclide141Eu is identified to have two beta decaying isomers,141g Eu and141m Eu, whose decay half-lives are measured to be 40.0±0.7 s and 3.3±0.3s, respectively. Their decay properties are studied by means of beta and gamma spectroscopy techniques. The states withJ π assignments in141Sm thus deduced are compared with those of the other odd-A, N=79 isotones. The total decay energy of141g Eu is measured to be 6.03±0.10 MeV, which is compared with the predictions of several mass formulae and with the decay energy systematics of theN=78 isotones. The141g Eu and141m Eu are deduced to haveJ π =5/2+ and 11/2?, respectively. A 96.4 keV isomeric transition between them is found to be anE3 transition with aB(E3)=1.6±0.4e 2fm6. The structure of141Eu is compared with that of the otherN = 78 isotones.  相似文献   

11.
The decay of125m Xe produced by the reaction122Te(α, n)125m Xe using a target enriched in122Te (95.4%) and the decay of127m Xe produced by the reaction127J(d, 2n)127m Xe have been investigated: 125m Xe decays with a half-life ofT 1/2=(56±3) sec by ayy- cascade withE γ1=(140.4 ±0.5) keV andE γ2=(110.5 ±0.5) keV. The experimental conversion coefficients yield multipolarities ofE3 for the 140.4 keV isomeric transition and predominantlyM1 for the 110.5 keV-transition. 127m Xe decays with a half-life ofT 1/2=(71±2) sec. The decay also proceeds by aγγ-cascade with an isomeric E3 transition ofE γ1=(172.5±0.3) keV and a predominantlyM1 transition ofE γ2=(124.6±0.3) keV. In the decay of127g Xe an additional branching of the electron capture to a level at (618.1±0.3) keV was observed. The relative probability forK-captureP K618/PK375=0.40 ±0.07 yields a total transition energyQ EC=(664 ±4)keV. A spin of 1/2+ was assigned to the ground state.  相似文献   

12.
The electric field gradients at Eu sites in GaN have been investigated in conversion electron Mössbauer spectroscopy (CEMS) in which 151Eu probe ions were implanted into an undoped GaN layer grown on a sapphire substrate. The sample was implanted with 120 keV 151Eu ions to a fluence of 1 × 1015, and annealed at 1,200 K. CEMS spectra of the 151Eu 21.6 keV transition were collected, of the GaN sample as well as of a Si sample implanted with overlapping profiles of 151Eu and O. The GaN spectra were fitted with two symmetric doublets, D1 and D2, with isomer shifts and quadrupole splittings of δ?=??0.27 mm/s (relative to Eu2O3), ΔE Q?= 0.85 (3) mm/s; and δ?=?? 0.22 mm/s, ΔE Q?= 2.90 (5) mm/s, respectively. D1 is attributed to Eu at substitutional Ga lattice sites; D2 to Eu at or near substitutional sites but with extensive lattice damage. The splittings of D1 and D2 correspond to quadrupole coupling frequency of 15 (2) and 50 (4) MHz, consistent with measurements of 69Ga, 71Ga and 111In in GaN.  相似文献   

13.
The isotope shift of the stable151Eu,153Eu, and the radioactive152Eu,154Eu isotopes and the hyperfine splitting of the152Eu isotope was investigated using a digital recording Fabry-Perot-spectrometer. From isotope shift measurements on the line λ 5 765 Å (4f 7 6s 6p z6P7/2-4f 7 6s2 a8S7/2) the relative isotope shift was derived:151Eu:0;152Eu: 0.923(8);153Eu: 1;154Eu: 1.197(8). The results show that there is a strong increase in the change of the mean square nuclear charge radius δ〈r2〉 when only one neutron is added to the 88 neutrons of the151Eu nucleus, whereas the change of δ〈r2〉 between152Eu and153Eu is of the same order of magnitude as that between153Eu and154Eu. From the hyperfine splitting of the radioactive isotope152Eu in the line δ 6865 Å (4f 7 6s 6p z 10 P 9/2-4f 7 6s2 a8S7/2) the sign of the magnetic dipole moment μI(152Eu) was found to be negative, and with this result and earlier experimental data the signs of the nuclear quadrupole momentsQ(152Eu) andQ (154Eu) could be determined to be positive.  相似文献   

14.
The 21.7 keV nuclear gamma resonance of 151Eu was used for studying the inhomogeneous mixed-valent compound Eu3S4 in the pressure range 0–15 kbar. At room temperature the activation energy for electron hopping between the crystallographically equivalent divalent and trivalent Eu sites was found to decrease with pressure by dEa/dP=-1.8±0.3 meV kbar-1. No change of the mean valence of Eu with pressure was observed.  相似文献   

15.
The Coster-Kronig and Auger spectrum of theL 1 shell of gaseous argon has been investigated with an electrostatical spectrometer. The ionization in theL 1 shell of argon was caused by electron impact. Absolute energies and relative intensities of all the Coster-Kronig and Auger transitions have been determined. The relative intensities of transitions within the groupsL 1 L 2, 3 M 1,L 1 L 2, 3 M 2, 3 andL 1 MM agree fairly well with the theoretical values, calculated byRubenstein for extreme Russel-Saunders coupling, if intermediate coupling theory is used properly. Via the widthγ(L 1) of theL 1 level of argon, found in this experiment to be (1.84±0.2) eV, the following absolute group transition probabilities were determined (in units of 1014 sec?1):W(L1 L 2, 3 M 1)=(5.5±1.0),W(L1 L 2, 3 M 2, 3)=(20.8±2.8),W(L1 MM)=(1.44±0.16). The theoretical values are 21.0, 20.4 and 1.27. The possible reason for the large discrepancy between the experimental and theoretical value ofW(L1 L 2, 3 M 1) is the use of the incorrect value of 287 eV for the binding energyE(L1) byRubenstein. From the energies of theL 1 MM transitions this value has been determined to beE(L1)=(326.5±0.5) eV. This is the first direct measurement ofE(L1) of argon.  相似文献   

16.
In 145Eu a high-spin isomer with E level = 8528 keV and T 1/2 = (3.7 ± 0.4) ns has been observed. The data were obtained by in-beam γ-ray spectroscopy using the reaction 122Sn(27Al,4n)145Eu at 127 MeV performed at the NORD-BALL spectrometer in Roskilde.  相似文献   

17.
A 53.3 keV E2 transition de-exciting the 60 ns isomer in152Dy has been identified in γγ-coincidence measurements, which locates that isomer at Ex=5088 keV. The half life of the 11? level at 3161 keV was measured to be T1/2=4.3±0.9 ns.  相似文献   

18.
Beta and gamma spectra of Os191 were studied using a magnetic double-focusing beta-spectrometer and a scintillation spectrometer. The isomeric state Os191m decays through the 74·4 ± 0·1 keV (E3/M4=50) transition with a half-lifeT 1/2=13·0 ± 0·5 hours. A continuous beta spectrum withE max=147 ± 3 keV and the gamma transitions 41·83 ± 0·05 keV (E3), 82·5 ± 0·3 keV and 129·4 ± 0·1 keV (70%M1 + 30%E2) were observed in the decay of the ground state of Os191. The conversion coefficient of the last transition was determined as 1·94 ±± — 0·10. Gamma transitions with energies of 47 keV and 185·8 keV were not observed.  相似文献   

19.
A camel's back-like nonparabolicity of the longitudinal electron mass enhances the density of states and strongly stabilized an electron-hole-liquid. In GaP therefore the EHL density is doubled to 8.6 × 1818cm?3 and the Fermi energy ratio EFh/EFe changes from 1.9 to 4.9. The theoretical binding energy agrees with the experimental EB=17.5±3meV interpreting the luminescence at 2.30 eV as a superposition of liquid and plasma recombination radiation.  相似文献   

20.
The isomer shift in the optical transition Eu II 4f7(8S 7 2/o )6p3/2 (7/2,3/2)4?4f7 (8S 7 2/o )5d9D 4 o , λ=6O4.95 nm, has been measured between the isotope152gEu(3?) and its isomer152mEu(0?). From the valuev(152gEu)–v(152mEu)=736(10) MHz the deformation parameter of152mEu has been estimated to be152mβ?+0.25. This value is smaller than152gβ as obtained from isotope shift measurements and the spectroscopic quadrupole moment. The influence of the shape difference on the decay of152mEu is discussed.  相似文献   

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