Structural, transport and optical properties of (La0.6Pr0.4)0.65Ca0.35MnO3 nanocrystals: a wide band-gap magnetic semiconductor Dalton Transactions PAPER Cite this: Dalton Trans., 2015, 44, 3109 Received 11th November 2014, Accepted 11th December 2014 DOI: 10.1039/c4dt03452j www.rsc.org/dalton Structural, transport and optical properties of (La0.6Pr0.4)0.65Ca0.35MnO3 nanocrystals: a wide band-gap magnetic semiconductor Satyam Kumar,a G. D. Dwivedi,b Shiv Kumar,a R. B. Mathur,c U. Saxena,d A. K. Ghosh,a Amish G. Joshi,c H. D. Yangb and Sandip Chatterjee*e (La0.6Pr0.4)0.65Ca0.35MnO3 system has been synthesized via a sol–gel route at different sintering tempera- tures. Structural, transport and optical measurements have been carried out to investigate (La0.6Pr0.4)0.65- Ca0.35MnO3 nanoparticles. Raman spectra show that Jahn–Teller distortion has been decreased due to the presence of Ca and Pr in A-site. Magnetic measurements provide a Curie temperature around 200 K and saturation magnetization (MS) of about 3.43µB/Mn at 5 K. X-ray photoemission spectroscopy study suggests that Mn exists in a dual oxidation state (Mn3+ and Mn4+). Resistivity measurements suggest that charge-ordered states of Mn3+ and Mn4+, which might be influenced by the presence of Pr, have enhanced insulating behavior in (La0.6Pr0.4)0.65Ca0.35MnO3. Band gap estimated from UV-Vis spectroscopy measurements comes in the range of wide band gap semiconductors (∼3.5 eV); this makes (La0.6Pr0.4)0.65Ca0.35MnO3 a potential candidate for device application. Introduction Hole doped manganite systems have been generating curiosity among scientists and engineers for more than 60 years because of their unprecedented and wide range of properties, e.g., ferromagnetism, insulator-metal transition and colossal magnetoresistive properties. The physics behind all these pro- perties is even more challenging and has attracted attentions of theoreticians and experimentalists with almost equal authority.1–11 Manganite materials have been used in different electronic devices such as magneto-tunable photocurrent devices, resistive switching devices, and spin hall magneto- resistive devices.12–18 The parent compound LaMnO3 is known to be an antiferromagnetic insulator, while divalent cation (Ca2+, Sr2+ and Ba2+) doping induces paramagnetism with polaron type conductivity at high temperatures, and metallic ferromagnetism below the Curie temperature TC. The origin of ferromagnetism has been attributed to the double-exchange interaction between the valence electronic states of Mn3+–O−2– Mn4+.19–21 The double-exchange mechanism along with the effect of lattice distortion is believed to be responsible for the occurrence of colossal magnetoresistance (CMR).22,23 As an outcome of the double-exchange interaction and the lattice distortion, a large spin splitting of the conduction band (majority and minority sub-bands) takes place in the ferro- magnetic state.8–11 Governed by the Hund’s rule, these sub- bands are separated by few electron-volts energy, which depends on A-site doping. The large spin splitting produces the half-metallic properties of the material because at Fermi level, charge carriers with only one spin direction (up/down) are present, whereas there is a gap in the density of states for the carriers with the other spin direction (down/up). Hole doped manganite systems in the nano-range act in a different way, i.e., ferromagnetic ordering and metal-insulator transition are well separated from each other. Transport pro- perties basically depend on boundary conditions. In nano- range, surface to volume ratio increases; thus, the boundary effect becomes more pronounced in transport properties. Due to more boundaries, charge carriers face much more scatter- ing, and as a result the resistivity of the system increases. However, the double exchange interaction between Mn3+ and Mn4+ is not affected by the boundary conditions, and therefore it is not affected much in the nano-phase.24 Magnetic properties of Ca doped PrMnO3 (Pr1−xCaxMnO3) materials at low temperatures are governed by Mn3+/Mn4+ ordering, intra- and inter-Mn exchange interactions and struc- tural distortions produced by the Ca2+ cations. PrMnO3 has an antiferromagnetic ground state. With Ca doping, a ferromagnetic ground state develops for x = 0.2. The charge-ordering of the Mn-ions occurs over a wide range from 0.3 < x < 0.75 with an aDepartment of Physics, Banaras Hindu University, Varanasi-221005, India bDepartment of Physics, National Sun Yat-sen University, Kaohsiung-80424, Taiwan cCSIR-National Physical Laboratory, Dr. K.S. Krishnan Road, New Delhi-110012, India dDepartment of Physics, Mahila Mahavidyalaya, Banaras Hindu University, Varanasi-221005, India eDepartment of Physics, Indian Institute of Technology (Banaras Hindu University), Varanasi-221005, India. E-mail: schatterji.app@iitbhu.ac.in This journal is © The Royal Society of Chemistry 2015 Dalton Trans., 2015, 44, 3109–3117 | 3109 P ub li sh ed o n 08 J an ua ry 2 01 5. D ow nl oa de d by N at io na l P hy si ca l L ab or at or y (N P L ) on 2 0/ 11 /2 01 5 06 :4 1: 07 . View Article Online View Journal | View Issue www.rsc.org/dalton http://crossmark.crossref.org/dialog/?doi=10.1039/c4dt03452j&domain=pdf&date_stamp=2015-01-29 http://dx.doi.org/10.1039/c4dt03452j http://pubs.rsc.org/en/journals/journal/DT http://pubs.rsc.org/en/journals/journal/DT?issueid=DT044007 ordering temperature near 250 K.25,26 Pr0.65Ca0.35MnO3 shows insulating behavior in both the paramagnetic and ferromagnetic states because of the charge-ordered state of Mn3+ and Mn4+.27 Magnetic and transport properties of manganites have been studied with great interest and enthusiasm by scientists and will be continued to be studied in the future because of the vast range of properties these systems possess which make them desirable from an application point of view. However, studies have not been done concerning their optical properties because these systems show either insulator (large band gap; typically >4 eV) behavior or metallic (no band gap) behavior, which makes them less interesting for optical studies. In this manuscript, we have doped 40% Pr in the La site of La0.65Ca0.35MnO3 system, which shows metallic ferromagnetic behavior below 260 K.28 The idea behind the doping of Pr is that the Pr0.65Ca0.35MnO3 system shows ferromagnetic charge- ordered insulator behavior. We are expecting that with the doping of Pr, the semiconducting behavior will increase because of the stabilization of charge-ordering, along with the sustaining magnetic order of the system. Along with a strong magnetic moment, if we can induce a semiconducting nature, these systems can be used as a better candidate to improve magnetic semiconducting devices. To realize this pheno- menon, we have used La0.65Ca0.35MnO3 nanoparticles, which show better semiconducting nature along with ferromagnetic ordering as compared to its bulk counterpart. In addition, the doping of Pr may also increase its semiconducting behavior without disturbing the magnetic ordering. We are using par- ticularly 40% of Pr doping in the La site because excess doping results in a completely insulating phase, while doping less than 40% decreases the band gap significantly,10 and both the cases are not favorable for application purpose. Experimental section (La0.6Pr0.4)0.65Ca0.35MnO3 samples were synthesized using the sol–gel method. Analytical grade metal oxides Pr6O11, La2O3, and CaCO3 powders were taken in stoichiometric proportions (0.39 mol: 0.26 mol: 0.35 mol) and dissolved in nitric acid (HNO3) and thoroughly mixed for 30 minutes. The prepared solution of metal nitrates along with Mn(NO3)3·4H2O (1 mol) were mixed in aqueous solution of citric acid [C6H8O7] (99.5% purity) with stirring, to obtain a homogeneous precursor solu- tion. Citric acid serves as the fuel for the reaction. In this solu- tion, ethylene glycol was added drop wise with stirring. Citric acid, ethylene glycol and metal nitrates were precisely taken in a 4 : 3 : 1 molar ratio. The precursor solution was dried at 200 °C for 12 h in an oven to obtain xerogel and the swelled xerogel was kept at 300 °C for 5 h to dry. After grinding the xerogel, powders were sintered at 600, 800, 1000 °C for 5 h under air to obtain (La0.6Pr0.4)0.65Ca0.35MnO3 nanoparticles. Phase purity of the as-prepared (La0.6Pr0.4)0.65Ca0.35MnO3 samples were checked with a Model: Philips X’pert ProX-ray diffractometer using CuKα radiation (λ = 1.5406 Å). Transmission electron microscopy measurements were done with a JEOL-2010 (Japan). Raman spectra were obtained with a Renishaw micro- Raman spectroscope in the range of 100 cm−1–1000 cm−1 using 514.5 nm Ar+ laser as the excitation source. Fourier transform infrared (FTIR) spectroscopy measurements were done with an FTIR Spectrometer (Spectrum One, Perkin Elmer Instrument, USA) in the range of 4000–400 cm−1 with a resolu- tion of 1 cm−1. Magnetic measurements were done using a superconducting quantum interference device [Magnetic Prop- erty Measurement System (MPMS) XL-7, Quantum Design Inc.]. Room temperature X-ray photoemission spectroscopy measure- ments were done using a Omicron multiprobe surface analysis system operating at an average base pressure of ∼5 × 10−10 torr with a monochromatic AlKα line at 1486.70 eV. The total energy resolution, estimated from the width of the Fermi edge, was about 0.25 eV for monochromatic AlKα line with photon energy 1486.70 eV. Resistivity measurements were done via 2-probe method using a Keithley 2400 Source meter. The optical absorp- tion spectra were measured in the range of 220–800 nm using a UV-Vis spectrometer (SHIMADZU). Results and discussion Structural analysis X-ray diffraction patterns of (La0.6Pr0.4)0.65Ca0.35MnO3 sintered at 600 °C, 800 °C and 1000 °C have been shown in Fig. 1. All the three samples are in single phase (without any secondary phase) and crystallize in orthorhombic Pbnm space group like their extreme parents La0.65Ca0.35MnO3 and Pr0.65Ca0.35MnO3. We have determined average crystallite size (D) of all the three samples sintered at 600 °C, 800 °C and 1000 °C from the Scherrer’s formula: D ¼ 0:9λ β cos θ where λ = 1.5406 Å, wavelength of X-ray used, β is full width at half maximum (FWHM) of Bragg’s reflection plane and θ is Fig. 1 X-ray diffraction pattern of (La0.6Pr0.4)0.65Ca0.35MnO3 nanoparti- cles sintered at 600 °C, 800 °C and 1000 °C. Paper Dalton Transactions 3110 | Dalton Trans., 2015, 44, 3109–3117 This journal is © The Royal Society of Chemistry 2015 P ub li sh ed o n 08 J an ua ry 2 01 5. D ow nl oa de d by N at io na l P hy si ca l L ab or at or y (N P L ) on 2 0/ 11 /2 01 5 06 :4 1: 07 . View Article Online http://dx.doi.org/10.1039/c4dt03452j half of the angle of the corresponding reflection plane. We have used the most intense peak (110) as a reference plane to calcu- late the crystallite size, which is observed to be about 25 nm, 27 nm and 29 nm for the samples sintered at 600 °C, 800 °C and 1000 °C, respectively. We have also estimated the strain using the Williamson–Hall method.29 The average strain values for different sizes of (La0.6Pr0.4)0.65Ca0.35MnO3 are given in Table 1. To study the surface morphology and microstructure of (La0.6Pr0.4)0.65Ca0.35MnO3 nanocrystals, low-resolution trans- mission electron microscopy (TEM) measurements have been performed. Due to the strong magnetic moment, particles are strongly agglomerated with each other to make irregular shapes and sizes, which makes it rather difficult to distinguish one from the other. Estimated average grain sizes of the three samples sintered at 600 °C, 800 °C and 1000 °C is observed to be about 36 nm, 38 nm and 42 nm respectively, which is con- sistent with the X-ray diffraction results, which suggests increase in crystallite sizes with increasing sintering tempera- ture (Fig. 2(a, c and e)). Selected area electron diffraction (SAED) images show increase in crystalline nature of (La0.6Pr0.4)0.65Ca0.35MnO3 system with increase in sintering temperature (Fig. 2(b, d and f)). (La0.6Pr0.4)0.65Ca0.35MnO3 sin- tered at 1000 °C shows much clearer and brighter Bragg’s spots than the rest of the two systems sintered at 600 °C and 800 °C, which indicates the better crystalline nature of this system. X-ray diffraction, low-resolution TEM and SAED measurements have confirmed the single crystalline nature of our samples with almost homogeneous distribution. Raman spectroscopy To investigate crystal structure, lattice distortions and defects, Raman spectroscopy is considered to be the most powerful non-destructive technique. We doped 40% Pr in the La-site of La0.65Ca0.35MnO3 to obtain magnetic semiconductor materials. To study the effect of doping on the crystal struc- ture and lattice distortions, we obtained Raman spectra of (La0.6Pr0.4)0.65Ca0.35MnO3 nanoparticles sintered at 600 °C, 800 °C and 1000 °C, which have been shown in Fig. 3. In the orthorhombic rare-earth manganites, Raman modes become active due to deviations from the ideal cubic perovskite struc- ture. Group theory analysis of the LaMnO3 structure suggests 60 normal modes. Among all these 60 modes, only 24 modes are Raman active and the remaining modes are infrared (IR) active.30 Γoptical ¼ ð7Ag þ 7B1g þ 5B2g þ 5B3gÞRaman þ ð8Au þ 10B1u þ 8B2u þ 10B3uÞIR Table 1 Particle sizes estimated from X-ray diffraction and TEM, and average strain estimated using Williamson–Hall method Samples Average strain (estimated using Williamson–Hall method) Particle size (nm) (estimated from XRD data) Particle size (nm) (estimated from TEM) (La0.6Pr0.4)0.65Ca0.35MnO3 sintered at 600 °C 1.58 × 10 −3 25 36 (La0.6Pr0.4)0.65Ca0.35MnO3 sintered at 800 °C 2.75 × 10 −3 27 38 (La0.6Pr0.4)0.65Ca0.35MnO3 sintered at 1000 °C 4.92 × 10 −3 29 42 Fig. 2 Low-resolution transmission electron micrographs and their corresponding selected area electron diffraction images of (La0.6Pr0.4)0.65Ca0.35MnO3 nanoparticles sintered at 600 °C (a, b), 800 °C (c, d) and 1000 °C (e, f). Fig. 3 Raman spectra of (La0.6Pr0.4)0.65Ca0.35MnO3 nanoparticles sin- tered at 600 °C, 800 °C and 1000 °C. Dalton Transactions Paper This journal is © The Royal Society of Chemistry 2015 Dalton Trans., 2015, 44, 3109–3117 | 3111 P ub li sh ed o n 08 J an ua ry 2 01 5. D ow nl oa de d by N at io na l P hy si ca l L ab or at or y (N P L ) on 2 0/ 11 /2 01 5 06 :4 1: 07 . View Article Online http://dx.doi.org/10.1039/c4dt03452j These 24 Raman active modes can be divided into 2 sym- metric modes, 4 asymmetric stretching modes, 4 bending modes, 6 rotation/tilt modes of the octahedral, and the remaining 8 modes are associated with the motion of A-site (La/Pr/Ca) cations. All these Raman modes become active because of 4 fundamental distortions from the ideal perovskite structure, namely, rotations of MnO6 octahedra around the cubic [001]c and [110]c axes, Jahn–Teller distortion, and A-site (La/Pr/Ca) shift from its position in the ideal perovskite lattice. The Raman spectra of (La0.6Pr0.4)0.65Ca0.35MnO3 sintered at 600 °C, 800 °C and 1000 °C do not show any phase changes due to change in sintering temperature (Fig. 3). We observed 3 distinct Raman modes in 200–800 cm−1 range; first, around 230 cm−1, second around 500 cm−1 and third around 680 cm−1. The Raman mode around 680 cm−1 assigned as B2g(1) is related to the symmetric stretching vibration of oxygen in MnO6 octahedra. However, a very broad Raman mode around 500 cm−1 can be divided into two distinct modes, namely, 460 cm−1(Ag(1)) and 520 cm −1 (B2g(2)), related to the Jahn–Teller type asymmetric stretching mode and sym- metric bending modes of MnO6 octahedra, respectively. Dediu et al.31 reported that Pr0.65Ca0.35MnO3 shows no variation in Raman spectra above the charge-ordered transition tempera- ture (TCO), while below TCO, Raman mode near 475 cm −1 has been divided into two modes: Ag(1) and B2g(2). In our case, due to the presence of Ca and Pr in A-site, the Jahn–Teller dis- tortion at room temperature further suppressed, and the Raman mode related to this becomes relatively less promi- nent.29 Consequently, the modes around 500 cm−1 are not con- siderably distinguishable. The Raman mode around 230 cm−1 denoted as Ag(2) is related to the tilting of MnO6 octahedra. Raman modes observed in the range of 100–200 cm−1 are pre- dominantly because of the vibrations of A-site cations. Fourier transform infrared spectroscopy To get information about the molecular and functional species present on the surface and to further investigate lattice vibration present in our system, we used Fourier transform infrared (FTIR) spectroscopy. FTIR measurements of (La0.6Pr0.4)0.65Ca0.35MnO3 sintered at 600 °C, 800 °C and 1000 °C have been shown in Fig. 4. In the finger-print region, the band around 600 cm−1 corresponds to the characteristic Mn–O bond. This confirms that each sample strongly contains Mn–O bond and a change in the bond length of Mn–O–Mn, because of the internal motion, is responsible for the band for- mation. Stretching vibration is responsible for the change in Mn–O–Mn length, while bending vibration involves the change of Mn–O–Mn bond angle. The peaks at 1400 and 1630 cm−1 corresponds to the asymmetric stretching vibrations of CvC bond and symmetric stretching of CvO bond in citrate (which formed in the solution and may be present on the surface of nano-crystals). Magnetic properties To investigate the magnetic properties of (La0.6Pr0.4)0.65- Ca0.35MnO3 nanoparticles sintered at 600 °C, 800 °C and 1000 °C, we performed temperature dependent field cooled magnetization measurements (M–T) from 300 K to 5 K at 100 Oe magnetic field (Fig. 5). M–T measurement of all the samples show that ferromagnetic transition occurs around 200 K and particle size is not showing any significant effect on Curie temperature, but it is considerably affecting the mag- netic moment. (La0.6Pr0.4)0.65Ca0.35MnO3 sintered at 600 °C, 800 °C and 1000 °C show magnetic moments of 6.58 emu gm−1, 8.56 emu gm−1 and 7.53 emu gm−1, respectively, at 5 K. At a low magnetic field, the (La0.6Pr0.4)0.65Ca0.35MnO3 sintered at 800 °C shows a higher magnetization value than the (La0.6Pr0.4)0.65Ca0.35MnO3 sintered at 1000 °C; however, at a Fig. 4 Fourier transform infrared spectroscopy of (La0.6Pr0.4)0.65- Ca0.35MnO3 nanoparticles sintered at 600 °C, 800 °C and 1000 °C. Fig. 5 Field cooled temperature dependent magnetization measure- ments of (La0.6Pr0.4)0.65Ca0.35MnO3 nanoparticles sintered at 600 °C, 800 °C and 1000 °C at 100 Oe magnetic field down to 5 K. Inset figure shows the M–H hysteresis loop up to 5 T magnetic field at 5 K. Paper Dalton Transactions 3112 | Dalton Trans., 2015, 44, 3109–3117 This journal is © The Royal Society of Chemistry 2015 P ub li sh ed o n 08 J an ua ry 2 01 5. D ow nl oa de d by N at io na l P hy si ca l L ab or at or y (N P L ) on 2 0/ 11 /2 01 5 06 :4 1: 07 . View Article Online http://dx.doi.org/10.1039/c4dt03452j higher field (La0.6Pr0.4)0.65Ca0.35MnO3 sintered at 1000 °C shows a higher saturated magnetic moment. Calculated satur- ation magnetization (Ms) of (La0.6Pr0.4)0.65Ca0.35MnO3 is observed to be around 3.65µB/Mn (with 65% of Mn 3+ and 35% of Mn4+). M–H measurements at 5 K show that 5 T magnetic field gives saturation magnetization of 2.49µB/Mn, 3.03µB/Mn and 3.43µB/Mn for (La0.6Pr0.4)0.65Ca0.35MnO3 sintered at 600 °C, 800 °C and 1000 °C, respectively (inset Fig. 5). Mag- netic moment observed for (La0.6Pr0.4)0.65Ca0.35MnO3 sintered at 1000 °C is very close to the calculated magnetic moment 3.65µB/Mn. This shows that with increasing particle size, mag- netic response increases consistently and approaches the mag- netic moment of bulk (La0.6Pr0.4)0.65Ca0.35MnO3. This confirms the strong ferromagnetic character of our samples below 200 K. The ferromagnetic behavior of a similar (La0.7Pr0.3)0.65- Ca0.35MnO3 has been reported earlier, 32 which is consistent with our result. X-ray photoemission spectroscopy X-ray photoemission spectroscopy (XPS) study has been done to investigate the chemical state of (La0.6Pr0.4)0.65Ca0.35MnO3 nanoparticles sintered at 600 °C, 800 °C and 1000 °C (Fig. 6). A survey scan of (La0.6Pr0.4)0.65Ca0.35MnO3 sintered at 600 °C, 800 °C and 1000 °C confirms the presence of La, Pr, Ca, Mn and O on the surface (Fig. 6(a)). High resolution XPS core level spectra of Ca2p, O1s, and Mn2p regions have been shown in Fig. 6(b), (c) and (d) respectively. In the Ca2p region, peaks observed at 345.5 eV and 349 eV have been denoted as Ca2p3/2 and Ca2p1/2. The spin–orbit splitting energy is 3.5 eV, which indicates that the Ca exists in +2 oxidation state. In O1s region, two peaks at 528.7 eV and 530.7 eV are attributed to the contribution of the crystal lattice oxygen and adsorbed oxygen, respectively. The adsorbed oxygen has a tendency to bind with oxygen vacancies (Vo). In the Mn2p region, the two Fig. 6 (a) Survey scan X-ray photoemission spectroscopy (XPS) for (La0.6Pr0.4)0.65Ca0.35MnO3 nanoparticles sintered at 600 °C, 800 °C and 1000 °C. High resolution core level XPS of (b) Ca2p region, (c) O1s region, (d) Mn2p region for (La0.6Pr0.4)0.65Ca0.35MnO3 nanoparticles sintered at 600 °C, 800 °C and 1000 °C. (e) Deconvoluted peaks of Mn2p region for (La0.6Pr0.4)0.65Ca0.35MnO3 nanoparticles sintered at 600 °C as a representative. (f) Valence band spectra of (La0.6Pr0.4)0.65Ca0.35MnO3 nanoparticles sintered at 600 °C, 800 °C and 1000 °C. Dalton Transactions Paper This journal is © The Royal Society of Chemistry 2015 Dalton Trans., 2015, 44, 3109–3117 | 3113 P ub li sh ed o n 08 J an ua ry 2 01 5. D ow nl oa de d by N at io na l P hy si ca l L ab or at or y (N P L ) on 2 0/ 11 /2 01 5 06 :4 1: 07 . View Article Online http://dx.doi.org/10.1039/c4dt03452j peaks are located at 641.5 and 653 eV, which belong to Mn2p3/2 and Mn2p1/2, respectively. The peaks of Mn2p3/2 and Mn2p1/2 can be deconvoluted into two peaks each. The deconvoluted peaks of Mn2p region for (La0.6Pr0.4)0.65Ca0.35MnO3 sintered at 600 °C have been shown as a representative in Fig. 6(e). The deconvoluted peaks of Mn2p3/2 at 640.88 eV and 642.85 eV (and Mn2p1/2 at 652.48 eV and 654.54 eV) represent Mn 3+ and Mn4+, respectively. This confirms that Mn exists in two oxi- dation states (+3 and +4), which participate in the double exchange interaction to give ferromagnetic ordering in the system. Valence band spectra have been shown in Fig. 6(f) for the discussed nanoparticles. The two most intense peaks around 2.7 eV and 6.2 eV are due to the strong hybridization of Mn3d(t2g) and O2p states. A weak emission near Fermi level have been detected, which belongs to Mn3d(eg) states. Similar type of features had been reported earlier in manganite materials,33,34 which supports our result. Resistivity measurement La0.65Ca0.35MnO3 shows insulator-metal transition around 260 K28 but Pr0.65Ca0.35MnO3 shows charge ordered type insu- lating behavior at low temperatures.35 The primary reason behind the formation of charge-ordered state in Pr0.65Ca0.35MnO3 is competition between double exchange and super exchange among the core spins of Mn and the coulom- bic interaction between the electrons of different orbitals of the same Mn-site.36,37 Fig. 7 shows the variation of resistivity (ρ) with respect to temperature for (La0.6Pr0.4)0.65Ca0.35MnO3 sintered at 600 °C, 800 °C and 1000 °C. The (La0.6Pr0.4)0.65- Ca0.35MnO3 system shows insulator type behavior at higher temperatures because of the development of charge-ordered states in the nano-crystalline system due to the presence of ample amount of Pr in A-sites and it is playing a dominant role in the transport behavior of the system at higher tempera- tures; however, at low temperatures, double exchange inter- action becomes more dominant and the system starts to behave as a metal. The insulator-metal transition temperature (TIM) and resistivity (ρ) of nanoparticles depend on the sinter- ing temperature of the system and decrease with increase of sintering temperature. In other words, insulator-metal tran- sition temperature depends on the particle size of the nano- crystals. As we have seen in X-ray diffraction analysis and low- resolution transmission electron microscopy analysis, particle size increases with increase in sintering temperature. Due to the increase in particle (grain) size, the effect of grain bound- ary reduces and consequently the charge carrier faces less scat- tering from grain boundaries. This factor also improves the double exchange interaction mechanism and the system starts to show metal-insulator transition at higher temperatures, and the resistivity of the system also decreases significantly. The resistivity of (La0.6Pr0.4)0.65Ca0.35MnO3 sintered at 600 °C, 800 °C and 1000 °C can be well fitted by ρ = ρ0exp(Ea/ kBT) for the nearest-neighbour hopping of small polarons (Fig. 8), where kB is the Boltzmann’s constant and Ea is the activation energy. The activation energy (Ea) for the samples was calculated using the small polaron theory, and values are given in Table 2. With increase in sintering temperature, the resistivity decreases and Ea increases. The linear fit shows that thermally activated band conduction is the dominant mechan- ism in the high-temperature region. The deviation from the linear fit indicates that the thermal activation mechanism is not valid in the low-temperature region. The variable-range- hopping (VRH) conduction of polarons has been found to dominate in this temperature region. The conduction mechan- ism due to the variable range hopping of polaron at low temp- erature can be described by the Mott’s equation38–40 ρ(T) = ρ0exp[T0/T] 1/4, where ρ0 and T0 are constants and are given by ρ0 = {[8παkBT/N(EF)] 1/2}/(3e2νph) and T0 = 18α 3/[kBN(EF)], where νph (∼10 13 s−1) is the phonon frequency at Debye temperature, N(EF) is the density of localized electron states at the Fermi level, and α is the inverse localization length. Using the above equations, a linear plot is expected from ln(ρT−1/2) versus (1/T)1/4 for VRH conduction. The linear fit of ln(ρT−1/2) versus (1/T)1/4 plot (see inset Fig. 8) indicates that VRH is the dominant mechanism of conduction below a certain temperature Th. The Th values are 165 K, 147 K and 140 K for the samples sintered at 600 °C, 800 °C and 1000 °C. The average hopping distance (R) and average hopping energy (Eh) at 150 K have been calcu- lated from R = [9/8παkBTN(EF)] 1/4 and Eh = 3/[4πR 3N(EF)]. Other conditions for VRH conduction41 are that the value of αR > 1 and that Eh > kBT. Both of these conditions are satisfied in all the studied samples (see Table 2). It is not possible that the variation of particle sizes can change the N(EF), which in effect can account for the large decrease of T0. However, the decrease of T0 may indicate the increase of localization length α −1 which leads to electronic delocalization. Ultraviolet-visible spectroscopy To investigate the optical absorbance and evaluate the optical band gap of (La0.6Pr0.4)0.65Ca0.35MnO3, we obtained ultraviolet- visible (UV-Vis) spectra. UV-Vis spectroscopy measurements have been done for (La0.6Pr0.4)0.65Ca0.35MnO3 sintered at 600 °C, 800 °C and 1000 °C (Fig. 9). UV-Vis spectra of all the Fig. 7 Variation of resistivity with temperature of (La0.6Pr0.4)0.65- Ca0.35MnO3 nanoparticles sintered at 600 °C, 800 °C and 1000 °C. Paper Dalton Transactions 3114 | Dalton Trans., 2015, 44, 3109–3117 This journal is © The Royal Society of Chemistry 2015 P ub li sh ed o n 08 J an ua ry 2 01 5. D ow nl oa de d by N at io na l P hy si ca l L ab or at or y (N P L ) on 2 0/ 11 /2 01 5 06 :4 1: 07 . View Article Online http://dx.doi.org/10.1039/c4dt03452j three samples can be divided into three parts: (i) a sharp absorption edge around 308 nm (ultraviolet region), (ii) an exponential decay region near the absorption edge (ultraviolet to visible region) and (iii) a long smooth extended region (visible to infra-red region). The optical absorption edge has been analyzed as follows:42 αhν / αðhν � EgÞn where n is equal to 12 and 2 for direct and indirect transitions, respectively, while absorption coefficient ‘α’ can be calculated from the following equation: αðνÞ ¼ 2:303 � ðA=dÞ where ‘A’ is the optical absorbance, and ‘d’ is the thickness of the sample. The variations of (αhν)2 with photon energy hν for (La0.6Pr0.4)0.65Ca0.35MnO3 sintered at 600 °C, 800 °C and 1000 °C have been plotted in Fig. 10. (αhν)2 varies linearly for a very wide range of photon energy (hν), which suggests direct type of transitions in these systems. The intercepts of these plots on the energy axis give the energy band gaps of the systems. Direct band gaps of (La0.6Pr0.4)0.65Ca0.35MnO3 sin- tered at 600 °C, 800 °C and 1000 °C determined from these plots are 3.52 eV, 3.46 eV and 3.42 eV, respectively. The decrease in band gap (red-shift) with increasing sintering temperature can be attributed to increased particle sizes, which have been related to the increased metallic behavior in Fig. 8 Variation of ln ρ as function of 1000/T for (La0.6Pr0.4)0.65- Ca0.35MnO3 nanoparticles sintered at 600 °C, 800 °C and 1000 °C in low temperature region (for T > 164 K, 147 K and 140 K, respectively). Inset: ln(ρT−1/2) vs. T−1/4 in lower temperature region (for T < 164 K, 147 K and 140 K, respectively, and above the metal-semiconductor tran- sition temperature). The linear fit indicates variable range hopping con- duction is active in this temperature range. Table 2 Values of various parameters of variable-range-hopping mechanism of (La0.6Pr0.4)0.65Ca0.35MnO3 and activation energy from small polaron theory Samples T0 (K) α (cm−1) (inverse localization length) R (cm) (average hopping distance) Activation energy (eV) (from SPT) Hopping energy Eh (eV) (from VRH) (La0.6Pr0.4)0.65Ca0.35MnO3 sintered at 600 °C 3.495 × 10 6 2.918 × 104 7.110 × 10−4 0.0706 3.37 × 10−6 (La0.6Pr0.4)0.65Ca0.35MnO3 sintered at 800 °C 6.141 × 10 6 2.815 × 106 1.971 × 10−6 0.1015 3.80 × 10−4 (La0.6Pr0.4)0.65Ca0.35MnO3 sintered at 1000 °C 1.000 × 10 7 1.361 × 109 9.919 × 10−8 0.1146 4.39 × 10−4 Fig. 9 Ultraviolet-visible spectra of (La0.6Pr0.4)0.65Ca0.35MnO3 nano- particles sintered at 600 °C, 800 °C and 1000 °C. Dalton Transactions Paper This journal is © The Royal Society of Chemistry 2015 Dalton Trans., 2015, 44, 3109–3117 | 3115 P ub li sh ed o n 08 J an ua ry 2 01 5. D ow nl oa de d by N at io na l P hy si ca l L ab or at or y (N P L ) on 2 0/ 11 /2 01 5 06 :4 1: 07 . View Article Online http://dx.doi.org/10.1039/c4dt03452j resistivity analysis. The observed band gaps of these systems appear in the range of wide band gap semiconductors and these values are even more than the band gap of ZnO (3.37 eV) and GaN (3.44 eV).43–45 In addition, these systems show much better magnetic ordering and magnetic moment46 than any known diluted magnetic semiconductors, which might prove significant in applications as magnetic semiconductors. The absorption coefficient near the band edge decays expo- nentially with photon energy (Fig. 9) and this dependence can be written as follows:47 α ¼ α0exp hν Eu � � where ‘α0’ is a constant and Eu is Urbach energy, defined as the width of the localized states (related to the amorphous state) present in the forbidden gap. This exponential depen- dence on photon energy may arise due to the random fluctu- ations associated with the small structural disorder present within the system. Conclusion X-ray diffraction, low-resolution TEM, SAED and X-ray photoe- mission spectroscopy (XPS) measurements have been done to confirm the phase formation, crystal quality and chemical con- stituents of our (La0.6Pr0.4)0.65Ca0.35MnO3 systems. Crystallite size and grain size calculated from XRD and TEM, respectively, confirm the nano-crystalline structure of our systems. SAED images show that the system becomes more crystalline with increasing sintering temperature. The Raman spectra of (La0.6Pr0.4)0.65Ca0.35MnO3 show typical vibration modes of perovskite structures. Raman study confirms the stretching (B2g(1)), bending (B2g(2)) and tilting (Ag(2)) modes of oxygen in MnO6 octahedra, which play a significant role in structural dis- tortion along with Jahn–Teller distortion (Ag(1)) mode, but due to the presence of Pr and Ca in A-site, Jahn–Teller distortion decreases, which is evident from the reduction of Ag(1) mode. FTIR measurements further confirm the presence of character- istic Mn–O stretching vibration mode near 600 cm−1, which is responsible for the structural distortion, magnetic and trans- port properties of this system. Magnetization measurement shows that the ferromagnetic ordering occurs around 200 K and the system shows a saturation magnetization of 3.43µB/ Mn, which is very close to the calculated value of the bulk sample. XPS measurement confirms that Mn exists in dual oxi- dation state (Mn3+ and Mn4+), which contributes to double exchange interaction and ferromagnetic ordering. Valence band spectra show two intense peaks around 2.7 eV and 6.2 eV, which is due to strong Mn3d(t2g)–O2p hybridization. Resistivity measurement shows that due to the doping of Pr in A-sites, the system started to behave like a charge ordered insu- lator and insulator-metal transition decreased up to 98 K. With the increase of particle size (by increasing sintering tempera- ture), this insulator-metal transition temperature improves to the higher temperature side. Band gap estimated from UV-Vis measurement appears in the wide band gap semiconductor range (∼3.5 eV), which is higher than ZnO (3.37 eV) and GaN (3.44 eV) systems. We believe that with wide band gap and strong magnetic properties, the (La0.6Pr0.4)0.65Ca0.35MnO3 system will certainly prove to be a potential candidate for mag- netic semiconductor device application. Acknowledgements SC is grateful to the funding agencies DST (grant no.: SR/S2/ CMP-26/2008), CSIR (grant no.: 03(1142)/09/EMR-II) and BRNS, DAE ((grant no.: 2013/37P/43/BRNS) for financial support. Satyam Kumar is grateful to UGC for financial support. Authors gratefully acknowledge Prof. O. N. Srivastava, Prof. R. S. Tiwari, Prof. P. C. Srivastava and Biophysics lab for their help in providing experimental facilities for TEM, XRD, UV-Vis and FTIR, respectively. References 1 G. Jonker and J. van Santen, Physica, 1950, 16, 337. 2 E. O. Wollan and W. C. Koehier, Phys. Rev., 1955, 100, 545. 3 R. von Helmolt, J. Weeker, B. Hopzapfel, L. Schulz and K. Samwer, Phys. Rev. Lett., 1993, 71, 2331. 4 S. Jin, T. H. Teifel, M. McCormack, R. A. Fastnacht, R. Ramesh and L. H. Chen, Science, 1994, 264, 413. 5 J. Vogier, Physica, 1954, 20, 48. 6 P. Schiffer, A. P. Raniirez, W. Bao and S. W. Cheong, Phys. Rev. Lett., 1995, 75, 3336. 7 A. P. Ramirez, J. Phys.: Condens. Matter, 1997, 9, 8171. 8 J. M. Coey, M. Viret and S. von Molnar, Adv. Phys., 1999, 48, 167. Fig. 10 Variation of (αhν)2 versus photon energy ‘hν’ plot for (La0.6Pr0.4)0.65Ca0.35MnO3 nanoparticles sintered at 600 °C, 800 °C and 1000 °C. Paper Dalton Transactions 3116 | Dalton Trans., 2015, 44, 3109–3117 This journal is © The Royal Society of Chemistry 2015 P ub li sh ed o n 08 J an ua ry 2 01 5. D ow nl oa de d by N at io na l P hy si ca l L ab or at or y (N P L ) on 2 0/ 11 /2 01 5 06 :4 1: 07 . View Article Online http://dx.doi.org/10.1039/c4dt03452j 9 M. B. Salamon and M. Jaime, Rev. Mod. Phys., 2001, 73, 583. 10 E. Dagotto, T. Hotta and A. Moreo, Phys. Rep., 2001, 344, 1. 11 M. Ziese, Rep. Prog. Phys., 2002, 65, 143. 12 Z. G. Sheng, M. Nakamura, W. Koshibae, T. Makino, Y. Tokura and M. Kawasaki, Nat. Commun., 2014, 5, 4584. 13 S. N. Jammalamadaka, J. Vanacken and V. V. Moshchalkov, Appl. Phys. Lett., 2014, 105, 033505. 14 H. Nakayama, M. Althammer, Y.-T. Chen, K. Uchida, Y. Kajiwara, D. Kikuchi, T. Ohtani, S. Geprägs, M. Opel, S. Takahashi, R. Gross, G. E. W. Bauer, S. T. B. Goennenwein and E. Saitoh, Phys. Rev. Lett., 2013, 110, 206601. 15 H. Boschker, J. Kautz, E. P. Houwman, W. Siemons, D. H. A. Blank, M. Huijben, G. Koster, A. Vailionis and G. Rijnders, Phys. Rev. Lett., 2012, 109, 157207. 16 M. Nakamura, Y. Ogimoto, H. Tamaru, M. Izumi and K. Miyano, Appl. Phys. Lett., 2005, 86, 182504. 17 Y. Ogimoto, N. Takubo, M. Nakamura, H. Tamaru, M. Izumi and K. Miyano, Appl. Phys. Lett., 2005, 86, 112513. 18 M. Minohara, Y. Furukawa, R. Yasuhara, H. Kumigashira and M. Oshima, Appl. Phys. Lett., 2009, 94, 242106. 19 C. Zener, Phys. Rev., 1951, 81, 440. 20 P. W. Anderson and H. Hasegawa, Phys. Rev., 1955, 100, 675. 21 J. Goodenough, Phys. Rev., 1955, 100, 564. 22 A. J. Millis, P. B. Littlewood and B. I. Shraiman, Phys. Rev. Lett., 1995, 74, 5144. 23 A. J. Millis, B. I. Shraiman and R. Mueller, Phys. Rev. Lett., 1996, 77, 175. 24 A. Gaur and G. D. Varma, J. Phys.: Condens. Matter, 2006, 18, 8837. 25 E. Pollert, S. Krupicka and E. Kuzmicova, J. Phys. Chem. Solids, 1982, 43, 1137. 26 Z. Jirak, S. Krupicka, Z. Somsa, M. Dlouha and S. Vratislav, J. Magn. Magn. Mater., 1985, 53, 153. 27 Y. Tomioka, A. Asamitsu, H. Kuwahara, Y. Morimoto and Y. Tokura, Phys. Rev. B: Solid State, 1996, 53, R1689. 28 B. Lorenz, A. K. Heilman, Y. S. Wang, Y. Y. Xue, C. W. Chu, G. Zhang and J. P. Franck, Phys. Rev. B: Condens. Matter, 2001, 63, 144405. 29 G. K. Williamson and W. H. Hall, Acta Metall., 1953, 1, 22. 30 J. Agostinho Moreira, A. Almeida, W. S. Ferreira, J. E. Araújo, A. M. Pereira, M. R. Chaves, J. Kreisel, S. M. F. Vilela and P. B. Tavares, Phys. Rev. B: Condens. Matter, 2010, 81, 054447. 31 V. Dediu, C. Ferdeghini, F. C. Matacotta, P. Nozar and G. Ruani, Phys. Rev. Lett., 2000, 84, 4489. 32 H. Sakaiand and Y. Tokura, Appl. Phys. Lett., 2008, 92, 102514. 33 A. Santoni, G. Speranza, M. R. Mancini, F. Padella, L. Petrucci and S. Casadio, J. Phys.: Condens. Matter, 1999, 11, 3387. 34 A. Kowalczyk, J. Baszyński, A. Szajek, A. Ślebarskiand and T. Toliński, J. Phys.: Condens. Matter, 2001, 13, 5519. 35 A. Biswas and I. Das, Phys. Rev. B: Condens. Matter, 2006, 74, 172405. 36 J. van den Brink and D. Khomskii, Phys. Rev. Lett., 1999, 82, 1016. 37 J. van den Brink, G. Khaliullin and D. Khomskii, Phys. Rev. Lett., 1999, 83, 5118. 38 N. F. Mott, J. Non-Cryst. Solids, 1968, 1, 1. 39 N. Sharma, S. Granville, S. C. Kashyap and J.-P. Ansermet, Phys. Rev. B: Condens. Matter, 2010, 82, 125211. 40 G. D. Dwivedi, K. F. Tseng, C. L. Chan, P. Shahi, J. Lourembam, B. Chatterjee, A. K. Ghosh, H. D. Yang and S. Chatterjee, Phys. Rev. B: Condens. Matter, 2010, 82, 134428. 41 N. F. Mott and E. A. Davis, Electronics Process in Non-Crystal- line Materials, Clarendon, Oxford, U.K., 1979. 42 N. F. Mott and R. W. Gurney, Electronic Processes in Ionic Crystals, Oxford Univ. Press, London, 1940. 43 A. Mang, K. Reimann and S. Rübenacke, Solid State Commun., 1995, 94, 251. 44 O. Madelung, Semiconductors-Basic Data 2nd Revised Edition, Springer, Berlin, 1996. 45 S. Kumar, S. Chatterjee, K. K. Chattopadhyay and A. K. Ghosh, J. Phys. Chem. C, 2012, 116, 16700. 46 S. Taran, S. Chatterjee and B. K. Chaudhuri, Phys. Rev. B: Condens. Matter, 2004, 69, 184413. 47 F. Urbach, Phys. Rev., 1953, 92, 1324. Dalton Transactions Paper This journal is © The Royal Society of Chemistry 2015 Dalton Trans., 2015, 44, 3109–3117 | 3117 P ub li sh ed o n 08 J an ua ry 2 01 5. D ow nl oa de d by N at io na l P hy si ca l L ab or at or y (N P L ) on 2 0/ 11 /2 01 5 06 :4 1: 07 . View Article Online http://dx.doi.org/10.1039/c4dt03452j Button 1: