After a 6-week washout period where no training was performed, su

After a 6-week washout period where no training was performed, subjects were then randomly assigned to receive either

a protein supplement or a placebo immediately before and after resistance exercise. Training consisted of 6– 8 sets BV-6 in vivo of elbow flexion carried out 3 days a week for 12 weeks. No significant differences were found in muscle volume or anatomical cross-sectional area between groups. Discussion Despite claims that immediate post-exercise nutritional intake is essential to maximize hypertrophic gains, evidence-based support for such an “anabolic window of opportunity” is far from definitive. The hypothesis is based largely on the pre-supposition that training is carried out in a fasted state. During fasted exercise, a concomitant increase in muscle protein breakdown causes the pre-exercise net negative amino acid balance to persist in the post-exercise period despite training-induced increases in muscle protein selleck chemicals synthesis [36]. Thus, in the case of resistance training after an overnight fast, it would make sense to provide immediate nutritional intervention–ideally in the form of a combination of protein and carbohydrate–for the purposes of promoting muscle protein synthesis and reducing proteolysis, thereby switching a

net catabolic state into an anabolic one. Over a chronic period, this tactic could conceivably lead cumulatively to an increased rate of gains in muscle mass. This inevitably begs the question of how pre-exercise nutrition might influence the urgency or effectiveness of post-exercise nutrition, since not everyone engages in fasted training. In practice, it is common for those with the primary goal of increasing muscular size and/or

strength to make a concerted effort to consume a pre-exercise meal within 1-2 hours prior to the bout in attempt to maximize training performance. Depending on its size and composition, this meal can conceivably function as both a pre- and an immediate post-exercise Galactosylceramidase meal, since the time course of its digestion/absorption can persist well into the recovery period. Tipton et al. [63] observed that a relatively small dose of EAA (6 g) taken immediately pre-exercise was able to elevate blood and muscle amino acid levels by roughly 130%, and these levels remained elevated for 2 hours after the exercise bout. Although this finding was subsequently challenged by Fujita et al. [64], other research by Tipton et al. [65] showed that the ingestion of 20 g whey taken immediately pre-exercise elevated muscular uptake of amino acids to 4.4 times pre-exercise resting levels during exercise, and did not return to baseline levels until 3 hours post-exercise. These data indicate that even minimal-to-moderate pre-exercise EAA or high-quality protein taken immediately before resistance training is capable of sustaining amino acid delivery into the post-exercise period.

The production of these compounds is associated with hypo-osmotic

The production of these compounds is associated with hypo-osmotic stress tolerance in rhizobia [47]. The higher sensitivity of the rosR mutants to hypo-osmotic stress might be explained by increased check details permeability of their cell envelopes, which could allow excretion of greater amounts of neutral polysaccharides. Recently, several other osmotically unstable rhizobial mutants have been described, among them salt-sensitive mutants of S. meliloti, some of them significantly affected in competing against the wild type for nodule occupancy [48]. Mutation in S. meliloti regulatory gene nesR affected competition for nodulation, adaptation to high osmolarity, and nutrient

starvation [49]. Also, genes encoding trehalose biosynthesis pathways and potassium uptake systems were found to be important for S. meliloti growth in hyperosmotic medium [50, 51]. R. leguminosarum bv. trifolii rosR mutants deficient in EPS production grew considerably slower than the wild type on minimal medium. Using the Biolog system, we established that the rosR mutant revealed differences in utilization of carbon and nitrogen sources in relation to the wild

type. Similarly, phenotypic analysis of S. meliloti exoS and chvI null mutants demonstrated that ExoS/ChvI regulatory system not only controls succinoglycan (EPS I) and galactoglucan (EPS II) synthesis but is also required for growth on over 21 different carbon sources [52]. Molecular motor The chvI mutant exhibited Batimastat datasheet several pleiotropic effects: failed to grow on complex medium, had an altered LPS profile, exhibited lower tolerance to acidic conditions, was hypermotile, and synthesized significantly less poly-3-hydroxybutyrate than wild type, indicating that ChvI is engaged in regulatory networks involving the cell envelope and metabolism [53]. In several studies, a connection between the production of bacterial polysaccharides and motility has been established. Both R. leguminosarum bv. trifolii

rosR mutants and the pssA mutant deficient in EPS production exhibited a significant decrease in motility. S. meliloti MucR protein that simultaneously acts as a transcriptional repressor of galactoglucan synthesis and an activator of succinoglycan synthesis [25, 54] inhibits the expression of rem encoding an activator of the expression of such genes as flaF and flgG [55]. Other regulatory proteins, such as the ExpR/Sin quorum system, are additionally engaged in the regulation of S. meliloti motility [56, 57]. A non-motile phenotype has also been described for ndvA and ndvB mutants defective in the synthesis of β-(1,2)-glucans under hypo-osmotic conditions [58, 59]. Alterations in the LPS structure often cause motility-related defects [60, 61]. The R. leguminosarum bv. viciae 3841 LPS mutant mentioned earlier was impaired in motility and biofilm formation.

All of the following results for these adsorbates are obtained ba

The corresponding adsorption energy is determined to be -211 meV. The CO molecule somewhat

favors both H and B sites, giving an identical absorption energy of -128 meV (see Figure 1g). For simplicity, the configuration at the H site is chosen as the representative for CO. All of the following results for these adsorbates are obtained based on their most favorable configurations if not specified. Table 1 Results for gas molecules on monolayer MoS 2 calculated by LDA functional Gas H site TMsite TSsite B site h E a ΔQ h E a ΔQ h E Selleckchem MAPK inhibitor a ΔQ h E a ΔQ H2 2.62 -70 0.004 2.61 -82 0.004 3.02 -49 0.008       O2 2.79 -106 0.034 2.71 -116 0.041 3.19 -64 0.020       H2O 2.59 -234 0.012 2.67 -222 0.016 3.13 -110 0.009       NH3 2.46 -250 -0.069 2.61 -222 -0.051 3.21 -100 -0.024       NO 2.68 -195 0.011 2.90 -185 0.011 2.88 -152 0.039 2.83 -211 0.022 NO2 2.65 -276 0.100       2.71 -249 0.119 2.62 -249 0.114 CO 2.95 -128 0.020 3.22 -124 0.006 3.28 -86 0.016 3.15 -128 0.013 Equilibrium height between the center of mass of the molecule and the top S-layer of the MoS2 sheet (h, in Å), adsorption energy (E a , in meV), and charge transfer from MoS2 to the molecule (ΔQ, click here in e). Negative ΔQ means charge transfer from the molecule to

MoS2. Figure 1 Adsorption configurations. Top and side views of the most favorable configurations for (a) H2, (b) O2, (c) H2O, (d) NH3, (e) NO, (f) NO2, and (g) CO on monolayer MoS2. The blue and yellow balls represent Mo and S atoms, whereas the cyanine, red, gray, and black balls represent H, O, N, and C atoms, respectively. Additionally, calculations of the gas adsorption are also these performed using GGA functional. Different from LDA functional which overestimates the adsorption energy, GGA functional usually has a tendency to underestimate it. Upon the application of the two kinds of functionals, the upper and lower bounds for adsorption

energy and other structural properties can be obtained [8]. The calculated values of equilibrium height and adsorption energy for gas molecules on MoS2 are listed in Table 2. Herein, two GGA functionals, PW91 and PBE, are used for the purpose of comparison. Both PW91 and PBE give a smaller adsorption energy compared to the LDA, whereas they show the molecules binding at an equilibrium height larger than that for LDA. For most molecules (with the exception of NO), it seems that PW91 gives more stable results than PBE, with their adsorption energy difference approximately between -7 and -28 meV. Table 2 Results for gas molecules on monolayer MoS 2 calculated by PW91 and PBE functionals Gas Site LDA GGA-PW91 GGA-PBE h E a h E a h E a H2 TM 2.61 -82 3.21 -4 3.07 6 O2 TM 2.71 -116 3.32 -11 3.40 -4 H2O H 2.59 -234 3.17 -37 3.14 -21 NH3 H 2.46 -250 2.99 -44 2.91 -24 NO B 2.83 -211 3.47 -14 3.25 -33 NO2 H 2.65 -276 3.33 -43 3.30 -15 CO H 2.95 -128 3.61 -13 3.

Competition assays were performed with nuclear extracts from cell

Competition assays were performed with nuclear extracts from cells infected with Corby for 2 h. 100-fold excess amounts of competitor were added (lanes 3 to 5). A supershift assay in the same nuclear extracts also was performed. Antibodies (Ab) were added (lanes 6 to 10). Arrows indicate specific complexes, while arrowheads indicate the DNA binding complexes supershifted. (C) Flagellin-induced p65 translocation. Cells were infected with Corby or flaA mutant. Nuclear extracts were subjected to immunoblotting. (D) Flagellin activates buy GDC-0973 NF-κB through the classical and alternative pathways. Cells were infected with Corby or flaA mutant. Lysates were subjected

to immunoblotting. (E) Overexpression of dominant negative mutants inhibits L. pneumophila-induced activation of the IL-8 promoter. Cells were transfected with -133-luc and the mutant plasmids

and then infected with Corby for 6 h. The solid bar Idasanutlin in vitro indicates luciferase activity of -133-luc and empty vector without infection. Activity is expressed relative to that of cells transfected with -133-luc with further Corby infection, which was defined as 100. Data are means ± SD values of three experiments. dn, dominant negative. *, P < 0.05; **, P < 0.001 (by Student t test). As described above, the flaA mutant strain failed to induce mRNA expression and production of IL-8. Next, we determined whether the flaA mutant strain induces NF-κB DNA binding activity. As expected, NF-κB DNA binding activity was not induced by the isogenic flaA mutant, unlike the wild-type strain Corby (Fig.

6A). These results indicate that better activation Cell press of NF-κB binding by flaA-positive strain is the underlying mechanism of the observed activation of the IL-8 promoter by this bacterial strain. Considered together, these results indicate that L. pneumophila infection induces IL-8 gene expression at least in part through the induced binding of p50 and p65 NF-κB family members to the NF-κB element of the IL-8 promoter and that this effect is dependent on flagellin. Because nuclear translocation is a key step for transcriptional activity [9], we next examined whether L. pneumophila induces the nuclear translocation of NF-κB. As shown in Fig. 6C, the wild-type Corby, but not the flaA mutant, induced nuclear translocation of NF-κB. NF-κB is normally present in the cytoplasm in an inactive state and is bound to members of the IκB inhibitor protein family, chiefly IκBα. In this complex, IκBα blocks the nuclear localization signal, thus preventing nuclear translocation. Translocation of NF-κB into the nucleus requires disruption of the cytoplasmic NF-κB:IκBα complex [9]. To determine the role of IκBα phosphorylation and degradation in L. pneumophila-induced NF-κB translocation and activation, we investigated whether L. pneumophila induces phosphorylation and degradation of IκBα.

Astron Astrophys 378:597–607CrossRef Pino T et al (2008) The 6 2 

Astron Astrophys 378:597–607CrossRef Pino T et al (2008) The 6.2 μm band position in laboratory and astrophysical spectra: a tracer of the aliphatic to aromatic evolution of interstellar carbonaceous dust. Astron Astrophys 490:665–672CrossRef Sandford SA et al (2006) Organics captured from comet 81P/Wild 2 by the Stardust spacecraft. Science 314:1720–1724PubMedCrossRef Volk K, Xiong G-Z, Kwok S (2000) Infrared space observatory spectroscopy of extreme carbon stars. Astrophys J 530:408–417CrossRef Zinner E (1998) Stellar nucleosynthesis and the selleck chemical isotopic

composition of presolar grains from primitive meteorites. Ann Rev Earth Planet Sci 26:147–188CrossRef”
“This last issue of OLEB of 2011 contains a collection of papers from ORIGINS 2011. The conference, which was jointly organized by Bioastronomy (IAU Commission 51) and ISSOL, was held in Montpellier, France from 3 to 8 July, 2011. EVP4593 nmr The joint meeting was an experiment for both organizations and was universally considered to have been a great success. It has been decided to repeat the exercise and the next conference will be held in 2014 in Nara, Japan. OLEB congratulates the two societies and, particularly, the Local Organizing Committee of ORIGINS 2011, which was chaired by Muriel Gargaud and Robert Pascal. ORIGINS 2011 photo by Innovaxiom (Paris). Open Access This article is distributed under the

terms of the Creative Commons Attribution Noncommercial License which permits any noncommercial use, distribution, and reproduction in any medium, provided the original author(s) and source are credited.”
“Introduction Lipmann (1965) assumed that, on the phosphate side, ‘the group potential might have originated with inorganic pyrophosphate (PPi) as the primitive group carrier’. The discovery that photosynthetic bacterial membrane-bound inorganic pyrophosphatase (PPase) catalyzed light-induced NADPH-cytochrome-c2 reductase phosphorylation of orthophosphate (Pi) to pyrophosphate (Baltscheffsky et al. 1966) and the capability of PPi to drive energy requiring dark reactions (Baltscheffsky

1967) supported pyrophosphate as a possible early alternative to adenosine triphosphate (ATP), the main chemical energy currency in living cells. Like the adenosine triphosphatase (ATPase), the corresponding membrane-bound PPase is also a H+-pump (Moyle et al. 1974), and can be a Na+-pump in both archaeal and bacterial membranes (Malinen et al. 2007). Support has been obtained for an earlier transport of Na+ than of H+ through biomembranes (Mulkidjanian et al. 2008a). The hyperthermophilic bacterium Thermotoga maritima, found in hydrothermal environments, as well as the mesophilic Methanosarcina mazei contain membrane-bound PPases (Tm-PPase and Mm-PPase, respectively) that are homologous to H+-PPases (Belogurov et al. 2005; Malinen et al. 2008). Both Tm-PPase and Mm-PPase have an absolute requirement for Na+, but display maximal activity in the presence of millimolar levels of K+.

Bootstrap values are shown as percentage (>50%) from 1,000 replic

Bootstrap values are shown as percentage (>50%) from 1,000 replicates for each node. The tree is unrooted tree. Scale bar represents number of nucleotide substitutions per site. GenBank accession numbers are in parenthesis. Sequences similar to the HrpL-dependent promoter consensus (GGAACC-N15-CCACTCAAT) [26–29] were detected upstream from orf1, orf6, hrpO, orf8, hrpB and orf10 (Figure 3a, b). The ORFs from orf8 to orf9, from hrpB to hrpE and from orf10 to hrcC overlap or are spaced by less than 94 nucleotides apart, suggesting that these three groups of genes are part of three distinct operons. The ORFs

from orf6 to hrcN appear to belong to the same operon, although a 114 bp gap is found between orf6 and orf7, but no promoter was found upstream from orf7. Likewise, the intergenic regions orf1 orf2 and orf3 orf4 contain 336 bp and 249 bp, respectively, but no promoter sequence selleck was identified. This HSP inhibitor analysis suggests that H. rubrisubalbicans hrp/hrc genes are probably organized in six HrpL-dependent operons. Figure 3 (a) Putative promoter sequences of the orf1,orf6, orf8, hrpB

and orf10 operons and hrpO gene of H. rubrisubalbicans. (b) Schematic conserved nucleotide bases found in the promoter regions – H. rubrisubalbicans Hrp-box. H. rubrisubalbicans hrp associated genes Two Hrp associated genes called hpaB (JN256204) and hpaB1 (JN256205) encode general T3SS chaperones, which promote secretion and translocation of multiple effectors proteins [30]. The hpaB and hpaB1 genes are predicted to belong to the TIR chaperone protein family. The hpaB1 gene was found

approximately 12 kb downstream from the hrcC gene and it encodes a small acidic chaperone. H. rubrisubalbicans T3SS effector proteins Type III secretion systems have been characterized in a variety of plant pathogenic bacteria. The structural proteins of these systems are highly conserved, but the T3SS effector proteins, that play a central role in virulence, are less conserved and difficult to identify. A BlastX search of the H. rubrisubalbicans partial genome sequence (30%) against NCBI-nr database allowed identification of five candidates of H. rubrisubalbicans effector proteins HropAN1 (H. rubrisubalbicans outer protein) (JN256208), HropAV1 (JN256209), HropF1 (JN256210), Hrop1 (JN256206) and Hrop2 (JN256207) (Table 1). Hrop1 and Hrop2 were Carteolol HCl also identified as T3SS effectors by the program EffectiveT3 (http://​www.​effectors.​org/​) [31]. The genes encoding these proteins are located apart from the hrp/hrc genes cluster. Table 1 Type III-effector proteins of H. rubrisubalbicans Putative Effector Protein Homology (Gene Bank accession number) Identity/Similarity % Predicted size aa HropAV1 type III effector, HopAV1 family [Ralstonia solanacearum] (CBJ40351.1) 56/70 784 HropAN1 type III effector Hrp-dependent outer protein [Burkholderia sp. Ch1-1] (ZP_06844144.1) 78/86 428 HropF1 XopF1 effector [Xanthomonas oryzae pv. oryzae PXO99A] (YP_001911267.

8 kb cat gene excised from pRY109) was inserted in the same trans

8 kb cat gene excised from pRY109) was inserted in the same transcriptional orientation as dba-dsbI operon at the BamHI site between the C. jejuni DNA fragments, generating suicide plasmid pUWM866. Gene versions inactivated by insertion of a resistance cassette were introduced into the C. jejuni 81-176 or 480 chromosome by the allele exchange method as described by Wassenaar et al. [24]. Construction of the C. jejuni 480 fur::cat mutant was achieved by natural transformation using C. jejuni 81-176 fur::cat chromosomal DNA. It should be pointed out that C. jejuni 480 was previously described as incapable of accepting chromosomal DNA by natural transformation [24]. Such inconsistency of experimental data

might be due to different chromosomal DNA used for natural transformation (C. jejuni 81116 vs C. jejuni 81-176). The mutant strains were obtained by two- or tri-parental mating experiments Belnacasan performed as described by Labigne-Roussel et al. [29] and Davis et al. [30]. The constructed mutants were named AG1 (C. jejuni 81-176 dba::aphA-3), AL1 (C. jejuni 81-176 dsbI::cat),

AL4 (C. jejuni 480 dsbI::cat), AG6 (C. jejuni 81-176 Δdba-dsbI::cat), AG11 (C. jejuni 81-176 fur::cat), and AG15 (C. jejuni 480 fur::cat). They demonstrated normal colony morphology and all but two had normal growth rates when cultured on BA plates. Only the C. jejuni 81-176 fur::cat and C. jejuni 480 fur::cat exhibited slower AZD6738 growth, an observation consistent with other studies on fur mutants [25]. Disruption of each gene as a result of double cross-over recombination was verified by PCR with appropriate pairs of primers flanking the insertion site (Table 2). The loss of DsbI synthesis in the constructed mutants was verified by Western blotting of whole-cell protein extracts against specific rabbit polyclonal Verteporfin in vivo anti-rDsbI antibodies. Protein manipulation, and β-galactosidase and arylsulfate sulfotransferase (AstA) assays Preparation of C. jejuni protein extracts, SDS-PAGE (sodium dodecyl sulfate polyacrylamide

gel electrophoresis) and blotting procedures were performed by standard techniques [26]. To obtain recombinant His6-DsbI protein, the 1100 bp DNA fragment containing the coding sequence for the predicted periplasmic DsbI C-region was PCR-amplified from the C. jejuni 81-176 chromosome using a primer pair: Cj17WDBam-up – Cj17WDBam-low. This fragment was cloned into the pGEM-T Easy vector and then, using BamHI restriction enzyme, into expression vector pET28a (Novagen) to generate plasmid pUWM657, whose correct construction was verified by restriction analysis and sequencing. Cytoplasm-located soluble fusion protein His6-DsbI purified from the E. coli Rosetta (DE3) LacIq strain by affinity chromatography was used for rabbit immunization (Institute of Experimental and Clinical Medicine, Polish Academy of Science, Warsaw, Poland).

Then, CH4 (3 sccm) was fed into the reactor After 30 min, the fe

Then, CH4 (3 sccm) was fed into the reactor. After 30 min, the feeding of CH4 was cut off and the reactor MDV3100 mw was cooled down to room temperature naturally in an Ar and H2 environment. The flow of all the gases

was stopped as the temperature reached close to the room temperature. On successful growth of graphene on Cu foil, polymethyl methacrylate (PMMA) (Sigma-Aldrich, average M W ~996,000, item no. 182265, 10 mg/ml in anisole) was used for the transfer of graphene onto different substrates like quartz, Si, SiO2-sputtered Si, and solar cells to study graphene quality and its electronic and optical properties. In the first step, the graphene-deposited Cu foil was attached to a glass slide with the help of a scotch tape and then ZD1839 supplier PMMA was spin coated on one side of the Cu foil. The other side of the foil was immersed into 10% HNO3 solution for 2 min to etch out the graphene from that side. Subsequently, the Cu foil was etched using FeCl3 (10% wt./vol.) for 3–4 h. The PMMA coated graphene film was transferred to the desired substrate (quartz, Si

or SiO2/Si, and solar cell) on several dips in deionized (DI) water as a cleaning step. In the final step, PMMA was etched out using acetone at 80°C for a duration of 2 h. Some residual PMMA was further removed by annealing in a H2 (500 sccm) and Ar (500 sccm) environment at a temperature of 450°C for 2 h. Solar cell fabrication In order to study the effect of graphene on photon absorption and carrier collection, we first fabricated Si solar cells with planar and untextured surfaces. A 156-mm monocrystalline silicon wafer was dipped in high-concentration alkali solution at 80°C for 1 to 2 min

to remove the roughness of the wafer. A p-n junction was then formed on the polished wafer through a high-temperature, solid-state diffusion process. Phosphorous oxy-chloride (POCl3) liquid dopant was used, and the wafers were subjected to elevated temperature Cell press in a furnace resulting in the formation of a thin layer of n-doped region (~0.5 μm). The wafers were etched using freon-oxygen (CF4) gas mixture in dry plasma etch machine to remove the junction regions created on the edge. These wafers were then chemically etched to remove the oxides and phosphorous glass formed on their surfaces. The entire backside was metallized with Ag-Al paste. Front contacts on the wafer surface were formed by screen printing the required pattern with a suitable metallic paste on them. The metal paste was dried and sintered in an infrared sintering belt furnace where temperature and belt speed were optimized to achieve a sharp temperature profile. The printed cells were then cut into smaller cells of dimension 10 mm × 10 mm for deposition of graphene. A similar printed cell is kept for comparative studies.

On the contrary, a Schottky barrier is expected to be formed betw

On the contrary, a Schottky barrier is expected to be formed between the top electrode and PCMO in the Al/PCMO/Pt and Ag/PCMO/Pt devices because the work function of Al and Ag is smaller than that of PCMO. Even though Ag has a similar work function to Al, the resistance switching ratio in the Ag/PCMO/Pt device is much smaller than that in the Al/PCMO/Pt

device. The work function is probably not the only cause of the large resistance switching of the Al/PCMO/Pt device. Figure 9 Work function and standard Gibbs free energy of formation of metal oxides of electrode metals. The standard Gibbs free energy of the formation of metal oxides is also shown together with the work function of Selleck Combretastatin A4 the electrode metals in Figure  9. The difference in the oxidation Gibbs free energy between Al and Ag shows a good correspondence with the difference in

the resistance switching behavior between the Al/PCMO/Pt and Ag/PCMO/Pt devices. An applied electric field may enhance the oxidation at the interface with the electrode metals with lower oxidation Gibbs free energy. The oxidation near the interface plays a role in the electrical hysteresis and resistance switching. The opposite switching polarity of the Ag/PCMO/Pt device to the Al/PCMO/Pt device is due to the difference in the oxidation Gibbs free energy [41]. As stated above, the resistance switching behavior was significantly different between the Ni/PCMO/Pt and Au/PCMO/Pt devices, although Au has a similar work function to Ni. This difference in the resistance check details switching also can be explained well by the difference in the oxidation Gibbs free energy between Ni and Au. Whether resistance switching can be observed or not seems to be dependent on the oxidation Gibbs free energy. Recently, an amorphous Al oxide layer find more with the thickness of several nanometers was found at the Al/PCMO interface by high-resolution transmission electron microscopy (HRTEM) [18]. It was also reported that the oxidation of Al metal in PCMO films at the Al/PCMO interface was observed by X-ray photoemission spectroscopy (XPS) [19, 20]. In order to evaluate the capacitance due to the Al oxide layer at the Al/PCMO interface,

the observed impedance spectra shown in Figure  5 were analyzed by comparing with the simulated spectra constructed on the basis of an equivalent circuit composed of parallel connection of resistance and capacitance (RC). Three sets of parallel RC components in series were required as an equivalent circuit to reproduce the observed spectra by theoretical simulation, although the experimental impedance spectra seemed to be composed of two semicircular arcs [30]. These three components can be assigned to grain bulk, grain boundary, and film-electrode interface. By fitting the experimental impedance spectra with the simulated ones, the interface resistance values of high and low resistance states were evaluated to be 915 and 15 kΩ, respectively.

8 to 10 3 mA/cm2 and the FF increased from 0 52 to 0 55 As a res

8 to 10.3 mA/cm2 and the FF increased from 0.52 to 0.55. As a result, the efficiency of 3.37% achieved by https://www.selleckchem.com/products/prt062607-p505-15-hcl.html the ITO/nc-TiO2/CdS(5)/P3HT:PCBM/PEDOT:PSS/Ag is about 13% higher than that (2.98%) of the ITO/nc-TiO2/P3HT:PCBM/PEDOT:PSS/Ag without CdS. As discussed above, one of

the reasons for the improved efficiency of the ITO/nc-TiO2/CdS(n)/P3HT:PCBM/PEDOT:PSS/Ag cells with CdS is reduced charge recombination in the cells due to the formation of CdS on the nc-TiO2 layer as an energy barrier layer. The charge recombination in organic solar cells can be represented by the dark current [31, 32]. To support this explanation, the I-V characteristics of the best ITO/nc-TiO2/P3HT:PCBM/PEDOT:PSS/Ag and ITO/nc-TiO2/CdS(5)/P3HT:PCBM/PEDOT:PSS/Ag devices in the dark are shown

in the inset of Figure 6. It can be found that the dark current density of the ITO/nc-TiO2/CdS(5)/P3HT:PCBM/PEDOT:PSS/Ag device is much smaller selleck inhibitor than that of the ITO/nc-TiO2/P3HT:PCBM/PEDOT:PSS/Ag device without CdS, which indicates that the charge recombination is suppressed by the deposited CdS nanoparticles. This result further confirmed the effectiveness of the chemical bath-deposited CdS on the nc-TiO2 film that can effectively reduce the charge recombination and improve the power conversion efficiency of the inverted polymer solar cells. Figure 6 I – V characteristics of the ITO/nc-TiO 2 /P3HT:PCBM/PEDOT:PSS/Ag and ITO/nc-TiO 2 /CdS(5)/P3HT:PCBM/PEDOT:PSS/Ag solar cells. Under an AM 1.5G (100 mW/cm2) condition and in the dark (inset). Conclusions CdS nanoparticles were deposited on a nc-TiO2 film by chemical bath deposition to improve the power conversion efficiency of the inverted solar cell with a device structure of ITO/nc-TiO2/P3HT:PCBM/PEDOT:PSS/Ag. In the case of ITO/nc-TiO2/CdS/P3HT:PCBM/PEDOT:PSS/Ag, deposited CdS does not only enhance the optical absorption but also suppresses the charge recombination. Finally, compared to that (2.98%) MYO10 of the ITO/nc-TiO2/P3HT:PCBM/PEDOT:PSS/Ag, the power

conversion efficiency of the ITO/nc-TiO2/CdS/P3HT:PCBM/PEDOT:PSS/Ag cell under white light illumination with an intensity of 100 mW/cm2 increased to 3.37% due to the increased optical absorption and the reduced recombination. Acknowledgements This work was supported by Henan University distinguished professor startup fund. References 1. Gunes S, Neugebauer H, Sariciftci NS: Conjugated polymer-based organic solar cells. Chem Rev 2007, 107:1324–1338.CrossRef 2. Dennler G, Sariciftc NS: Flexible conjugated polymer-based plastic solar cells: from basics to applications. Proc IEEE 2005, 93:1429–1439.CrossRef 3. Sun JM, Zhu YX, Xu XF, Lan LF, Zhang LJ, Cai P, Chen JW, Peng JB, Cao Y: High efficiency and high V oc inverted polymer solar cells based on a low-lying HOMO polycarbazole donor and a hydrophilic polycarbazole interlayer on ITO cathode. J Phys Chem C 2012, 116:14188–14198.CrossRef 4.