5,690 research outputs found
On the valence bond solid in the presence of Dzyaloshinskii-Moriya interaction
We examine the stability of the valence bond solid (VBS) phase against the
Dzyaloshinskii-Moriya (DM) interaction in the bipartite lattice. Despite the
VBS is vulnerable against the antiferromagnetic interaction, for example in the
Q-J model proposed by Sandvik, where the quantum phase transition occurs at
, we found that on the contrary the VBS is very stable against
the DM interaction. The quantum phase transition does not occur until D/Q goes
to infinity, where D is the strength of the DM interaction. The VBS in the ALKT
model and the Haldane gap system also exhibit the same property.Comment: 5 pages and 5 figure
Testing the phenomenological interacting dark energy with observational data
In order to test the possible interaction between dark energy and dark
matter, we investigate observational constraints on a phenomenological
scenario, in which the ratio between the dark energy and matter densities is
proportional to the power law case of the scale factor, . By using the Markov chain Monte Carlo method,
we constrain the phenomenological interacting dark energy model with the newly
revised data, as well as the cosmic microwave background (CMB)
observation from the 7-year Wilkinson Microwave Anisotropy Probe (WMAP7)
results, the baryonic acoustic oscillation (BAO) observation from the
spectroscopic Sloan Digital Sky Survey (SDSS) data release 7 (DR7) galaxy
sample and the type Ia supernovae (SNe Ia) from Union2 set. The best-fit values
of the model parameters are
,
, and
, which are more
stringent than previous results. These results show that the standard
CDM model without any interaction remains a good fit to the recent
observational data; however, the interaction that the energy transferring from
dark matter to dark energy is slightly favored over the interaction from dark
energy to dark matter. It is also shown that the data can give more
stringent constraints on the phenomenological interacting scenario when
combined to CMB and BAO observations, and the confidence regions of
+BAO+CMB, SNe+BAO+CMB, and +SNe+BAO+CMB combinations are consistent
with each other.Comment: 6 pages, 4 figures, 1 table. MNRAS in pres
2,3-butanediol production from cellobiose by engineered Saccharomyces cerevisiae
Production of renewable chemicals from cellulosic biomass is a critical step towards energy sustainability and reduced greenhouse gas emissions. Microbial cells have been engineered for producing fuels and chemicals from cellulosic sugars. Among these chemicals, 2,3-butanediol (2,3-BDO) is a compound of interest due to its diverse applications. While microbial production of 2,3-BDO with high yields and productivities has been reported, there are concerns with the use of potential pathogenic bacteria and inefficient utilization of cellulosic sugars. To address these problems, we engineered Saccharomyces cerevisiae to produce 2,3-BDO, especially from cellobiose which is a prevalent sugar in cellulosic hydrolyzates. Specifically, we overexpressed alsS and alsD from Bacillus subtilis to convert pyruvate to 2,3-BDO via Ξ±-acetolactate and acetoin in engineered S. cerevisiae capable of fermenting cellobiose directly. Under oxygen-limited conditions, the resulting strain was able to produce 2,3-BDO. Still, the majority of carbon flux in the strain went to ethanol, resulting in significant amounts of ethanol production. To enhance pyruvate flux to 2,3-BDO through elimination of the pyruvate decarboxylation (PDC) reaction, we employed a deletion mutant of both PDC1 and PDC5 for producing 2,3-BDO from cellobiose. The subsequent strain was able to produce only 2,3-BDO without ethanol production from cellobiose under oxygen-limited conditions. These results suggest the possibility of producing 2,3-BDO safely and sustainably from cellulosic hydrolyzates
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