1,075 research outputs found
Strange Matter: a state before black hole
Normal baryonic matter inside an evolved massive star can be intensely
compressed by gravity after a supernova. General relativity predicts formation
of a black hole if the core material is compressed into a singularity, but the
real state of such compressed baryonic matter (CBM) before an event horizon of
black hole appears is not yet well understood because of the non-perturbative
nature of the fundamental strong interaction. Certainly, the rump left behind
after a supernova explosion could manifest as a pulsar if its mass is less than
the unknown maximum mass, . It is conjectured that pulsar-like
compact stars are made of strange matter (i.e., with 3-flavour symmetry), where
quarks are still localized as in the case of nuclear matter. In principle,
different manifestations of pulsar-like objects could be explained in the
regime of this conjecture. Besides compact stars, strange matter could also be
manifested in the form of cosmic rays and even dark matter.Comment: 20 pages, 3 figures, contribution to "Centennial of general
relativity - A celebration
Project-Based Learning: an Effective Approach to Link Teacher Professional Development and Students Learning
Professional development for teachers is a key mechanism for improving classroom instruction and student achievement, yet there is little empirical evidence upon which to damonstrate the connection between teachersā professional development and studentsā achievement. This paper presents a pilot research which adopts project-based teaching and learning(PjBL) as an approch to link teahcer professional development and student learning. In our longitudinal study, a resource-rich school in urban areas and a less developed school in outlying areas join hands to carry out a research project. Study groups were composed of 2-3 teachers and 10-15 students in each school. The groups from different regions then collaboratively carried out a learning project with the support of an online learning community. The data is collected from focus groups and interviews with stakeholders, online surveys and paper-based questionnaires, computer proficiency tests, observations from site visits, and an analysis of the students\u27 artificial product. Research findings show that project-based collaborative inquiry activity provides the greatest support for teachers and students to develop their comprehensive capacity
Singular Trudinger--Moser inequality involving norm in bounded domain
In this paper, we use the method of blow-up analysis and capacity estimate to
derive the singular Trudinger--Moser inequality involving
-Finsler--Laplacian and norm, precisely, for any ,
and , we
have \begin{align} \sup_{u\in W_{0}^{1,N}(\Omega),\;\int_{\Omega}F^{N}(\nabla
u)dx-\gamma\|
u\|_p^N\leq1}\int_{\Omega}\frac{e^{\lambda_{N}(1-\frac{\beta}{N})\lvert
u\rvert^{\frac{N}{N-1}}}}{F^{o}(x)^{\beta}}\;\mathrm{d}x<+\infty\notag,
\end{align} where
and is the volume of a unit Wulff ball in ,
moreover, extremal functions for the inequality are also obtained. When
and , we can obtain the singular version of Tintarev
type inequality by the obove inequality, namely, for any
and , it holds
where and is the volume of unit ball in . Our results extend
many well-known Trudinger--Moser type inequalities to more general setting
Identification of candidate genes involved in wax deposition in Poa pratensis by RNA-seq
A, Randomness test of cDNA fragments; B, Sequencing saturation analysis. T1 and T2 represent NEZm; T3 and T4 represent EBZ. (PDF 290 kb
Contagion processes on the static and activity driven coupling networks
The evolution of network structure and the spreading of epidemic are common
coexistent dynamical processes. In most cases, network structure is treated
either static or time-varying, supposing the whole network is observed in a
same time window. In this paper, we consider the epidemic spreading on a
network consisting of both static and time-varying structures. At meanwhile,
the time-varying part and the epidemic spreading are supposed to be of the same
time scale. We introduce a static and activity driven coupling (SADC) network
model to characterize the coupling between static (strong) structure and
dynamic (weak) structure. Epidemic thresholds of SIS and SIR model are studied
on SADC both analytically and numerically with various coupling strategies,
where the strong structure is of homogeneous or heterogeneous degree
distribution. Theoretical thresholds obtained from SADC model can both recover
and generalize the classical results in static and time-varying networks. It is
demonstrated that weak structures can make the epidemics break out much more
easily in homogeneous coupling but harder in heterogeneous coupling when
keeping same average degree in SADC networks. Furthermore, we show there exists
a threshold ratio of the weak structure to have substantive effects on the
breakout of the epidemics. This promotes our understanding of why epidemics can
still break out in some social networks even we restrict the flow of the
population
An Ultra Low Mass and Small Radius Compact Object in 4U 1746-37?
Photospheric radius expansion (PRE) bursts have already been used to
constrain the masses and radii of neutron stars. RXTE observed three PRE bursts
in 4U 1746-37, all with low touchdown fluxes. We discuss here the possibility
of low mass neutron star in 4U 1746-37 because the Eddington luminosity depends
on stellar mass. With typical values of hydrogen mass fraction and color
correction factor, a Monte-Carlo simulation was applied to constrain the mass
and radius of neutron star in 4U 1746-37. 4U 1746-37 has a high inclination
angle. Two geometric effects, the reflection of the far side accretion disc and
the obscuration of the near side accretion disc have also been included in the
mass and radius constraints of 4U 1746-37. If the reflection of the far side
accretion disc is accounted, a low mass compact object (mass of
and radius of at 68% confidence)
exists in 4U 1746-37. If another effect operated, 4U 1746-37 may contain an
ultra low mass and small radius object
( at 68% confidence). Combined
all possibilities, the mass of 4U 1746-37 is at
99.7% confidence. For such low mass NS, it could be reproduced by a self-bound
compact star, i.e., quark star or quark-cluster star.Comment: accepted by Ap
Poinsettia and Easter Lily Growth and Development Responses to Root Substrate Containing Biochar
Greenhouse production of Poinsettia (Euphorbia pulcherrima) and Easter lily (Lilium longiflorum) mainly uses peat-based root substrates. The decrease of peatland has increased the need for alternative root substrate components in the horticulture industry. Biochar, a byproduct of bio-energy production, has the potential to be an alternative root substrate component to reduce the use of peatmoss in greenhouse production. The objectives of the present studies were to determine the effects of different percentages of biochar and fertigation regimes on the growth and development of āPrestige Redā poinsettia and Easter lily āNellie Whiteā in greenhouse production.
Two experiments were conducted to evaluate different percentages of one type of biochar added to a commercial peat-based root substrate for poinsettia and Easter lily greenhouse production. In experiment one, rooted poinsettia cuttings were potted in one of the six root substrates mixes including Sunshine Mix #1 replaced by 0%, 20%, 40%, 60%, 80%, or 100% biochar (by volume) and irrigated under four fertigation regimes (100 to 200 mgā¢L-1 N, 200 to 300 mgā¢L^-1 N, 300 to 400 mgā¢L^-1 N, or 400 to 500 mgā¢L^-1 N). Root rot and red bract necrosis were only observed in the highest fertigation regime (400-500 mgā¢L^-1 N) combined with the highest biochar percentage (100%). At 100 to 400 mgā¢L^-1 N fertilization rate, up to 80% of the commercial peat-based root substrate could be replaced by biochar without a significant change in poinsettia growth and quality.
In experiment two, Easter lily bulbs were potted in one of the five root substrates mixes (Sunshine Mix #1 amended with 0%, 20%, 40%, 60%, and 80% biochar) and irrigated under four fertigation regimes (constant liquid feed at 200 mgā¢L^-1 N or 300 mgā¢L^-1 N, and fertilization at every third watering with 200 mgā¢L^-1 N or 300 mgā¢L^-1 N). Neither fertigation regimes nor biochar percentages significantly affected the Easter lily growth and development. Under the four fertigation regimes used in this experiment, up to 80% peat-based root substrate could be replaced by biochar without a significant difference on the growth and development of Easter lily
Does a higher minimum wage accelerate labour division in agricultural production? Evidence from the main riceplanting area in China
Agricultural production outsourcing, a new means of agricultural
production, can optimise the allocation of resources, reduce agricultural production costs, and improve agricultural productivity.
However, farmersā outsourcing behaviours are strongly interfered
with by many factors such as economics, technology and institutions. Using a farmer-level data set from 2014 to 2018 in China,
we examine the effects of the minimum wage increase on rice
farmersā production outsourcing behaviours. Our study relies on a
Logit regression framework and uses the control function (C.F.)
approach to address potential endogeneity concerns. Results
show that the minimum wage increase significantly reduces the
probability of farmers conducting production outsourcing. We
also examine the heterogeneous effects of the minimum wage
increase, and find that compared with other outsourcing services,
the adverse effects on harvesting outsourcing are the strongest;
the negative effects on production outsourcing are stronger for
rice farmers with higher education. Our results provide new
insights into understanding how labour regulation affects labour
division in agricultural production
- ā¦