3,058 research outputs found
Editorial: Insect physiological changes during insect-plant interaction
The interactions between phytophagous insects and their host plants result from a long and continuous evolutionary process (Beran and Petschenka, 2022). Such ecological relationships led to an extraordinary diversity of insects and shaped their complex physiological systems (Wheat et al., 2007). The impacts of host plants on the physiology of herbivorous insects have increasingly become a paramount focus that should not be ignored. Chemical compounds’ composition of plants have not only significant variations in the inter/intra species aspect but also show spatiotemporal variations in different developmental stages and tissue types, or under changeable environments in nature, which lead to the resource assimilation and fitness challenges of insects (Delucia et al., 2012; Brütting et al., 2017). These close interations with plants affect the ecological plasticity of the performance of insect herbivores (Barker et al., 2019). Currently, in-depth exploration of the host plants’ effect on insects has become a research hotspot of insect physiology, however to test the highly complex hypothesis can be difficult. The current Research Topic aimed to highlight the recent developments on 1) how physiological changes occurred in herbivores during their interaction with host plants, 2) how these physiological changes in insects could be affected by other biotic factors
Non-relativistic Extended Gravity and its applications across different astrophysical scales
Using dimensional analysis techniques we present an extension of Newton's
gravitational theory built under the assumption that Milgrom's acceleration
constant is a fundamental quantity of nature. The gravitational force converges
to Newton's gravity and to a MOND-like description in two different mass and
length regimes. It is shown that a modification on the force sector (and not in
the dynamical one as MOND does) is more convenient and can reproduce and
predict different phenomena usually ascribed to dark matter at the
non-relativistic level.Comment: 4 pages, 2 figures. To appear in the proceedings of the 2011 Spanish
Relativity Meeting (ERE2011) held in Madrid, Spai
The connection between entropy and the absorption spectra of Schwarzschild black holes for light and massless scalar fields
We present heuristic arguments suggesting that if EM waves with wavelengths
somewhat larger than the Schwarzschild radius of a black hole were fully
absorbed by it, the second law of thermodynamics would be violated, under the
Bekenstein interpretation of the area of a black hole as a measure of its
entropy. Thus, entropy considerations make the well known fact that large
wavelengths are only marginally absorbed by black holes, a natural consequence
of thermodynamics. We also study numerically the ingoing radial propagation of
a scalar field wave in a Schwarzschild metric, relaxing the standard assumption
which leads to the eikonal equation, that the wave has zero spatial extent. We
find that if these waves have wavelengths larger that the Schwarzschild radius,
they are very substantially reflected, fully to numerical accuracy.
Interestingly, this critical wavelength approximately coincides with the one
derived from entropy considerations of the EM field, and is consistent with
well known limit results of scattering in the Schwarzschild metric. The
propagation speed is also calculated and seen to differ from the value , for
wavelengths larger than , in the vicinity of . As in all
classical wave phenomena, whenever the wavelength is larger or comparable to
the physical size of elements in the system, in this case changes in the
metric, the zero extent 'particle' description fails, and the wave nature
becomes apparent.Comment: 14 Pages, 4 figures. Accepted for publication in the Journal Entrop
A cosmological dust model with extended f(chi) gravity
Introducing a fundamental constant of nature with dimensions of acceleration
into the theory of gravity makes it possible to extend gravity in a very
consistent manner. At the non-relativistic level a MOND-like theory with a
modification in the force sector is obtained, which is the limit of a very
general metric relativistic theory of gravity. Since the mass and length scales
involved in the dynamics of the whole universe require small accelerations of
the order of Milgrom's acceleration constant a_0, it turns out that the
relativistic theory of gravity can be used to explain the expansion of the
universe. In this work it is explained how to use that relativistic theory of
gravity in such a way that the overall large-scale dynamics of the universe can
be treated in a pure metric approach without the need to introduce dark matter
and/or dark energy components.Comment: 7 pages, 1 figure. Accepted for publication in the European Physical
Journal
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