256 research outputs found
Selecting between two transition states by which water oxidation intermediates on an oxide surface decay
While catalytic mechanisms on electrode surfaces have been proposed for
decades, the pathways by which the product's chemical bonds evolve from the
initial charge-trapping intermediates have not been resolved in time. Here, we
discover a reactive population of charge-trapping intermediates with states in
the middle of a semiconductor's band-gap to reveal the dynamics of two parallel
transition state pathways for their decay. Upon photo-triggering the water
oxidation reaction from the n-SrTiO3 surface with band-gap, pulsed excitation,
the intermediates' microsecond decay reflects transition state theory (TST)
through: (1) two distinct and reaction dependent (pH, T, Ionic Strength, and
H/D exchange) time constants, (2) a primary kinetic salt effect on each
activation barrier and an H/D kinetic isotope effect on one, and (3) realistic
activation barrier heights (0.4 - 0.5 eV) and TST pre-factors (10^11 - 10^12
Hz). A photoluminescence from midgap states in n-SrTiO3 reveals the reaction
dependent decay; the same spectrum was previously assigned by us to
hole-trapping at parallel Ti-O(dot)-Ti (bridge) and perpendicular Ti-O(dot)
(oxyl) O-sites using in situ ultrafast vibrational and optical spectroscopy.
Therefore, the two transition states are naturally associated with the decay of
these respective intermediates. Furthermore, we show that reaction conditions
select between the two pathways, one of which reflects a labile intermediate
facing the electrolyte (the oxyl) and the other a lattice oxygen (the bridge).
Altogether, we experimentally isolate an important activation barrier for water
oxidation, which is necessary for designing water oxidation catalysts with high
O2 turn over. Moreover, in isolating it, we identify competing mechanisms for
O2 evolution at surfaces and show how to use reaction conditions to select
between them
Signatures of pressure induced superconductivity in insulating Bi2212
We have performed several high pressure electrical resistance experiments on
Bi1.98Sr2.06Y0.68Cu2O8, an insulating parent compound of the high-Tc Bi2212
family of copper oxide superconductors. We find a resistive anomaly, a downturn
at low temperature, that onsets with applied pressure in the 20-40 kbar range.
Through both resistance and magnetoresistance measurements, we identify this
anomaly as a signature of induced superconductivity. Resistance to higher
pressures decreases Tc, giving a maximum of 10 K. The higher pressure
measurements exhibit a strong sensitivity to the hydrostaticity of the pressure
environment. We make comparisons to the pressure induced superconductivity now
ubiquitous in the iron arsenides.Comment: 5 pages, 4 figures, submitted to Phys. Rev.
Single polaron properties of the breathing-mode Hamiltonian
We investigate numerically various properties of the one-dimensional (1D)
breathing-mode polaron. We use an extension of a variational scheme to compute
the energies and wave-functions of the two lowest-energy eigenstates for any
momentum, as well as a scheme to compute directly the polaron Greens function.
We contrast these results with results for the 1D Holstein polaron. In
particular, we find that the crossover from a large to a small polaron is
significantly sharper. Unlike for the Holstein model, at moderate and large
couplings the breathing-mode polaron dispersion has non-monotonic dependence on
the polaron momentum k. Neither of these aspects is revealed by a previous
study based on the self-consistent Born approximation
ARPES kink is a "smoking gun" for the theory of high-Tc superconductors: dominance of the electron-phonon interaction with forward scattering peak
The ARPES spectra in high-Tc superconductors show four distinctive features
in the quasiparticle self-energy. All of them can be explained consistently by
the theory in which the electron phonon interaction (EPI) with the forward
scattering peak dominates over the Coulomb scattering. In particular, this
theory explains why there is no shift of the nodal kink at 70 meV in the
superconducting state, contrary to the clear shift of the anti-nodal
singularity at 40 meV. The theory predicts a ``knee''-like structure of the
imaginary part of the self-energy, which is phonon dominated for , and shows linear behavior for - due to the Coulomb scattering. Recent ARPES spectra give
that the EPI coupling constant is much larger than the Coulomb one. The
dip-hump structure in the spectral function comes out naturally from the
proposed theory.Comment: 5 pages, 3 figure
Momentum average approximation for models with electron-phonon coupling dependent on the phonon momentum
We generalize the momentum average (MA) approximation to study the properties
of models with momentum-dependent electron-phonon coupling. As in the case of
the application of the original MA to the Holstein model, the results are
analytical, numerically trivial to evaluate, exact for both zero bandwidth and
for zero electron-phonon coupling, and are accurate everywhere in parameter
space. Comparison with available numerical data confirms this accuracy. We then
show that further improvements can be obtained based on variational
considerations, using the one-dimensional breathing-mode Hamiltonian as a
specific example. For example, by using this variational MA, we obtain ground
state energies within at most 0.3% error of the numerical data.Comment: 15 pages, 10 figure
Tidal Evolution of the Earth–Moon System with a High Initial Obliquity
A giant impact origin for the Moon is generally accepted, but many aspects of
lunar formation remain poorly understood and debated. \'Cuk et al. (2016)
proposed that an impact that left the Earth-Moon system with high obliquity and
angular momentum could explain the Moon's orbital inclination and isotopic
similarity to Earth. In this scenario, instability during the Laplace Plane
transition, when the Moon's orbit transitions from the gravitational influence
of Earth's figure to that of the Sun, would both lower the system's angular
momentum to its present-day value and generate the Moon's orbital inclination.
Recently, Tian and Wisdom (2020) discovered new dynamical constraints on the
Laplace Plane transition and concluded that the Earth-Moon system could not
have evolved from an initial state with high obliquity. Here we demonstrate
that the Earth-Moon system with an initially high obliquity can evolve into the
present state, and we identify a spin-orbit secular resonance as a key
dynamical mechanism in the later stages of the Laplace Plane transition. Some
of the simulations by Tian and Wisdom (2020) did not encounter this late
secular resonance, as their model suppressed obliquity tides and the resulting
inclination damping. Our results demonstrate that a giant impact that left
Earth with high angular momentum and high obliquity () is
a promising scenario for explaining many properties of the Earth-Moon system,
including its angular momentum and obliquity, the geochemistry of Earth and the
Moon, and the lunar inclination.Comment: Accepted for the Planetary Science Journa
Uncovering a pressure-tuned electronic transition in BiSrYCu2O8 using Raman scattering and x-ray diffraction
We report pressure tuned Raman and x-ray diffraction data of
Bi1.98Sr2.06Y0.68Cu2O8 revealing a critical pressure at 21 GPa with anomalies
in six physical quantities: electronic Raman background, electron-phonon
coupling, spectral weight transfer from high to low frequency, density
dependent behaviour of phonon and magnon frequencies, and a compressibility
change in the c-axis. For the first time in a cuprate, mobile charge carriers,
lattice, and magnetism all show anomalies at a distinct critical pressure in
the same experimental setting. Furthermore, the Raman spectral changes are
similar to that seen traversing the superconducting dome with doping,
suggesting that the critical pressure at 21 GPa is related to the much
discussed critical point at optimal doping.Comment: 5 pages, 4 figures, submitted to PR
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