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<link href="http://arxiv.org/api/query?search_query%3Dall%3Aelectron%20AND%20all%3Aproton%26id_list%3D%26start%3D0%26max_results%3D10" rel="self" type="application/atom+xml"/>
<title type="html">ArXiv Query: search_query=all:electron AND all:proton&id_list=&start=0&max_results=10</title>
<id>http://arxiv.org/api/5SM+U4Y158JiJuDXkggxPJF18mw</id>
<updated>2025-08-20T00:00:00-04:00</updated>
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<entry>
<id>http://arxiv.org/abs/astro-ph/9904306v1</id>
<updated>1999-04-22T15:54:59Z</updated>
<published>1999-04-22T15:54:59Z</published>
<title>Improved scenario of baryogenesis</title>
<summary> It is assumed that, in the primordial plasma, at the temperatures above the
mass of electron, fermions are in the neutral state being the superposition of
particle and antiparticle. There exists neutral proton-electron symmetry.
Proton-electron equilibrium is defined by the proton-electron mass difference.
At the temperature equal to the mass of electron, pairs of neutral electrons
annihilate into photons, and pairs of neutral protons and electrons survive as
protons and electrons.
</summary>
<author>
<name>D. L. Khokhlov</name>
</author>
<arxiv:comment xmlns:arxiv="http://arxiv.org/schemas/atom">3 pages LaTeX</arxiv:comment>
<link href="http://arxiv.org/abs/astro-ph/9904306v1" rel="alternate" type="text/html"/>
<link title="pdf" href="http://arxiv.org/pdf/astro-ph/9904306v1" rel="related" type="application/pdf"/>
<arxiv:primary_category xmlns:arxiv="http://arxiv.org/schemas/atom" term="astro-ph" scheme="http://arxiv.org/schemas/atom"/>
<category term="astro-ph" scheme="http://arxiv.org/schemas/atom"/>
</entry>
<entry>
<id>http://arxiv.org/abs/hep-ph/9411242v1</id>
<updated>1994-11-08T11:19:41Z</updated>
<published>1994-11-08T11:19:41Z</published>
<title>Proton-ring and Electron-linac Collider (PRELC) as a (first)
TeV-rangeelectron-proton or photon-proton collider</title>
<summary> The use of the existing proton storage rings combined with electron linear
accelerator as a ring-linac type electron-proton or photon-proton collider is
investigated. The total CM-energy of Proton-ring and Electron-linac Collider
(PRELC) is in the range of 1.0 TeV. The most important physical issues are
listed and the most critical machine aspects of the PRELC are studied. It is
shown that the luminosities in the range of $10^{31}$ to $10^{32}$ could be
achieved. The PRELC could be used simultaneously with the $e^+e^-$-collider if
the refocused electron beam could be used as the electron beam for the PRELC.
</summary>
<author>
<name>Raimo Vuopionperä</name>
<arxiv:affiliation xmlns:arxiv="http://arxiv.org/schemas/atom">SEFT, Univ. Helsinki</arxiv:affiliation>
</author>
<arxiv:comment xmlns:arxiv="http://arxiv.org/schemas/atom">4 pages, revtex</arxiv:comment>
<link href="http://arxiv.org/abs/hep-ph/9411242v1" rel="alternate" type="text/html"/>
<link title="pdf" href="http://arxiv.org/pdf/hep-ph/9411242v1" rel="related" type="application/pdf"/>
<arxiv:primary_category xmlns:arxiv="http://arxiv.org/schemas/atom" term="hep-ph" scheme="http://arxiv.org/schemas/atom"/>
<category term="hep-ph" scheme="http://arxiv.org/schemas/atom"/>
</entry>
<entry>
<id>http://arxiv.org/abs/1706.01836v2</id>
<updated>2017-09-24T14:21:38Z</updated>
<published>2017-06-06T16:12:51Z</published>
<title>Development of a Practical Multicomponent Density Functional for
Electron-Proton Correlation to Produce Accurate Proton Densities</title>
<summary> Multicomponent density functional theory (DFT) enables the consistent quantum
mechanical treatment of both electrons and protons. A major challenge has been
the design of electron-proton correlation functionals that produce even
qualitatively accurate proton densities. Herein an electron-proton correlation
functional, epc17, is derived analogously to the Colle-Salvetti formalism for
electron correlation and is implemented within the nuclear-electronic orbital
(NEO) framework. The NEO-DFT/epc17 method produces accurate proton densities
efficiently and is promising for diverse applications.
</summary>
<author>
<name>Yang Yang</name>
</author>
<author>
<name>Kurt R. Brorsen</name>
</author>
<author>
<name>Tanner Culpitt</name>
</author>
<author>
<name>Michael V. Pak</name>
</author>
<author>
<name>Sharon Hammes-Schiffer</name>
</author>
<arxiv:doi xmlns:arxiv="http://arxiv.org/schemas/atom">10.1063/1.4996038</arxiv:doi>
<link title="doi" href="http://dx.doi.org/10.1063/1.4996038" rel="related"/>
<arxiv:journal_ref xmlns:arxiv="http://arxiv.org/schemas/atom">The Journal of Chemical Physics 147, 114113 (2017)</arxiv:journal_ref>
<link href="http://arxiv.org/abs/1706.01836v2" rel="alternate" type="text/html"/>
<link title="pdf" href="http://arxiv.org/pdf/1706.01836v2" rel="related" type="application/pdf"/>
<arxiv:primary_category xmlns:arxiv="http://arxiv.org/schemas/atom" term="physics.chem-ph" scheme="http://arxiv.org/schemas/atom"/>
<category term="physics.chem-ph" scheme="http://arxiv.org/schemas/atom"/>
</entry>
<entry>
<id>http://arxiv.org/abs/astro-ph/9901367v1</id>
<updated>1999-01-26T16:05:34Z</updated>
<published>1999-01-26T16:05:34Z</published>
<title>Scenario of baryogenesis</title>
<summary> Scenario of baryogenesis is considered in which primordial plasma starting
from the Planck scale consists of primordial particles being the precursors of
electrons and clusters of particles being the precursors of protons.
Equilibrium between the precursors of protons and the precursors of electrons
is defined by the proton-electron mass difference. At the temperature equal to
the mass of electron, primordial particles transit into protons, electrons,
photons.
</summary>
<author>
<name>D. L. Khokhlov</name>
</author>
<arxiv:comment xmlns:arxiv="http://arxiv.org/schemas/atom">2 pages, LaTeX</arxiv:comment>
<link href="http://arxiv.org/abs/astro-ph/9901367v1" rel="alternate" type="text/html"/>
<link title="pdf" href="http://arxiv.org/pdf/astro-ph/9901367v1" rel="related" type="application/pdf"/>
<arxiv:primary_category xmlns:arxiv="http://arxiv.org/schemas/atom" term="astro-ph" scheme="http://arxiv.org/schemas/atom"/>
<category term="astro-ph" scheme="http://arxiv.org/schemas/atom"/>
</entry>
<entry>
<id>http://arxiv.org/abs/1207.3978v1</id>
<updated>2012-07-17T12:58:05Z</updated>
<published>2012-07-17T12:58:05Z</published>
<title>Relativistic Ohm and Fourier laws for binary mixtures of electrons with
protons and photons</title>
<summary> Binary mixtures of electrons with protons and of electrons with photons
subjected to external electromagnetic fields are analyzed by using the Anderson
and Witting model equation. The relativistic laws of Ohm and Fourier are
determined as well as general expressions for the electrical and thermal
conductivities for relativistic ionized gas mixtures. Explicit expressions for
the transport coefficients are given for the particular cases: a
non-relativistic mixture of protons and non-degenerate electrons; an
ultra-relativistic mixture of photons and non-degenerate electrons; a
non-relativistic mixture of protons and completely degenerate electrons; an
ultra-relativistic mixture of photons and completely degenerate electrons and a
mixture of non-relativistic protons and ultra-relativistic completely
degenerate electrons.
</summary>
<author>
<name>Gilberto M. Kremer</name>
</author>
<arxiv:comment xmlns:arxiv="http://arxiv.org/schemas/atom">17 pages</arxiv:comment>
<link href="http://arxiv.org/abs/1207.3978v1" rel="alternate" type="text/html"/>
<link title="pdf" href="http://arxiv.org/pdf/1207.3978v1" rel="related" type="application/pdf"/>
<arxiv:primary_category xmlns:arxiv="http://arxiv.org/schemas/atom" term="cond-mat.stat-mech" scheme="http://arxiv.org/schemas/atom"/>
<category term="cond-mat.stat-mech" scheme="http://arxiv.org/schemas/atom"/>
</entry>
<entry>
<id>http://arxiv.org/abs/0806.3233v1</id>
<updated>2008-06-19T16:39:33Z</updated>
<published>2008-06-19T16:39:33Z</published>
<title>Shuttle-mediated proton pumping across the inner mitochondrial membrane</title>
<summary> Shuttle-assisted charge transfer is pivotal for the efficient energy
transduction from the food-stuff electrons to protons in the respiratory chain
of animal cells and bacteria. The respiratory chain consists of four
metalloprotein Complexes (I-IV) embedded in the inner membrane of a
mitochondrion. Three of these complexes pump protons across the membrane,
fuelled by the energy of food-stuff electrons. Despite extensive biochemical
and biophysical studies, the physical mechanism of this proton pumping is still
not well understood. Here we present a nanoelectromechanical model of the
electron-driven proton pump related to the second loop of the respiratory
chain, where a lipid-soluble ubiquinone molecule shuttles between the Complex I
and Complex III, carrying two electrons and two protons. We show that the
energy of electrons can be converted to the transmembrane proton potential
gradient via the electrostatic interaction between electrons and protons on the
shuttle. We find that the system can operate either as a proton pump, or, in
the reverse regime, as an electron pump. For membranes with various
viscosities, we demonstrate that the uphill proton current peaks near the body
temperature $T \approx 37 ^{\circ}$C.
</summary>
<author>
<name>Anatoly Yu. Smirnov</name>
</author>
<author>
<name>Sergey E. Savel'ev</name>
</author>
<author>
<name>Franco Nori</name>
</author>
<arxiv:comment xmlns:arxiv="http://arxiv.org/schemas/atom">22 pages, 6 figures</arxiv:comment>
<link href="http://arxiv.org/abs/0806.3233v1" rel="alternate" type="text/html"/>
<link title="pdf" href="http://arxiv.org/pdf/0806.3233v1" rel="related" type="application/pdf"/>
<arxiv:primary_category xmlns:arxiv="http://arxiv.org/schemas/atom" term="cond-mat.other" scheme="http://arxiv.org/schemas/atom"/>
<category term="cond-mat.other" scheme="http://arxiv.org/schemas/atom"/>
<category term="physics.bio-ph" scheme="http://arxiv.org/schemas/atom"/>
<category term="q-bio.SC" scheme="http://arxiv.org/schemas/atom"/>
</entry>
<entry>
<id>http://arxiv.org/abs/1602.03411v1</id>
<updated>2016-02-10T15:36:31Z</updated>
<published>2016-02-10T15:36:31Z</published>
<title>Effects of electron temperature anisotropy on proton mirror instability
evolution</title>
<summary> Proton mirror modes are large amplitude nonpropagating structures frequently
observed in the magnetosheath. It has been suggested that electron temperature
anisotropy can enhance the proton mirror instability growth rate while leaving
the proton cyclotron instability largely unaffected, therefore causing the
proton mirror instability to dominate the proton cyclotron instability in
Earth's magnetosheath. Here, we use particle-in-cell simulations to investigate
the electron temperature anisotropy effects on proton mirror instability
evolution. Contrary to the hypothesis, electron temperature anisotropy leads to
excitement of the electron whistler instability. Our results show that the
electron whistler instability grows much faster than the proton mirror
instability and quickly consumes the electron free energy, so that there is no
electron temperature anisotropy left to significantly impact the evolution of
the proton mirror instability.
</summary>
<author>
<name>Narges Ahmadi</name>
</author>
<author>
<name>Kai Germaschewski</name>
</author>
<author>
<name>Joachim Raeder</name>
</author>
<arxiv:doi xmlns:arxiv="http://arxiv.org/schemas/atom">10.1002/2016JA022429</arxiv:doi>
<link title="doi" href="http://dx.doi.org/10.1002/2016JA022429" rel="related"/>
<arxiv:comment xmlns:arxiv="http://arxiv.org/schemas/atom">11 pages, 19 figures</arxiv:comment>
<link href="http://arxiv.org/abs/1602.03411v1" rel="alternate" type="text/html"/>
<link title="pdf" href="http://arxiv.org/pdf/1602.03411v1" rel="related" type="application/pdf"/>
<arxiv:primary_category xmlns:arxiv="http://arxiv.org/schemas/atom" term="physics.plasm-ph" scheme="http://arxiv.org/schemas/atom"/>
<category term="physics.plasm-ph" scheme="http://arxiv.org/schemas/atom"/>
<category term="physics.space-ph" scheme="http://arxiv.org/schemas/atom"/>
</entry>
<entry>
<id>http://arxiv.org/abs/2507.06488v1</id>
<updated>2025-07-09T02:18:06Z</updated>
<published>2025-07-09T02:18:06Z</published>
<title>High Proton Conductivity of HxWO3 at Intermediate Temperatures:
Unlocking Its Application as a Mixed Ionic-Electronic Conductor</title>
<summary> Hydrogen tungsten bronzes (HxWO3), known for their mixed protonic-electronic
conduction near room temperature, are extensively studied for electrochromic
and gasochromic applications. However, their proton transport properties at
elevated temperatures, particularly in the intermediate-temperature range
(200-500 {\deg}C), remain unexplored. This study revealed the proton transport
behavior of HxWO3, focusing on its potential as a proton-conducting mixed
ionic-electronic conductor (MIEC) for intermediate-temperature electrochemical
applications. By employing a proton-conducting phosphate glass as an
electron-blocking electrode, we selectively measured the partial proton
conductivity of sintered HxWO3. Hydrogen incorporation into the sintered WO3
pellet was found to occur preferentially near the surface, forming an
approximately 500-micrometer-thick hydrogen-rich region. This region reached a
composition of x = 0.24 and exhibited proton conductivity exceeding 10^-1 S/cm
at 275 {\deg}C, well above those of state-of-the-art perovskite proton
conductors. Impedance spectroscopy revealed distinct features of proton
transport, including an isotope effect. The proton diffusion coefficient was
100-1000 times greater than that of H0.0001TiO2, which exhibits mixed
protonic-electronic conduction via hydrogen dissolution. The larger proton
diffusion coefficient of H0.24WO3 suggests that large polaron formation
enhances proton mobility.These findings unlock new functionality of HxWO3 as a
MIEC in the intermediate-temperature range, paving the way for the development
of next-generation hydrogen energy conversion systems.
</summary>
<author>
<name>Rantaro Matsuo</name>
</author>
<author>
<name>Tomoyuki Yamasaki</name>
</author>
<author>
<name>Takahisa Omata</name>
</author>
<link href="http://arxiv.org/abs/2507.06488v1" rel="alternate" type="text/html"/>
<link title="pdf" href="http://arxiv.org/pdf/2507.06488v1" rel="related" type="application/pdf"/>
<arxiv:primary_category xmlns:arxiv="http://arxiv.org/schemas/atom" term="cond-mat.mtrl-sci" scheme="http://arxiv.org/schemas/atom"/>
<category term="cond-mat.mtrl-sci" scheme="http://arxiv.org/schemas/atom"/>
<category term="cond-mat.dis-nn" scheme="http://arxiv.org/schemas/atom"/>
</entry>
<entry>
<id>http://arxiv.org/abs/1403.6944v1</id>
<updated>2014-03-27T08:10:23Z</updated>
<published>2014-03-27T08:10:23Z</published>
<title>Particle production from the Color Glass Condensate: proton-nucleus
collisions in light of the HERA data</title>
<summary> We compute single inclusive hadron production in proton-proton and
proton-nucleus collisions consistently within the CGC framework. The parameters
in the calculations are obtained from electron-proton DIS and standard nuclear
geometry. We obtain a good description of the DIS data without an anomalous
dimension in the initial condition of the BK evolution and get a good agreement
with the available single inclusive proton-proton and proton-nucleus data.
</summary>
<author>
<name>T. Lappi</name>
</author>
<author>
<name>H. Mäntysaari</name>
</author>
<arxiv:doi xmlns:arxiv="http://arxiv.org/schemas/atom">10.1016/j.nuclphysa.2014.08.038</arxiv:doi>
<link title="doi" href="http://dx.doi.org/10.1016/j.nuclphysa.2014.08.038" rel="related"/>
<arxiv:comment xmlns:arxiv="http://arxiv.org/schemas/atom">4 pages, 4 figures, talk given at the 6th International Conference on
Hard and Electromagnetic Probes of High-Energy Nuclear Collisions (Hard
Probes 2013), November 4-8, 2013 (Cape Town, South Africa)</arxiv:comment>
<link href="http://arxiv.org/abs/1403.6944v1" rel="alternate" type="text/html"/>
<link title="pdf" href="http://arxiv.org/pdf/1403.6944v1" rel="related" type="application/pdf"/>
<arxiv:primary_category xmlns:arxiv="http://arxiv.org/schemas/atom" term="hep-ph" scheme="http://arxiv.org/schemas/atom"/>
<category term="hep-ph" scheme="http://arxiv.org/schemas/atom"/>
<category term="nucl-th" scheme="http://arxiv.org/schemas/atom"/>
</entry>
<entry>
<id>http://arxiv.org/abs/2407.11707v1</id>
<updated>2024-07-16T13:25:36Z</updated>
<published>2024-07-16T13:25:36Z</published>
<title>The neutron skin-thickness of 208 Pb determined by electron and proton
scattering</title>
<summary> The consistency between electron-scattering and proton-scattering is examined
through the fourth moment of the charge distribution.
</summary>
<author>
<name>Toshio Suzuki</name>
</author>
<author>
<name>Rika Danjo</name>
</author>
<author>
<name>Toshimi Suda</name>
</author>
<link href="http://arxiv.org/abs/2407.11707v1" rel="alternate" type="text/html"/>
<link title="pdf" href="http://arxiv.org/pdf/2407.11707v1" rel="related" type="application/pdf"/>
<arxiv:primary_category xmlns:arxiv="http://arxiv.org/schemas/atom" term="nucl-th" scheme="http://arxiv.org/schemas/atom"/>
<category term="nucl-th" scheme="http://arxiv.org/schemas/atom"/>
</entry>
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