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1 ne glass (with a barrier to tunneling of 1.4 electron volts).
2 and-gap energy than rutile (2.32 versus 3.00 electron volts).
3 and lowest unoccupied orbitals of 0.4 to 0.9 electron volt.
4 t with a spin gap of approximately one milli-electron volt.
5  measured apparent activation energy of 0.16 electron volt.
6 n is most pronounced at approximately 1 kilo-electron volt.
7 with adsorption energies between 0.2 and 3.5 electron volts.
8 tor with an indirect bandgap of 1.36 to 1.41 electron volts.
9  30 nanometers and waveguide modes above 1.9 electron volts.
10 ayer-tunable band offset shift exceeding 0.5 electron volts.
11 e also changes by 90 degrees at ~4 to 5 kilo-electron volts.
12  and rises to 35.2 +/- 7.1% at 5.5 to 8 kilo-electron volts.
13 l calculated bandgap reduction as much as ~2 electron volts.
14 n a large-scale bandgap narrowing up to ~2.2 electron volts.
15  a full width at half maximum of 0.625 milli-electron volts.
16 f the spectrum, up to photon energies of 280 electron volts.
17 unction of Ag, Cu, and Au electrodes to 3.65 electron volts.
18 c-ray electron intensity down to ~10 x 10(6) electron volts.
19  relatively narrow absorber band gap of 1.55 electron volts.
20 ate cosmic rays to energies close to ~10(15) electron volts.
21 tween 2 x 10(8) electron volts and 3 x10(11) electron volts.
22 d is observed at energies from 0.2 to 6 kilo-electron volts.
23  small optical gap edge of approximately 2.2 electron volts.
24 ale reconnection-driven flows are just a few electron volts.
25 ted to very high energies of several million electron volts.
26 metal with a band width of approximately 0.5 electron volts.
27 ron volts) and an optical energy gap of 0.34 electron volts.
28  emitted via synchrotron radiation from peta-electron-volt (10(15) electron volts) electrons in a reg
29 ssion electron microscope, we detected a 5.7-electron volt (2175 angstrom) feature in interstellar gr
30  a CH3OH overlayer state that is 2.3 +/- 0.2 electron volts above the Fermi level.
31  we found an unoccupied electronic state 2.4 electron volts above the Fermi level.
32 s essentially spin-independent already a few electron-Volts above the vacuum level.
33 m rods with distinct energy gaps (0.6 to 1.3 electron volts), all sharing the same radial dimension b
34 m from the ultraviolet to more than 1.6 kilo-electron volts, allowing, in principle, the generation o
35 Area Telescope at energies between 2 x 10(8) electron volts and 3 x10(11) electron volts.
36 spectrum of pulsed emission between 100 mega-electron volts and 400 GeV is described by a broken powe
37 a magnitude of approximately 10 to 100 milli-electron volts and a nanotube radius (r) dependence of a
38 erate particles to energies exceeding 10(12) electron volts and are bright sources of very-high-energ
39 emiconductor with a discrete band gap of 1.9 electron volts and can be chemically oxidized to enhance
40 vated conductivity (activation energy, 0.054 electron volts) and an optical energy gap of 0.34 electr
41 have narrow energy gaps (between 0.2 and 2.0 electron volts) and low densities, and they may be usefu
42 ow the instrumental sensitivity ~4 to 5 kilo-electron volts, and rises to 35.2 +/- 7.1% at 5.5 to 8 k
43 oximately 100 kilocalories per mole (about 4 electron volts) are reported for polyatomic molecules, i
44 band energy separation of approximately 0.25 electron volts, are capped by an epitaxial zinc selenide
45  bandgap energy red shift of 13 (+/-7) milli-electron volts as mass of Mo isotopes is increased in la
46 sured an even narrower linewidth of 410 pico-electron volts at 77 kelvin.
47 termine the plasma frequency of 32.5 +/- 2.1 electron volts at a temperature of 5.5 kelvin, with a co
48          A large conduction band offset (3.4 electron volts) at the Ga(2)O(3)/AlN interface improves
49  6 lines at 320, 400, 490, 560, 600, and 670 electron volts, attributable to electron capture and rad
50         We develop an infrared-absorbing 1.2-electron volt band-gap perovskite, FA0.75Cs0.25Sn0.5Pb0.
51 13.5 +/- 0.8% averaged over the 2- to 8-kilo-electron volt band.
52 solar photovoltaics that require a fully 2.0-electron-volt bandgap absorber(2,6).
53 in an energy splitting of more than 10 milli-electron volts between the K and K' valley exciton trans
54 ed to a difference of approximately 60 milli-electron volts between zero-point energies of incident p
55 ses of new physics above [Formula: see text] electron volts, beyond the direct reach of the current p
56 hod to prepare highly textured columnar 1.75-electron volt Br-I mixed WBG perovskite films with reduc
57 tier of particle physics is several trillion electron volts, but colliders capable of reaching this r
58  downward to obtain energies of several kilo electron volts by a quasi-static electric field.
59 nty; syst, systematic uncertainty; MeV, mega-electron volts; c, speed of light in a vacuum).
60  proton-antiproton collisions at a 1.96 tera-electron volt center-of-mass energy with the CDF II dete
61 tz range with photon energies of a few milli-electron volts, classical mechanisms are used instead.
62 produced hot electrons with energies of mega-electron volts, cold ions in the inner wall surface impl
63 ) + D reaction at a collision energy of 1.97 electron volts contradict this behavior.
64  As concentration rises, a narrow peak at ~2 electron volts, corresponding to vertical photodetachmen
65 ve and reveal a confinement gap of up to 0.5 electron volt, demonstrating the possibility of molecula
66                           The resulting 1.53-electron-volt devices achieved 25.6% certified power con
67 h ultrasharp peaks (widths of 12 to 25 milli-electron volts) devoid of the characteristic background
68  (Fig. 2C) as a function of maximum work (in electron volts) done by electron (laser photon) E(alpha)
69 : The degree is 15.0 +/- 1.0% at 2 to 4 kilo-electron volts, drops below the instrumental sensitivity
70 ighlights the opportunities provided by Mega-electron-volt electron and X-ray free electron laser to
71 on radiation from peta-electron-volt (10(15) electron volts) electrons in a region smaller than 1.4 x
72 87A) have resolved the 67.87- and 78.32-kilo-electron volt emission lines from decay of (44)Ti produc
73 f accelerated leptons, but the measured tera-electron volt emission profile constrains the diffusion
74 sion is similar to that of lower-energy giga-electron volt emission, indicating a common origin, with
75  clusters coherently interconvert over an ~1-electron volt energy barrier with a 140-milli-electron v
76 ent nonlinear optical spectroscopy with nano-electron volt energy resolution and low-temperature near
77 ayer trions with binding energy in the milli-electron volt energy scale at temperatures two orders of
78 nce with mainly ultra-relativistic (> 2 mega-electron-volts) energy electrons.
79 te-mediated attraction of approximately 0.12 electron volt (eV).
80 um perovskite cell optical band gap of ~1.75 electron volts (eV) can be achieved by varying halide co
81    This average temperature dependence (0.96 electron volts (eV)), which corresponds to a 57-fold inc
82 mma-ray (photon energy greater than 100 mega-electron volts) flares from this source detected by the
83 racted degradation activation energy of 0.61 electron volts for solar modules is comparable to that o
84 x-ray quantum interferometry using 17.5-kilo-electron volt ( [Formula: see text] = 70 picometers) pho
85 riable gamma-ray emission (0.1 to 10 billion electron volts) from the recently detected optical nova
86 erenkov Observatory (HAWC), of extended tera-electron volt gamma-ray emission coincident with the loc
87 m the Crab pulsar at energies above 100 giga-electron volts (GeV) with the Very Energetic Radiation I
88 ps reveal distinct nonthermal (0.2 to 6 kilo-electron volts) heliosheath proton populations with spec
89 h potential energy barriers that are several electron-volts high and several nanometers wide.
90 bited semiconducting behavior (bandgap ~1.94 electron volts), high strength (~66 gigapascals), and ex
91 B) states, with subband gaps (~0.78 and 1.26 electron volts) ideal for next-generation solar devices,
92   An isotopic red shift of 4.8 +/- 0.4 milli-electron volts in C-O asymmetric stretching modes was ob
93  graphite, it is found that changes of milli-electron volts in the energy range of up to 50 electron
94 stant is 1.62 per angstrom (the barrier, 2.6 electron volts) in a frozen 2-methyl-tetrahydrofuran gla
95 (and a broad resonance centered at +20 milli-electron volts) in spectroscopic measurements, indicatin
96 a broad absorption peak emerges at ~18 milli-electron volts, indicating direct optical excitation acr
97 ity(3-5): this occurs in wide-bandgap (>1.65 electron volts) iodide/bromide mixed perovskite absorber
98 electrons with energies greater than 30 kilo-electron volts (keV) shortly after its insertion into or
99 expected x-ray emission line around 3.5 kilo-electron volts (keV).
100 e a gas-phase ionization energy (onset, 3.51 electron volts) lower than that of the cesium atom (whic
101 pa in conjunction with its wide bandgap (6.2 electron volts) makes cBN a promising material for micro
102  a narrow emission feature at about 2.1 mega-electron volts (MeV) in the spectrum of GRB 221023A.
103 >6sigma) narrow emission feature at ~10 mega-electron volts (MeV) in the spectrum of the bright GRB 2
104               A preliminary design of a mega-electron-volt (MeV) monochromator with 10(-5) energy spr
105 he cesium ratio of a methylammonium-free 1.8-electron volt mixed-halide perovskite, we improve the ho
106            When further integrated with 1.25-electron volt narrow-bandgap PSC, we obtained a 27.1% ef
107 -H bond formation, where H atoms lose 1 to 2 electron volts of energy within a 10-femtosecond interac
108 onths (radon exposure averaging 130,000 mega-electron volts of potential alpha energy per liter of ai
109 tion due to large binding energy (E(B) ~ 0.5 electron volts) of Frenkel excitons, particularly in nar
110         Hydronium ions were soft-landed at 1 electron volt on cold films of 3-methylpentane ("oil") o
111 urface plasmon polariton between 1.4 and 1.9 electron volts on MXene flakes thicker than 30 nanometer
112 ay spectroscopy near the carbon K-edge ( 284 electron volts) on a tabletop apparatus to directly reve
113 ges that extend up to an energy of about 0.3 electron volt, or 40kTc (where k is the Boltzmann consta
114 we infer a maximum energy gain of 0.915 kilo-electron volts over 30 micrometers, corresponding to an
115  of all other competing phases by >=60 milli-electron volt per atom.
116 states at the Fermi level of 15.5 states per electron volt per mole.
117 th unusually low counting rates of >0.5 mega-electron volt per nuclear particle.
118 ing to an acceleration gradient of 30.5 mega-electron volts per meter.
119 th broad peaks from 10 x 10(6) to 40 x 10(6) electron volts per nucleon and an increasing galactic co
120 iron nuclei, with energies ~195 to ~500 mega-electron volts per nucleon, of which we identify 15 (60)
121 a of galactic cosmic rays down to ~3 x 10(6) electron volts per nucleon, revealing H and He energy sp
122 operties of Sn-Pb mixed, low-band gap (~1.25 electron volt) perovskite films.
123  coincides with the hardening of a sub-milli-electron volt phonon mode related to the antiferrodistor
124 ge of energetic neutral atoms (ENAs) >6 kilo-electron volts produced by energetic protons occupying t
125  population comprises accelerated ions (<800 electron volts), produced upstream of Rosetta, and lower
126     Its steepening above approximately 10(9) electron volts provides a probe with which to study how
127 endent of excitation photon energy over a ~1-electron volt range, and dependent on the excitation pol
128  perovskite absorber, with a bandgap of 1.68 electron volts, remained phase-stable under illumination
129 ectron volts in the energy range of up to 50 electron volts reveal the compression and expansion of l
130                   Using an approximately 2.0-electron-volt rubidium/caesium mixed-cation inorganic pe
131 possibility for a completely integrated mega-electron volt-scale DLA.
132 current arises from the existence of a ~0.95-electron volt Schottky barrier at the Te-electrode inter
133 cluded HPLC-MS, Raman spectroscopy, and mega-electron volt-secondary ionization mass spectrometry.
134 The short-wavelength driver results in a 6.2-electron volt separation between harmonics, markedly red
135 lectron volt energy barrier with a 140-milli-electron volt shift in their excitonic energy gaps.
136     Some gamma-ray bursts (GRBs) have a tera-electron volt (TeV) afterglow, but the early onset of th
137 interstellar modulation of high-energy (tera-electron volts, TeV) cosmic rays and diffusive propagati
138 perovskite solar cell with a bandgap of ~1.7 electron volts that retained more than 80% of its initia
139 ndence of the desorption yield peaks at 0.26 electron volt: the energy of the Si-H vibrational stretc
140 etic particles were observed up to 200 kilo--electron volts; these particles are capable of penetrati
141 n energy distribution width of less than 0.5 electron volts, this source of monochromatic electrons m
142        Between energies of 0.18 and 3.3 tera-electron volts, this spectrum is described by a power la
143 ral atoms (ENAs) at energies between tens of electron volts to hundreds of kiloelectron volts (keV).
144 s by forming an interface with J ~ 100 milli-electron volts transferred between a Eu triangular latti
145 al-pointing jitter information into the mega-electron-volt ultrafast electron diffraction pattern.
146  observing the atomic arrangement using mega-electron-volt ultrafast electron diffraction studies, we
147 ing the enhanced temporal resolution of mega-electron-volt ultrafast electron diffraction with a supe
148 eleration of electrons from hundreds of kilo-electron volts up to >7 MeV.
149 idence for neutron emission near 2.5 million electron volts was also observed, as would be expected f
150  laser excitation (at a photon energy of 1.5 electron volts) was used to introduce a spatially period
151         With this approach, we obtained 1.75-electron volt WBG PSCs with greater than 20% power conve
152 tals of the carbon-atom framework, above 3.5 electron volts we found atomlike orbitals bound to the c
153 surface with electrons with an energy of 300 electron volts were analyzed by scanning tunneling micro
154 tron energies reach hundreds of thousands of electron volts, whereas the typical electron energies as
155 ission extending to high energies (>10 kilo--electron volts), which is ascribed to an accretion disk
156  solar cells of bandgaps between 1.6 and 1.8 electron volts, which is crucial for tandem applications
157  mass-splitting with an accuracy of 300 kilo-electron volts, which is greater than 0 by 5 standard de
158 A1g transition state is 1.099 ± 0.010 electron volts, which is lower by 12.1 ± 0.3 kilo
159  with a bandwidth of approximately 200 milli-electron volts, which is reminiscent of the spin wave of
160                     We report efficient 1.67-electron volt wide-band gap perovskite top cells using t
161 he Rabi splitting between ~108 and 102 milli-electron volts with a bias of only 2.5 volts.
162 f conventional spin resonance (here ~10 nano-electron volts) with scanning tunneling microscopy to me

 
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