Nanophotonics for pair production
Article
https://doi.org/10.1038/s41467-023-43701-5
Nanophotonics for pair production
Received: 21 August 2023
Valerio Di Giulio
1
& F. Javier García de Abajo
1,2
Accepted: 9 November 2023
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The transformation of electromagnetic energy into matter represents a fascinating prediction of relativistic quantum electrodynamics that is paradigmatically exemplified by the creation of electron-positron pairs out of light.
However, this phenomenon has a very low probability, so positron sources rely
instead on beta decay, which demands elaborate monochromatization and
trapping schemes to achieve high-quality beams. Here, we propose to use
intense, strongly confined optical near fields supported by a nanostructured
material in combination with high-energy photons to create electron-positron
pairs. Specifically, we show that the interaction between near-threshold γ-rays
and polaritons yields higher pair-production cross sections, largely exceeding
those associated with free-space photons. Our work opens an unexplored
avenue toward generating tunable pulsed positrons from nanoscale regions at
the intersection between particle physics and nanophotonics.
The creation of massive particles from electromagnetic energy
emerged as a prominent focus of attention in 1934, when the materialization of an electron and its antiparticle—the positron—was predicted
to occur with nonvanishing probability by Breit and Wheeler (BW) from
the scattering of two photons1, by Bethe and Heitler (BH) from the
interaction of a photon and the Coulomb potential of a nucleus2, and by
Landau and Lifshitz (LL) from the collision of two other massive
particles3. A main difference between these processes relates to the real
or virtual nature of the involved photons. While only real electromagnetic quanta lying inside the light cone (i.e., satisfying the light
dispersion relation in vacuum, k = ω/c) participate in the BW mechanism
for pair production, the LL process is mediated by two virtual photons,
and both real and virtual photons play a role in BH scattering. Eventually, pair production was achieved by colliding energetic electrons
and real photons delivered by high-power lasers4, and more recently
using only real photons generated from atomic collisions5.
Besides the fundamental interest of these processes, the generation of positrons finds application in surface science6 through, for
example, positron annihilation spectroscopy7–9 and low-energy positron diffraction10, as well as in the study of their interactions with
atoms and molecules11,12. Positrons are also used to create antimatter,
for example, antihydrogen13–16 and positronium17. In these studies, slow
positrons are commonly obtained from beta decay, decelerated
through metallic moderators18, and subsequently stored in different
types of traps, from which they are extracted as low-energy, quasimonochromatic pulses19–22.
Direct positron generation from light would not require nuclear
decay and could further leverage recent advances in optics to produce ultrashort photon pulses. However, the cross-sections associated with the aforementioned processes are extremely small. As a
possible avenue to increase the pair-production rate, we consider the
replacement of free photons by confined optical modes in the hope
that they alleviate the kinematic mismatch between the particles
involved in BW scattering. In particular, surface polaritons, which are
hybrids of light and polarization charges bound to material interfaces, can display short in-plane wavelengths compared with the freespace light wavelength. Such modes involve electromagnetic energy
trapped at the interface between two media with different dielectric
properties. For example, for a planar interface, when the sign of the
real part of the permittivity of the two media is opposite, the associated optical fields decay exponentially away from the interface, but
a similar behavior is observed when light is trapped by a thin metallic
film23. Likewise, light can be trapped in polaritons sustained by more
involved geometries24 (e.g., in a self-standing sphere, a polariton is
defined by the condition that its permittivity is equal to −2 if one
neglects retardation effects). Actually, a broad suite of twodimensional (2D) materials has recently been identified to sustain
including
long-lived,
strongly
confined
polaritons25,26,
23,27,28
29,30
, phononic
, and excitonic31 modes that cover a
plasmonic
wide spectral range extending from mid-infrared frequencies23,27,29,30
to the visible domain28,31. Specifically, modes bound to nanogaps32
feature large field confinement and enhancement (in vacuum
1
ICFO-Institut de Ciencies Fotoniques, The Barcelona Institute of Science and Technology, 08860 Castelldefels, Barcelona, Spain. 2ICREA-Institució Catalana
e-mail:
de Recerca i Estudis Avançats, Passeig Lluís Companys 23, 08010 Barcelona, Spain.
Nature Communications | (2023)14:8189
1
Article
https://doi.org/10.1038/s41467-023-43701-5
regions) that boost light-mediated processes, such as surfaceenhanced Raman scattering (SERS).
In this work, we calculate the pair-production cross section
associated with the annihilation of γ-ray photons (γ-photons) and
confined polaritons, leading to a substantial enhancement compared
to free-space BW scattering. Part of this enhancement relates to the
spatial confinement of surface polaritons, as the lack of translational
invariance enables pair production for γ-photon energies just above
the 2mec2 threshold (e.g., at the 60Co emission line ℏωγ ~1.17 MeV
combined with a polariton energy ℏωp of a few eV), in contrast to freespace BW scattering, for which visible-range photons need to be paired
with GeV photons such as those generated in astrophysical
processes33,34. The latter include absorption of high-energy γ rays by
extra-galactic background light35, by active galactic nuclei36, and during γ-ray bursts37, as well as plasma production in neutron-star
magnetospheres38. For polaritonic nanogap modes confined in three
dimensions, pairs can be produced by γ-photon scattering in the gap
vacuum region, where polariton-mediated positron emission is not
affected by the background of other emission processes such as BH
scattering. By demonstrating the advantages of using deeply confined
light, our work inaugurates an avenue in the exploration of nanophotonic structures as a platform for high-energy physics.
Results
Pair production from the scattering of a polariton and a γphoton
Considering the general configuration illustrated in Fig. 1a, we study pair
production by using the relativistic minimal coupling Hamiltonian39,40
^ int ðtÞ = 1
H
c
Z
3
d r ^jðrÞ Aðr, tÞ,
ð1Þ
!^
: is the fermionic current, A(r, t) is the
where ^jðrÞ = ec : ΨðrÞ γ ΨðrÞ
classical vector potential associated with the polariton and photon
fields, and we adopt a gauge with vanishing scalar potential. Here,
: ⋅ : denotes normal product concerning electron and posit (...truncated)