
Nitrogen-vacancy singlet manifold ionization energy
S. A. Wolf,1, 2 I. Meirzada,1G. Haim,3and N. Bar-Gill1, 2, 3
1The Racah Institute of Physics, The Hebrew University of Jerusalem, Jerusalem 91904, Israel
2The Center for Nanoscience and Nanotechnology,
The Hebrew University of Jerusalem, Jerusalem 91904, Israel
3Dept. of Applied Physics, Rachel and Selim School of Engineering, Hebrew University, Jerusalem 91904, Israel
The singlet states of the negatively-charged nitrogen-vacancy centers in diamond play a key role
in its optical spin control and readout. In this work, the hitherto unknown ionization energy of
the singlet is measured experimentally and found to be between 1.91-2.25 eV. This is obtained by
analyzing photoluminescence measurements incorporating spin control and NV charge state dif-
ferentiation, along with simulations based on the nitrogen-vacancy’s master equation. This work
establishes a protocol for a more accurate estimate of this ionization energy, which can possibly lead
to improved read-out methods.
INTRODUCTION
Negatively charged Nitrogen vacancy (NV−) centers
are point defects in diamond which show promising quan-
tum properties essential for various applications ranging
from magnetic sensing to quantum computing. These
applications rely on the NV center’s exceptionally long
coherence times and optical spin readout, even at room
temperature. The properties of the NV center are con-
stantly being studied to improve its coherence time and
readout signal-to-noise ratio (SNR). While most of the
energy levels and transition rates have been measured,
some are still unknown and may have a significant im-
pact on our understanding of the system’s dynamics.
The NV center is a defect in diamond where two adja-
cent carbons are replaced by one nitrogen and a vacancy.
The negatively charged NV has an additional electron
which leads to two holes in the valence shell and an effec-
tive two-electron system. The ground state of the NV−
is a spin one triplet with a 2.87 GHz zero-field-splitting
between spin projections ms= 0 and ms=±1, and can
be controlled using a resonant microwave (MW) drive.
These spin states are located 2.6 eV below the conduction
band (Fig. 1). The electronically excited triplet state is
located 1.945 eV above the ground state with a lifetime
of ∼13 ns [1, 2]. The radiative transition between the
two triplet states is dominated by the phonon side band
(PSB), with ∼650-800 nm emission. The NV−has an
additional singlet (spin zero) manifold consisting of two
energy levels that are separated by 1.19 eV with an ex-
cited state lifetime of ∼0.1 ns [3–6]. Spin selective inter-
system crossing (ISC) allows the excited triplet to decay
non radiatively to the singlet excited state predominantly
from the ms=±1 spin projection. The ground singlet
state, commonly referred to as a metastable state due
to its long lifetime, ∼300 ns, decays back to the ground
triplet state. Theoretical studies have predicted different
values for the energy of the singlet state [7–16]. How-
ever, the energy gap between the singlet manifold and the
conduction band has yet to be measured experimentally,
and is the focus of this work. The NV−can also be ion-
ized optically, and convert to a neutral NV (NV0) center
which has an energy gap of 2.16 eV between it’s ground
and excited states.
FIG. 1. Known energy levels of NV centers.
The most commonly used readout method at room
temperature is based on collecting photoluminescence
(PL) from the PSB while exciting the triplet transition
using the PSB (typically at 532 nm) [17]. Due to the
spin selective ISC, the number of photons emitted de-
pends on the initial spin projection of the ground triplet
state. However, this readout method yields very poor
SNR and requires thousands of repetitions [17]. Different
readout methods have been proposed in order to increase
the readout SNR [17, 18], but those readout methods all
rely on the spin-dependent transition to the metastable
singlet state. Better knowledge of the energy levels and
transition rates, and specifically the unknown singlet en-
ergy, will allow more accurate modeling of the NV dy-
namics and may lead to the development of improved
readout methods. Theoretical studies have predicted var-
arXiv:2210.04171v1 [quant-ph] 9 Oct 2022