
2
ically, with 83.2% of atoms in the 1s-state and 10.4% in the
2s-state and the remainder in an ns-state where n≥3[10].
In this study, we propose a scheme to detect the BoB that
will rely on the measurement of H atoms through its energy
spectrum structure, in order to observe for the first time this
hitherto unobserved decay mode. As known, the standard
three-body decay mode is n→H++e−+ ¯νe, where the
proton and electron are charged particles that are easily cap-
tured by solid materials, while the antineutrino is extremely
difficult to capture. The total energy in the three-body decay
is conserved, leading to continuum energy spectra for each of
particles. Since the mass of the proton is much larger than
that of the electron and neutrino, the decay energy is obtained
mainly by the electron and neutrino, both of which have ki-
netic energies in the range of 0–782 keV, while the energy
spectrum of the proton lies in the range of 0–750 eV [11].
For the BoB mode, the conservation of momentum and
energy during the decay leads to the energy carried by the
antineutrino is constant, while the kinetic energy of the hy-
drogen atom is also constant (325.7 eV), making it easy to
be captured by solid materials. Since the hydrogen atom in
the ns (≥2) state after the two-body decay can be captured
by the detector, it will de-excite to the 1s state very quickly,
transferring its thermal energy greater than 10.2 eV to the
detector. Thus, the kinetic energy spectra of the hydrogen
atoms on the detector would be a multiple line structure dom-
inated by 325.7 eV and 335.9 eV. The lower right panel of
Fig. 2shows only these two spectral lines, and the other spec-
tral lines from ns states are ignored for the moment. More-
over, three-body-decay protons will introduce a strong back-
ground continuum spectrum contaminating the measurement
of the hydrogen atoms, which needs to be removed to obtain
a high signal-to-noise ratio. Since the charged protons and
electrons are susceptible to an external electric field, one can
set up positive and negative electrodes at about 1 kV in a low-
temperature vacuum, resulting in a large difference in signal
amplitudes between electrons with E > 1keV and hydrogen
atoms at 325.7 eV, which therefore can be easily identified.
In Fig. 3, the expected shapes of energy spectrum before and
after electric field screening is shown. As seen, combine with
the 1kV screening electric field, the central energy of the elec-
trons is in the energy region of several hundred keV, which is
very different from the line signature of the two-body-decay
hydrogen atoms.
A microcalorimeter is a sensitive detector for heat signals,
with extremely high energy resolution at eV level and no dead
layer, as well as a wide range of available absorption materi-
als [12,13]. The energy of the particle deposition is converted
into heat and the resulting temperature rise is measured. Since
hydrogen atoms, electrons and protons can all generate heat
signals at the detector, and the energy resolution at the eV
level fully satisfies the requirement for resolution of a single
energy peak at 325.7 eV, the microcalorimeter detector is thus
an ideal detector for measuring the BoB according to energy
spectrometry. Although electrons and protons below 1 keV
can be completely eliminated by the electric field, there are
still some background processes that would produce a con-
tinuum at the detector. As seen from the lower right panel of
Fig. 2, if the initial kinetic energy of neutrons is much less
than 1 eV and the resolution of the detector is around 1 eV,
not only can the hydrogen atom be clearly seen in the 1s or 2s
or even a higher state, but also a high signal-to-background
can be obtained. For the transition edge sensor (TES)-based
microcalorimeter, in the 1 keV energy range, the best reported
energy resolution is about 0.75 eV [14], and the best one we
obtained so far is about 1.4 eV [15], so that the detector per-
formance is basically appropriate for the BoB measurement.
More importantly, as the energy range of interest is around
325.7 eV, a better energy resolution can be obtained by fur-
ther reducing the heat capacity of the microcalorimeter [13].
This paper is organized as follows. In Sect. II, we will
present the theoretical calculations for the BoB and summa-
rize various neutron sources, then discuss the the require-
ments for the BoB measurements, in addition we briefly re-
view the working principle of microcalorimeter. In Sect. III,
we outline our experimental concept and investigate suitable
neutron sources, as well as discuss measurement related is-
sues, such as the 3He problem in refrigerators, the elimination
of proton effects, effects of high-energy particles, the method
of readout electronics, etc. Finally, we draw our summary and
conclusions in Sect. IV.
II. BASIC PRINCIPLES
A. Theoretical Calculations of Neutron Two-Body Decay
Let us consider the BoB process, n→H + ¯νe, where the
expression for the kinetic energy of the hydrogen atom can
be derived from the conservation of energy and momentum.
In the following, the subscripts of n, H, ¯νerepresent neu-
tron, hydrogen atom and electron antineutrino, respectively.
E,Pand Mdenote the energy, the momentum and the rest
mass, respectively. We will use natural units in which c= 1
throughout. First, the conservation of energy leads to
En=EH+E¯νe,(1)
According to the energy–momentum relation and the momen-
tum conservation, PH+P¯νe= 0, Eq. 1is then expressed by
Mn=qM2
H+P2
H+qM2
¯νe+P2
¯νe,(2)
which yields
Mn−qM2
H+P2
H2
=M2
¯νe+P2
H,(3)
and by expanding it, one obtain
M2
n+M2
H−M2
¯νe
2Mn
=qM2
H+P2
H(4)
In the non-relativistic limit for H,
qM2
H+P2
H≈MH+TH,with TH=P2
H
2MH
(5)