AC Recombination Velocity in the Back Surface of a Lamella Silicon Solar Cell under Temperature

The ac recombination velocity of the excess minority carriers, in the back surface of a silicon solar cell with a vertical junction connected in series, is developed through Einstein’s law giving the diffusion coefficient of minority carriers according to temperature, through mobility. The frequency spectrum of both, amplitude and phase, are produced for the diffusion coefficient and the recombination velocity in the rear face, in order to identify the parameters of equivalent electric models.

Two types of VMJ solar cells are developed, by a succession of npp or pnn junctions. The VMJ-P has connections in parallel, between bases and connections between emitters. Thus a base type (p) is surrounded by two emitters allowing the collection of minority carriers at close range, leading to the increase Journal of Modern Physics of photocurrent [6] [7] [8]. The VMJ-S, presents a succession of npp+ or pnn+ solar cells, connected in series, allowing increasing the electrical voltage [9].
The VMJ is designed to operate under light concentration to generate more minority carriers, thereby increasing voltage or current production. In this situation, temperature is an important factor that influences the operating performance of the solar cell, through the physical mechanisms that are important to study [10]. In this work, the ac recombination velocity in the rear face (p/p+) of the solar cell, is determined and studied in temperature using the frequency spectrum of its amplitude and phase.

Theory
The structure of the serially connected vertical multi-junctions silicon solar cell, under monochromatic illumination in frequency modulation, is given by Figure   1 [11].
The unit of the solar cell extracted from the series representation, is a npp+ structure, the base of which is studied by variation in the temperature T ( Figure   2 , , ,  , , , ,  , , , ,  , , ,  The density of photogenerated carriers is written according to the space coordinates (x, z) and the time t as: The minority carriers generation rate at depth z in the base and at any point of absciss x, under the modulation frequency ω of the incident wave, is given by the relationship: where g(z) is the steady stateminority carriers generation rate at the z depth induced in the base by a monochromatic light of incident flow ( ) φ λ , respectively with monochromatic absorption and reflecting coefficients ( ) α λ and ( ) R λ . It is then written by the following relation: With τ the excess minority carrier lifetime in the base.

( )
, D T ω is the complex diffusion coefficient of excess minority carrier in the base at T-temperature. Its expression is given by the relationship [14]: D T is the temperature-dependent diffusion coefficient given by Einstein's relationship [15]: T is the temperature in Kelvin, K b the Boltzmann constant: The minority carrier mobility coefficient [16] expressed according to the temperature, is given by: By replacing the Equations (2) and (3) in the Equation (1), the continuity equation for the excess minority carriers density in the base is reduced to the following relationship: , , ω is the complex diffusion length of excess minority carrier in the base; ilest donné par : (ω, T) is the ac minority carriers diffusion coefficient in the base under the influence of temperature and the minority carrier lifetime in the base.

Journal of Modern Physics
Thus the solution of the Equation (9) is given by the following expression of the ac density of minority carriers: Coefficients A and B are determined from conditions at the base space boundaries, i.e. at the junction (x = 0) and in the rear (x = H) and are expressed by: 1) At, x = 0, at the junction emitter-base (n/p) surface 2) At, x = H, the back surface (p/p+) where Sf is the junction surface recombination velocity [17]. It can be represented into the sum of two terms. We then get: Sb is the excess minority carrier recombination velocity at the rear surface of the solar cell's base (p/p+) [19]. It characterizes the electric field in this area (low-high junction), which allows the return of minority carrier to the junction to participate in the photocurrent.

Diffusion Coefficient: Bode and Nyquist Diagrams for Différent Temperatures
The amplitude and phase of the diffusion coefficient under different temperatures, are represented versus frequency, through the Figure 3 and Figure 4.

Photocurrent
The density of photocurrent at the junction is obtained from the density of minority carriers in the base and is given by the following expression:  ⋅ ∂ (15) where q is the elementary electron charge. Figure 6 shows ac photocurrent density versus the junction surface recombination velocity for different temperatures.

Deduction of the Sb(ω, T) Expression
The representation of photocurrent density according to the junction recombination velocity of minority carriers shows that, for very large Sf, a bearing sets up and corresponds to the short-circuit current density (Jphsc). So in this junction recombination velocity interval, we can write [20]: The solution of this equation leads to expressions of the ac recombination velocity in the back surface, given by: Previous studies have looked at the second solution given to the Equation (18). Our study will consider this second solution, whose module and phase are represented versus the logarithm of the modulation frequency by the Figure 7 and Figure 8, for different temperatures.   and can be written as: We define the ac phase for a given temperature, as following equation: φ ω correspond for a given temperature T, to the amplitude and phase component of Sb.
At low frequencies (≤10 4 rad/s), the stationary regime is observed and gives constant amplitudes for each T. These amplitudes decrease with the temperature T. Beyond the frequency ( 4 10 rad/s), the cut-off frequency (ω c , sb(T)) is determined for each temperature. It is noted that the cut-off frequency decreases with the temperature T, as does the amplitude (Sb ampl ) and on the other hand the frequency (ω Sb (T)) of oscillations increases, in the part corresponding to the dynamic regime(See Table 1).
The phase is represented versus the logarithm of the modulation frequency.
The part corresponding to the dynamic regime shows sinusoidal oscillations between positive and negative values of the phase, amplitude (Φampl) that decreases with the temperature T and the frequency of oscillations (ω Φ ), which on the other hand increases with the temperature T (See Table 2). Figure 9 produces the Niquyst diagram of the excess minority carrier recombination velocity for different temperatures. The radius of the resulting circles decreases with temperature, with a shift from the center of the circles to the origin of the axes (See Table 3 and Table 4). Figure 10 and Figure 11 show that the sb recombination velocity decreases with temperature. Indeed, when the temperature is above the optimum temperature (Topt-300 K) [24], thermal agitation leads to the exponential evolution of umklapp processes that predict a temperature dependence of thermal conductivity      in 1/T [25] [26] [27]. This decreases the mobility of excess minority carriers and results in a decrease in the diffusion coefficient [25] which increases recombination.
The negative phase of the ac Sb recombination velocity and the determination of electrical parameters, with the Bode and Nyquist diagrams, characterizing Sb, allow to determine the equivalent electric model [28] [29].

Conclusion
The solar cell's ac back surface (p/p+) recombination velocity that controls the recombination of the excess minority carrier has been determined. Thus, the spectroscopy method allowed the study of the Bode and Nyquist diagrams and extracted certain electrical parameters characterizing the equivalent electric model. The effect of temperature on back surface recombination velocity was explained by umklapp processes.