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On the Analytical Solution of the Sirv-Model for the Temporal Evolution of Epidemics for General Time-Dependent Recovery, Infection and Vaccination Rates

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23 December 2023

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Abstract
The susceptible-infected-recovered/removed-vaccinated (SIRV) epidemics model is an important generalization of the SIR epidemics model as it accounts quantitatively for the effects of vaccination campaigns on the temporal evolution of epidemics outbreaks. Additional to the time-dependent infection ($a(t)$) and recovery ($\mu (t)$) rates, regulating the transitions between the compartments $S\to I$ and $I\to R$, respectively, the time-dependent vaccination rate $v(t)$ accounts for the transition between the compartments $S\to V$ of susceptible to vaccinated fractions. An accurate analytical approximation is derived for arbitrary and different temporal dependencies of the rates which is valid for all times after the start of the epidemics for which the cumulative fraction of new infections $J(t)\ll 1$. As vaccination campaigns automatically reduce the rate of new infections by transferring susceptible to vaccinated persons, the limit $J(t)\ll 1$ is even better fulfilled than in the SIR-epidemics model. The comparison of the analytical approximation for the temporal dependence of the rate of new infections $\jt(t)=a(t)S(t)I(t)$, the corresponding cumulative fraction $J(t)$, and $V(t)$, respectively, with the exact numerical solution of the SIRV-equations for different illustrative examples proves the accuracy of our approach. The considered illustrative examples include the cases of stationary ratios with a delayed start of vaccinations, and an oscillating ratio of recovery to infection rate with a delayed vaccination at constant rate. The proposed analytical approximation is self-regulating as the final analytical expression for the cumulative fraction $\jinf $ after infinite time allows us to check the validity of the original assumption $J(t)\le \jinf \ll 1$.
Keywords: 
Subject: Computer Science and Mathematics  -   Applied Mathematics

1. Introduction

The susceptible-infected-recovered/removed-vaccinated (SIRV) epidemic model [1,2,3,4,5,6,7,8,9,10,11,12,13,14,15,16,17,18,19,20,21,22] is an important generalization of the simpler susceptible-infected -recovered/removed (SIR) epidemic model [23,24,25,26,27] as it accounts for the effects of vaccination campaigns on a considered population, while the original SIR model does not take into account vaccination campaigns. In the SIRV model the time-dependent infection ( a ( t ) ), recovery ( μ ( t ) ) and vaccination ( v ( t ) ) rates regulate the transitions between the compartments S I , I R and S V , respectively. Two important key parameters of the SIRV pandemic model are the ratios k ( t ) = μ ( t ) / a ( t ) of the recovery to infection rate and b ( t ) = v ( t ) / a ( t ) of the vaccination to infection rate. Existing analytical solutions to the SIRV equations [2,28] have adopted originally stationary values of the ratios k ( t ) = k 0 and b ( t ) = b 0 , allowing for arbitrary time-dependent infection rates a ( t ) so that the recovery and vaccination rates have the same time dependence as the infection rate. Here we apply the recently developed analytical approach for the solution of the SIR-epidemics model [29] to the SIRV-epidemics model. For all times after the start of the epidemic, for which the cumulative fraction of infected persons J ( t ) 1 is much less then unity, an accurate analytical approximative solution of the SIRV equations is possible for general and arbitrary time dependences of the infection ( a ( t ) ), recovery ( μ ( t ) ) and vaccination ( v ( t ) ) rates. As vaccination campaigns automatically reduce the rate of new infections by transferring susceptible persons directly to vaccinated persons, who then no longer can get infected, the limit J 1 is even better fulfilled than in the SIR-epidemics model.
Of high interest, especially from the medical and public health care points of view, are the rate of new infections J ˚ ( t ) and its corresponding cumulative number J ( t ) , defined by
J ˚ ( t ) = a ( t ) S ( t ) I ( t ) , J ( t ) = J ( t 0 ) + t 0 t d ξ J ˚ ( ξ ) ,
respectively, after the start of the pandemic outburst at time t 0 , as the hospitalization and death rates are directly proportional to J ˚ ( t ) . Forecasts of the hospitalization and death rates are essential in order to prepare a community for an upcoming pandemic outburst by introducing non-pharmaceutical interventions and/or vaccination campaigns at an optimized time.
The organization of the manuscript is as follows. In Sect. 2 we introduce the starting SIRV-model equations both in terms of the real time t and the reduced time τ = t 0 t d ξ a ( ξ ) . It is beneficial for the analysis to express the SIRV-equations in a form directly involving the observable quantities such as rate of new infections j ( τ ) = S ( τ ) I ( τ ) , the cumulative fraction of infections J ( τ ) = J ( 0 ) + 0 τ d x j ( x ) = η + 0 τ d x j ( x ) = 1 S ( τ ) V ( τ ) = R ( τ ) + I ( τ ) and the cumulative fraction of vaccinated persons V ( τ ) . As shown in Sect. 3 the SIRV-equations in this form allow an approximate analytical solution in the limit of small cumulative fractions J 1 . The approximate solution can be written both as function of the real and the reduced time. In Sect. 4 the approximate solutions are compared with the earlier obtained analytical results for the special case of stationary ratios between the recovery to infection rate and the vaccination to infection rate, respectively. In Sects. 5 and 6 we investigate two applications which were inaccessible to analytical treatment before. The considered applications include the cases of stationary ratios with a delayed start of vaccinations (Sect. V), and an oscillating ratio of recovery to infection rate with a delayed vaccination at constant rate (Sect. VI). Here the analytical approximations are compared with the exact numerical solution of the SIRV-equations for these two applications in order to test the accuracy of the analytical approach. A summary and conclusion (Sect. VII) completes the manuscript.

2. SIRV model

The original SIRV-equations read [1]
d S d t = a ( t ) S I v ( t ) S ,
d I d t = a ( t ) S I μ ( t ) I ,
d R d t = μ ( t ) I ,
d V d t = v ( t ) S ,
obeying the sum constraint
S ( t ) + I ( t ) + R ( t ) + V ( t ) = 1
at all times t t 0 after the start of the wave at time t 0 with the initial conditions
I ( t 0 ) = η , S ( t 0 ) = 1 η , R ( t 0 ) = 0 , V ( t 0 ) = 0 ,
where η is positive and usually very small, η 1 .
Recently, it has been demonstrated [30] that the SIRV equations (2) -() can be expressed as
b ( τ ) = d V d τ 1 V ( τ ) J ( τ ) ,
I ( τ ) = j ( τ ) 1 V ( τ ) J ( τ ) ,
and
k ( τ ) = 1 V ( τ ) J ( τ ) d d τ ln j ( τ ) 1 V ( τ ) J ( τ )
in terms of the reduced time
τ = t 0 t d ξ a ( ξ ) ,
and the ratios
k ( τ ) = μ ( τ ( t ) ) a ( τ ( t ) ) , b ( τ ) = v ( τ ( t ) ) a ( τ ( t ) ) .
The great advantage of the SIRV equations written in the form (8)–(10) is the direct involvement of observable and monitored quantities, such as the rate of new infections j ( τ ) = S ( τ ) I ( τ ) , the cumulative fraction of new infections J ( t ) = J ( τ ) = J ( 0 ) + 0 τ d x j ( x ) = η + 0 τ d x j ( x ) = 1 S ( τ ) V ( τ ) = R ( τ ) + I ( τ ) and the cumulative fraction of vaccinated persons V ( t ) = V ( τ ) . This has enabled the determination [30] of the time variation of the ratios k ( t ) and b ( t ) from past Covid-19 mutant waves. For completeness we note the SIRV equations (2)–(5) in terms of the reduced time (11)
d S d τ = S I b ( τ ) S ,
d I d τ = S I k ( τ ) I ,
d R d τ = k ( τ ) I ,
d V d τ = b ( τ ) S ,
1 = S ( τ ) + I ( τ ) + R ( τ ) + V ( τ ) .
In the following we will derive approximate analytical solutions of the four nonlinear differential equations (13)–(16) in the limit of small J ( τ ) 1 and prove its accuracy by comparing with the exact numerical solutions of these equations for a number of illustrative examples of the reduced time dependence of the ratios k ( τ ) and b ( τ ) . As will be demonstrated the proposed analytical approximation is self-regulating as the final analytical expression for the cumulative fraction J = lim t J ( t ) after infinite time allows us to check the validity of the original assumption J ( t ) = J ( τ ) J 1 ,

3. Approximative analytical solutions

3.1. Solution in the limit of small J 1

Initially at reduced time τ = 0 the cumulative number of new infections is extremely small. In the limit J ( τ ) J 1 , where J = J ( τ = ) , also at later times we use the approximations 1 J ( τ ) 1 J to obtain for Eq. (8)
b ( τ ) d V d τ 1 J V ( τ ) = d d τ ln [ 1 J V ( τ ) ] 1 ,
With the initial condition V ( 0 ) = 0 for arbitrary but given dependencies b ( τ ) , Eq. (18) immediately integrates to
V ( τ ) ( 1 J ) [ 1 e 0 τ d x b ( x ) ] ,
which approaches V = V ( ) = 1 J after infinite time.
Likewise, in the same limit J J 1 Eq. (10) becomes
k ( τ ) 1 J V ( τ ) d d τ ln j ( τ ) 1 J V ( τ ) = ( 1 J ) e 0 τ d x b ( x ) d d τ ln j ( τ ) e 0 τ d x b ( x ) 1 J ,
where we inserted Eq. (19). With the initial condition j ( 0 ) = η ( 1 η ) Eq. (20) integrates to
j ( τ ) η ( 1 η ) exp 0 τ d x ( 1 J ) e 0 x d y b ( y ) k ( x ) b ( x ) .
Because of the adopted smallness J 1 we simplify the approximative solution (21) in the following as
j ( τ ) η ( 1 η ) exp 0 τ d x e 0 x d y b ( y ) k ( x ) b ( x ) .
but we keep the J in the solution (19) in order not to violate the restriction J ( τ ) + V ( τ ) J + V 1 .
In terms of the real time in this early time limit the approximative solution (19) and (22) read
V ( t ) ( 1 J ) [ 1 e t 0 t d ξ v ( ξ ) ] ,
and
J ˚ ( t ) a ( t ) η ( 1 η ) exp 0 t d ξ [ a ( ξ ) e t 0 ξ d y v ( y ) μ ( ξ ) v ( ξ ) ] ,
respectively.

3.2. Comparison with the SIR model limit

The SIR model corresponds to the limit of no vaccinations v = b = 0 , corresponding to V = 0 . In this limit the solutions (22) and (24) reduce to
j SIR ( τ ) η ( 1 η ) e 0 τ d x [ 1 k ( x ) ]
and
J ˚ SIR ( t ) a ( t ) η ( 1 η ) e 0 t d ξ [ a ( ξ ) μ ( ξ ] ,
respectively, in perfect agreement with the earlier derived Eqs. (15) and (17) of ref. [29].

3.3. Properties of the approximative solution (22)

The approximative solution (22) is predominantly determined by the reduced time variation of the ratios k ( τ ) and b ( τ ) . For the first and second time derivatives of the solution (22) we obtain
d j d τ = η ( 1 η ) e 0 τ d y b ( y ) k ( τ ) b ( τ ) exp 0 τ d x e 0 x d y b ( y ) k ( x ) b ( x ) ,
d 2 j d τ 2 = η ( 1 η ) [ e 0 τ d y b ( y ) k ( τ ) b ( τ ) ] 2 d k d τ d b d τ b ( τ ) e 0 τ d y b ( y ) exp 0 τ d x e 0 x d y b ( y ) k ( x ) b ( x ) .
Consequently, extrema of the rate of new infections occur at reduced times τ E determined by
k ( τ E ) + b ( τ E ) = e 0 τ E d y b ( y ) .
As the right-hand side of this Eq. is smaller or equal than unity no extrema of infections occur for a sum of variations
k ( τ ) + b ( τ ) > 1
greater than unity at all times. As both rates are semi-positive the condition (30) for no extrema in the rate iof new infections is fulfilled if either the vaccination rate v ( t ) > a ( t ) is greater than the infection rate and/or the recovery rate μ ( t ) > a ( t ) is greater than the infection rate.
In the case of reduced time intervals where
k ( τ ) + b ( τ ) < 1 ,
we obtain
[ d 2 j d τ 2 ] τ E = η ( 1 η ) [ d k d τ ] τ E + [ d b d τ ] τ E + b 2 ( τ E ) + b ( τ E ) k ( τ E ) exp 0 τ E d x e 0 x d y b ( y ) k ( x ) b ( x ) ,
so that the extrema are maxima if
[ d k d τ ] τ E + [ d b d τ ] τ E + b 2 ( τ E ) + b ( τ E ) k ( τ E ) > 0
is positive. Alternatively, the extrema are minima if
[ d k d τ ] τ E + [ d b d τ ] τ E + b 2 ( τ E ) + b ( τ E ) k ( τ E ) < 0
is negative. Note that there can be multiple minima and maxima depending on the reduced time variation of the ratios k ( τ ) and b ( τ ) . The extreme values of the rate of new infections in the case τ E < τ c are given by
j E ( τ E τ c ) = η ( 1 η ) e 0 τ E d x e 0 x d y b ( y ) k ( x ) b ( x ) .

3.4. Cumulative fraction

Integrating the rate of new infections (22) provides us with the corresponding cumulative fraction
J ( τ τ c ) = η + η ( 1 η ) 0 τ d z exp 0 z d x ( e 0 x d y b ( y ) k ( z ) b ( z ) ) .
For general reduced time variations k ( τ ) and b ( τ ) the integral in Eq. (36) can be reasonably well approximated evaluated using the method of steepest descent [31,32] by expanding the argument in the exponential function in Eq. (36) to second order in z around its (possible multiple) minimum values τ m
h ( z ) = 0 z d x ( e 0 x d y b ( y ) k ( z ) b ( z ) ) h ( τ m ) + ( z τ m ) 2 2 h m   ,
where
h m = [ d 2 h ( z ) d z 2 ] τ m .
With this expansion we obtain for the cumulative fraction (36)
J ( τ τ c ) η + η ( 1 η ) m π 2 h m   e h ( τ m ) erf h m   2 ( τ τ m ) + erf h m   2 τ m ,
where the sum of m accounts for possible multiple minima and
h ( τ m ) = 0 τ m d x k ( x ) + b ( x ) e 0 x d y b ( y ) , h m = [ d k d τ ] τ m + [ d b d τ ] τ m + b 2 ( τ m ) + b ( τ m ) k ( τ m ) .
For a minimum the second derivative h m > 0 has to be positive. The minima occur at times given by
k ( τ m ) + b ( τ m ) = e 0 τ m d y b ( y ) ,
and, as discussed before, see Eqs. (29)–(31) only for reduced time intervals where the sum k ( τ ) + b ( τ ) < 1 is less than unity.

4. Special case: stationary ratios

We first consider the approximative solutions (19) and (22) in the special case of stationary ratios
k ( τ ) = k 0 , b ( τ ) = b 0 ,
considered before [1]. We readily obtain
V ( τ ) = ( 1 J ) [ 1 e b 0 τ ] ,
and
j ( τ ) = η ( 1 η ) exp 1 e b 0 τ b 0 ( k 0 + b 0 ) τ .
Provided k 0 + b 0 < 1 the rate of new infections (44) attains its maximum value at the reduced time
τ m = ln ( k 0 + b 0 ) b 0 .
The maximum rate of new infections then is
j max = j ( τ m ) = η ( 1 η ) ( k 0 + b 0 ) k 0 + b 0 b 0 e 1 ( k 0 + b 0 ) b 0 .
Equations (45) and (46) agree exactly with Eqs. (98) and (100) derived before [1].

4.1. Cumulative fraction

Integrating Eq. (44) yields for the cumulative fraction
J ( τ ) = η + η ( 1 η ) H ( τ ) ,
with the integral
H ( τ ) = 0 τ d x exp 1 e b 0 x b 0 ( k 0 + b 0 ) x = b 0 k 0 b 0 e 1 b 0 e b 0 τ b 0 1 b 0 d y y k 0 b 0 e y ,
where we substituted y = e b 0 x / b 0 . The integral (48) can be expressed as the difference of two lower incomplete gamma functions
γ ( s , x ) = 0 x t s 1 e t d t = Γ ( s ) Γ ( s , x ) ,
yielding
H ( τ ) = b 0 k 0 b 0 e 1 b 0 γ 1 + k 0 b 0 , 1 b 0 γ 1 + k 0 b 0 , e b 0 τ b 0 ,
so that the cumulative fraction (47) is given by
J ( τ ) = η + η ( 1 η ) b 0 k 0 b 0 e 1 b 0 γ 1 + k 0 b 0 , 1 b 0 γ 1 + k 0 b 0 , e b 0 τ b 0 .
For infinitely large times the fraction (51) approaches the final value
J = J ( τ = ) = η + η ( 1 η ) b 0 k 0 b 0 e 1 b 0 γ 1 + k 0 b 0 , 1 b 0 .
Equations (51) and (52) agree exactly with the earlier derived Eqs. (A10) and (102) of ref. [1], using a different approach.
Because the analytical approximations were derived in the limit J J 1 , for consistency we have to require J < 1 for the values of k 0 and b 0 for which our approximation holds. In Figure 1 we calculate the required values of k 0 and b 0 fulfilling J < 1 using Eq. (52). The required values depend on the initial condition encoded by η , and are located above the line shown in this figure. For sufficiently large k 0 , J < 1 for any ratio b 0 , while at low recovery to infection ratios k 0 , the vaccination to infection rate must be significant to ensure J < 1 . The regime of b 0 close to zero is numerically difficult to evaluate using Eq. (52).

4.2. Limit b 0 1

In the limit of small b 0 1 we use relation (49) and the asymptotic expansion (Eq. 6.5.32 in [33]) of the upper incomplete gamma function for large arguments x 1
Γ ( s , x 1 ) x s 1 e x 1 + s 1 x + ( s 1 ) ( s 2 ) x 2 + ,
to obtain for
γ 1 + k 0 b 0 , 1 b 0 Γ 1 + k 0 b 0 b 0 k 0 b 0 e 1 b 0 [ 1 + k 0 + k 0 ( k 0 1 ) + ]
The fraction (52) then becomes
J ( b 0 1 ) η + η ( 1 η ) Γ 1 + k 0 b 0 b 0 k 0 b 0 e 1 b 0 [ 1 + k 0 + k 0 ( k 0 1 ) + ]
Using Stirling’s (Eq. 6.1.37 in [33]) formula for the gamma function Γ ( x + 1 ) 2 π x ( x / e ) x [ 1 + ( 12 x ) 1 ] for large x, Eq. (55) becomes,
J ( b 0 1 ) η + η ( 1 η ) 2 π k 0 b 0 k 0 k 0 b 0 e 1 k 0 b 0 1 + b 0 12 k 0 [ 1 + k 0 + k 0 ( k 0 1 ) + ]
For values of b 0 < k 0 < 1 the fraction (56) to leading orders is given by
J ( b 0 1 ) η + η ( 1 η ) 2 π k 0 / b 0 e ( 1 k 0 ) / b 0 k 0 k 0 / b 0 1 .
Because one has to require J 1 , or equivalently, ln ( J ) 0 , Eq. (57) turns into an inequality for b 0 , that can be written in terms of the principal branch W 0 of Lambert’s W-function, because ( x / b 0 ) ln b 0 = ln y is solved for any x 0 and y by x / W 0 ( x y ) , leading to
b 0 2 ( 1 k 0 + k 0 ln k 0 ) W 0 ( 1 + η ) 2 [ 1 k 0 + k 0 ln ( k 0 ) ] π k 0 η 2 .
This inequality (58) ensures J 1 . Along with the information contained in Eq. (52), it is visualized in Figure 1.

5. Stationary ratios with delayed start of vaccinations

As first new application of our results we discuss the case of stationary ratio k ( τ ) = k 0 for all reduced times and the influence of a stationary ratio b ( τ ) starting at the delayed reduced time τ v > 0 , i.e.,
k ( τ ) = k 0 , b ( τ ) = b 0 Θ ( τ τ v )
where Θ ( x < 0 ) = 0 and Θ ( x 1 ) denotes the step function. We then obtain for Eq. (19), i.e., in the limit J 1 , V = 0 for τ < τ V and
V ( τ τ v ) = ( 1 J ) [ 1 e b 0 ( τ τ v ) ] .
Likewise the rate (22) becomes the SIR-rate [29]
j ( 0 τ < τ v ) = η ( 1 η ) e ( 1 k 0 ) τ
at times without vaccination and
j ( τ τ v ) = η ( 1 η ) exp ( 1 k 0 ) τ v + 1 e b 0 ( τ τ v ) b 0 ( k 0 + b 0 ) ( τ τ v )
at later times. While the SIR-rate (61) is exponentially increasing in reduced time, the rate (62) has a maximum value
j max = j ( τ m ) = η ( 1 η ) exp ( 1 k 0 ) τ v + 1 e b 0 ( τ m τ v ) b 0 ( k 0 + b 0 ) ( τ m τ v ) = η ( 1 η ) ( k 0 + b 0 ) k 0 + b 0 b 0 exp ( 1 k 0 ) τ v + 1 ( k 0 + b 0 ) b 0 ,
provided k 0 + b 0 < 1 , the rate of new infections attains its maximum at the reduced time
τ m = τ v ln ( k 0 + b 0 ) b 0 .
We first note that for τ v = 0 the rates (62) and (63) correctly reproduce the earlier results (44) and (46). We emphasize that the delayed start of the vaccinations increases both the maximum time of the rate of infections and the maximum rate of new infections. Compared to the case of no delay in the start of vaccinations ( τ v = 0 ) we introduce the enhancement factor for the maximum rate
E ( τ v ) = j max ( τ v ) j max ( τ v = 0 ) = e ( 1 k 0 ) τ v ,
shown in Figure 2, which is independent of the vaccination rate and determined by the values of k 0 and τ v . Apparently, this exponential enhancement solely results from the new infections before the vaccinations start. While the enhancement factor increases exponentially over a wide range of k 0 τ v , in accord with Eq. (65), it numerically reaches a plateau as k 0 τ v approaches infinity, whose height increases with decreasing η . This is a clear indications that for large values of the enhancement factor a regime is reached where no longer J ( τ m ) is much smaller than unity so that the analytical approximation no longer holds. This explanation is supported by the cumulative fraction at large times (68) (see below) being directly proportional to the enhancement factor (65).
Integrating the rates of new injections (61) and (63) yields for the cumulative fraction
J ( 0 τ < τ v ) = η + η ( 1 η ) 1 k 0 [ e ( 1 k 0 ) τ 1 ] ,
and
J ( τ τ v ) = η + η ( 1 η ) 1 k 0 e ( 1 k 0 ) τ v 1 + η ( 1 η ) b 0 k 0 b 0 e ( 1 k 0 ) τ v + 1 b 0 γ 1 + k 0 b 0 , 1 b 0 γ 1 + k 0 b 0 , e b 0 ( τ τ v ) b 0 .
For infinite large times the fraction (67) approaches the final value
J = J ( τ = ) = η + η ( 1 η ) 1 k 0 e ( 1 k 0 ) τ v 1 + η ( 1 η ) b 0 k 0 b 0 e ( 1 k 0 ) τ v + 1 b 0 γ 1 + k 0 b 0 , 1 b 0 = η ( 1 η ) 1 k 0 E ( τ v ) 1 + ( 1 k 0 ) b 0 k 0 b 0 e 1 b 0 γ 1 + k 0 b 0 , 1 b 0 + η ( η k 0 ) 1 k 0 .
An example showing all quantities calculated analytically in this section, along with the numerical solution for a case with J 1 (Figure 1), is given in Figure 3.

6. Oscillating ratio k with delayed vaccinations at constant rate b 0

As second application we investigate the influence of delayed vaccinations with constant rate on the earlier discussed SIR-application [29] with an oscillating k ratio and delayed vaccination ratio b,
k ( τ ) = 1 + α sin ( β τ ) ,
b ( t ) = b 0 Θ ( τ τ v ) ,
with constant values α and β . As noted before [29] the oscillating ratio (69) represents a series of repeating pandemic outbursts with equal amplitudes in the rate of new infections. We then obtain for Eq. (19) V = 0 for τ < τ V and
V ( τ τ v ) = 1 e b 0 ( τ τ v ) .
Likewise the rate (22) becomes the SIR-rate [29]
j ( 0 τ τ v ) = η ( 1 η ) e α β [ cos ( β τ ) 1 ]
at times without vaccination, and
j ( τ τ v ) = η ( 1 η ) exp α β cos ( β τ ) 1 + 1 e b 0 ( τ τ v ) b 0 ( 1 + b 0 ) ( τ τ v )
at later times. In Figure 4-a we show the rate of new infections (72)–(73) in the case α = 0 . 8 and β = 0 . 5 for several values of the starting time of vaccinations τ v and the vaccination rate b 0 = 0 . 2 . We also compare in each case the analytical approximations with the exact rates of new infections from solving the SIRV equations numerically.
For the corresponding cumulative fractions one finds [29]
J ( τ τ v ) = η + η ( 1 η ) e α β τ I 0 α β + 2 n = 1 I n ( α β ) n β sin ( n β τ )
in terms of an infinite series of the modified Bessel function of the first kind I n ( z ) , and
J ( τ τ v ) = η + η ( 1 η ) e α β M ( τ ) + τ v I 0 ( α β ) + 2 n = 1 I n ( α β ) n β sin ( n β τ v ) ,
with the integral
M ( τ ) = τ v τ d x e α β cos ( β x ) ( 1 + b 0 ) ( x τ v ) + 1 e b 0 ( x τ v ) b 0 = 0 τ τ v d y e α β cos [ β ( y + τ v ) ] + g ( y ) ,
where we substituted y = x τ and introduced the function
g ( y ) = 1 e b 0 y b 0 ( 1 + b 0 ) y .
This function (77) has the following asymptotic behaviors for small and large values of b 0 y , i.e.
g ( y ) b 0 y ( 1 + y 2 ) , for y b 0 1 , 1 b 0 ( 1 + b 0 ) y , d for y b 0 1 .
In the following we therefore approximate the function (77) as g ( y ) g A ( y ) with
g A ( y ) = b 0 y 1 + y 2 Θ b 0 1 y + 1 2 b 0 ( 1 + b 0 ) y ] Θ [ y b 0 1 .
With this approximation we calculate the integral (76). For values of τ τ v + b 0 1 we obtain
M ( τ τ v b 0 1 ) 0 τ τ v d y e α β cos [ β ( y + τ v ) ] b 0 y ( 1 + y 2 ) = 0 τ τ v d y I 0 α β + 2 n = 1 I n α β cos [ n β ( y + τ v ) ] e b 0 y ( 1 + y 2 ) = π 2 b 0 e b 0 2 I 0 α β erf b 0 2 ( τ τ v + 1 ) erf b 0 2 + 2 n = 1 I n α β e n 2 β 2 2 b 0 W n ( τ ) ,
with
W n ( τ ) = 2 b 0 π e b 0 / 2 e n 2 β 2 2 b 0 0 τ τ v d y cos [ n β ( y + τ v ) ] e b 0 y ( 1 + y 2 ) = e ı n β ( τ v 1 ) erf b 0 2 ( τ τ v + 1 ) ı n β 2 b 0 erf b 0 2 ı n β 2 b 0
in terms of error functions with complex arguments. The real part in Eq. (81) is calculated in detail in Appendix A providing
W n ( τ ) = cos [ n β ( τ v 1 ) ] erf b 0 2 ( τ τ v + 1 ) erf b 0 2 + e b 0 2 ( τ τ v + 1 ) 2 π 2 b 0 ( τ τ v + 1 ) cos [ n β ( τ v 1 ) ] cos n β τ e b 0 2 π 2 b 0 cos [ n β ( τ v 1 ) ] cos n β τ v + 2 e b 0 2 ( τ τ v + 1 ) 2 π m = 1 e m 2 4 2 b 0 ( τ τ v + 1 ) cos [ n β ( τ v 1 ) ] cosh ( m n β 2 b 0 ) cos n β τ + m sinh ( m n β 2 b 0 ) sin n β τ m 2 + 2 b 0 ( τ τ v + 1 ) 2 2 e b 0 2 π m = 1 e m 2 4 2 b 0 cos [ n β ( τ v 1 ) ] cosh ( m n β 2 b 0 ) cos n β τ v + m sinh ( m n β 2 b 0 ) sin n β τ v m 2 + 2 b 0 .
Likewise, in the alternative case τ τ v + b 0 1 we find
M ( τ τ v b 0 1 ) 0 b 0 1 d y e α β cos [ β ( y + τ v ) ] b 0 y ( 1 + y 2 ) + e 1 2 b 0 b 0 1 τ τ v d y e α β cos [ β ( y + τ v ) ] ( 1 + b 0 ) y = π 2 b 0 e b 0 2 I 0 α β erf b 0 2 ( 1 b 0 + 1 ) erf b 0 2 + 2 n = 1 I n α β e n 2 β 2 2 b 0 W n τ v + 1 b 0 + e 1 2 b 0 b 0 1 τ τ v d y I 0 α β + 2 n = 1 I n α β e ı n β ( y + τ v ) e ( 1 + b 0 ) y .
The remaining integrals can be evaluated with the help of
b 0 1 τ τ v d y e ( 1 + b 0 ) y = e 1 + b 0 b 0 e ( 1 + b 0 ) ( τ τ v ) 1 + b 0 ,
and
b 0 1 τ τ v d y e ı n β ( y + τ v ) ( 1 + b 0 ) y = 1 n 2 β 2 + ( 1 + b 0 ) 2 [ n β sin n β τ ( 1 + b 0 ) cos n β τ e ( 1 + b 0 ) ( τ τ v ) n β sin n β ( τ v + 1 b 0 ) ( 1 + b 0 ) cos n β ( τ v + 1 b 0 ) e 1 + b 0 b 0 ] .
Consequently, Eq. (83) becomes
M ( τ τ v b 0 1 ) π 2 b 0 e b 0 2 I 0 α β erf b 0 2 ( 1 b 0 + 1 ) erf b 0 2 + 2 n = 1 I n α β e n 2 β 2 2 b 0 W n ( τ v + 1 b 0 ) + e 1 2 b 0 I 0 α β e 1 + b 0 b 0 e ( 1 + b 0 ) ( τ τ v ) 1 + b 0 + 2 e 1 2 b 0 n = 1 I n ( α β ) n 2 β 2 + ( 1 + b 0 ) 2 × n β sin n β τ ( 1 + b 0 ) cos n β τ e ( 1 + b 0 ) ( τ τ v ) n β sin [ n β ( τ v + 1 b 0 ) ] ( 1 + b 0 ) cos [ n β ( τ v + 1 b 0 ) ] e 1 + b 0 b 0 .
For the cumulative fraction (75) we obtain
J ( τ v τ τ v + b 0 1 ) = η + η ( 1 η ) e α β τ v I 0 ( α β ) + 2 n = 1 I n ( α β ) n β sin ( n β τ v ) + M ( τ τ v b 0 1 ) ,
and
J ( τ τ v + b 0 1 ) = η + η ( 1 η ) e α β τ v I 0 ( α β ) + 2 n = 1 I n ( α β ) n β sin ( n β τ v ) + M ( τ τ v b 0 1 ) ,
by inserting Eq. (83) and (86), respectively. Hence the cumulative fraction after infinite time is given by
J = η + η ( 1 η ) e α β { τ v I 0 α β + 2 n = 1 I n ( α β ) n β sin ( n β τ v ) + π 2 b 0 e b 0 2 I 0 α β erf b 0 2 1 b 0 + 1 erf b 0 2 + 2 n = 1 I n α β e n 2 β 2 2 b 0 W n τ v + 1 b 0 + e 1 2 b 0 I 0 α β e 1 + b 0 b 0 1 + b 0 + 2 e 1 + 2 b 0 2 b 0 n = 1 I n ( α β ) n 2 β 2 + ( 1 + b 0 ) 2 ( 1 + b 0 ) cos [ n β ( τ v + 1 b 0 ) ] n β sin [ n β ( τ v + 1 b 0 ) ] } ,
which is compared in Figure 5 with the numerical values. It is sufficient to evaluate the sums up to n = m = 50 ; with this setting the calculation of a J value lasts only a fraction of a second.

7. Summary and conclusions

The dynamical equations of the susceptible-infected-recovered/removed-vaccinated (SIRV) epidemics model play an important role to predict and/or analyze the temporal evolution of epidemics outbreaks accounting quantitatively for the influence of vaccination campaigns. Additional to the time-dependent infection ( a ( t ) ) and recovery ( μ ( t ) ) rates, regulating the transitions between the compartments S I and I R , respectively, the time-dependent vaccination ( v ( t ) accounts for the transition between the compartments S V of susceptible to vaccinated fractions. Here apparently for the first time a new accurate analytical approximation is derived for arbitrary and different but given temporal dependences of the infection, recovery and vaccination rates, which is valid for all times after the start of the epidemics for which the cumulative fraction of new infections J ( t ) 1 is much less than unity. As vaccination campaigns automatically reduce the rate of new infections by transferring susceptible persons to vaccinated persons, who then no longer can get infected, the limit J 1 is even better fulfilled than in the SIR-epidemics model which does not account for vaccinations. The proposed analytical approximation is self-regulating as the final analytical expression for the cumulative fraction J after infinite time allows to check the validity of the original assumption J ( t ) J 1 , thus indicating the allowed range of parameter values describing the temporal dependence of the ratios k ( t ) = μ ( t ) / a ( t ) and b ( t ) = v ( t ) / a ( t ) .
The comparison of the analytical approximation for the temporal dependence of the rate of new infections J ˚ ( t ) = a ( t ) S ( t ) I ( t ) , the corresponding cumulative fraction of new infections J ( t ) = J ( t 0 ) + t 0 t d x j ( x ) ,and the fraction of vaccinated persons V ( t ) , respectively, with the exact numerical solution of the SIRV-equations for two different and interesting applications proves the accuracy of the analytical approach. These two applications were not accessible to analytical treatment before. The considered applications include the cases of stationary ratios with a delayed start of vaccinations, and an oscillating ratio of recovery to infection rate with a delayed vaccination at constant rate. The excellent agreement of the analytical approximations with the exact numerical solution of the SIRV-equations for these two applications proves the accuracy of the analytical approach. In the first case the effect of a delayed start of vaccinations on the maximum rate of new infections and on the final cumulative fraction of infected persons is quantitatively calculated demonstrating the importance of an early start of vaccinations during a new epidemic outburst. Moreover, the new analytical approximation agrees favorably well with the earlier obtained analytical approximation [28] for the case of stationary ratios between the recovery to infection rate and the vaccination to infection rate, respectively, implying that the time dependence of the three rates a ( t ) , μ ( t ) , and v ( t ) is the same.

Data Availability Statement

The data that support the findings of this study are available within the article.

Appendix A Reduction of the function W n (τ)

In order to reduce the function W n ( τ ) introduced in Eq. (81) we use for the error function with complex argument their infinite series representation (Eq. 7.1.29 in [33])
erf ( X + ı Y ) = erf X + e X 2 2 π X [ 1 cos 2 X Y + ı sin 2 X Y ] + 2 π e X 2 m = 1 e m 2 4 m 2 + 4 X 2 [ f m ( X , Y ) + ı g m ( X , Y ) ] ,
with
f m ( X , Y ) = 2 X 2 X cosh ( m Y ) cos ( 2 X Y ) + m sinh ( m Y ) sin ( 2 X Y ) , g m ( X , Y ) = 2 X cosh ( m Y ) sin ( 2 X Y ) + m sinh ( m Y ) cos ( 2 X Y )
and the properties f m ( X , Y ) = f m ( X , Y ) and g m ( X , Y ) = g m ( X , Y ) . After straightforward but tedious algebra one obtains for general real values of A, B and C for
e ı A erf ( C ı B ) = cos ( A ) erf ( C ) + e C 2 2 π C [ ( 1 cos 2 B C ) cos A + sin ( 2 B C ) sin A ] + 2 e C 2 π m = 1 e m 2 4 m 2 + 4 C 2 [ f m ( C , B ) cos A + g m ( C , B ) sin A ] = cos ( A ) erf ( C ) + e C 2 2 π C [ cos A cos ( A + 2 B C ) ] + 2 e C 2 π m = 1 e m 2 4 m 2 + 4 C 2 { 2 C [ cos A cosh ( m B ) cos ( A + 2 B C ) ] + m sinh ( m B ) sin ( A + 2 B C ) } .
Applying Eq. (A3) to the two error functions in Eq. (81) then yields Eq. (82). For A, B, C equally distributed in the range [ 0 , 10 ] , the first term cos ( A ) erf ( C ) in Eq. (A3) contributes on average about 97% to the full expression. This feature can be used to write down a simplified expression for W n ( τ ) .

References

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Figure 1. Required lower limiting values of b 0 versus k 0 , fulfilling J 1 using Eq. (52), for various initial η (solid lines). Within the ( k 0 , b 0 ) -region above a certain solid line, J < 1 , while the exact numerical solution features J 1 for any choice of k 0 and b 0 . The regime b 0 1 is numerically difficult to evaluate using Eq. (52); beyond k 0 > 1 / 2 (marked by black dots), we use the explicit Eq. (58). For k 0 < 1 / 2 , the Eq. (58) is shown as dashed line, highlighting the region of k 0 where Eq. (58) cannot be used.
Figure 1. Required lower limiting values of b 0 versus k 0 , fulfilling J 1 using Eq. (52), for various initial η (solid lines). Within the ( k 0 , b 0 ) -region above a certain solid line, J < 1 , while the exact numerical solution features J 1 for any choice of k 0 and b 0 . The regime b 0 1 is numerically difficult to evaluate using Eq. (52); beyond k 0 > 1 / 2 (marked by black dots), we use the explicit Eq. (58). For k 0 < 1 / 2 , the Eq. (58) is shown as dashed line, highlighting the region of k 0 where Eq. (58) cannot be used.
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Figure 2. The enhancement factor E ( τ v ) as function of k 0 τ v for various k 0 . Analytical result (65) (colored) compared with the numerical result (black) for b 0 = 0 . 5 and η = 10 5 . Note the double-logarithmic representation. The dashed parts of the analytic results highlight the regimes for which Eq. (65) cannot be used anymore, as J (68) exceeds unity.
Figure 2. The enhancement factor E ( τ v ) as function of k 0 τ v for various k 0 . Analytical result (65) (colored) compared with the numerical result (black) for b 0 = 0 . 5 and η = 10 5 . Note the double-logarithmic representation. The dashed parts of the analytic results highlight the regimes for which Eq. (65) cannot be used anymore, as J (68) exceeds unity.
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Figure 3. Example for Section 5 using k 0 = 0 . 7 , b 0 = 0 . 1 , τ v = 10 , and η = 10 5 . Numerical solution (solid black curve) for (a) j ( τ ) and (b) J ( τ ) . In (a) the analytical expressions (61) (blue) and (62) (red) had been added. The vertical lines are at τ = τ v (dashed) and τ = τ m (solid) according to Eq. (64). The filled red circle corresponds to Eq. (63). In (b) the analytical expressions are taken from Eqs. (66) (blue) and (67) (red), while the red circle marks the analytical expression for J according to Eq. (68).
Figure 3. Example for Section 5 using k 0 = 0 . 7 , b 0 = 0 . 1 , τ v = 10 , and η = 10 5 . Numerical solution (solid black curve) for (a) j ( τ ) and (b) J ( τ ) . In (a) the analytical expressions (61) (blue) and (62) (red) had been added. The vertical lines are at τ = τ v (dashed) and τ = τ m (solid) according to Eq. (64). The filled red circle corresponds to Eq. (63). In (b) the analytical expressions are taken from Eqs. (66) (blue) and (67) (red), while the red circle marks the analytical expression for J according to Eq. (68).
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Figure 4. (a) Perfect agreement between the analytical solutions (72) and (73) (colored) with the numerical solutions (black) for different values of τ v = 1 , 5 , 10 , 20 , 30 (see figure legends) at α = 0 . 8 , β = 0 . 5 , b 0 = 0 . 2 , and η = 10 5 . For times τ < τ v , the analytical solution is insensitive to τ v , and branches from this curve at τ = τ v . The vertical black lines are at τ = τ v (dashed) and τ = 2 π / β (solid), and τ = τ v + b 0 1 (dot-dashed). (b) Corresponding cumulative J ( τ ) . Numerical solution (black) together with the analytical Eqs. (74) and (87) - (88) (colored).
Figure 4. (a) Perfect agreement between the analytical solutions (72) and (73) (colored) with the numerical solutions (black) for different values of τ v = 1 , 5 , 10 , 20 , 30 (see figure legends) at α = 0 . 8 , β = 0 . 5 , b 0 = 0 . 2 , and η = 10 5 . For times τ < τ v , the analytical solution is insensitive to τ v , and branches from this curve at τ = τ v . The vertical black lines are at τ = τ v (dashed) and τ = 2 π / β (solid), and τ = τ v + b 0 1 (dot-dashed). (b) Corresponding cumulative J ( τ ) . Numerical solution (black) together with the analytical Eqs. (74) and (87) - (88) (colored).
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Figure 5. J as function of b 0 and τ v . Remaining parameters as in Fig Figure 4, i.e., α = 0 . 8 , β = 0 . 5 , and η = 10 5 . (a) The numerical result, (b) The analytic result using Eq. (89).
Figure 5. J as function of b 0 and τ v . Remaining parameters as in Fig Figure 4, i.e., α = 0 . 8 , β = 0 . 5 , and η = 10 5 . (a) The numerical result, (b) The analytic result using Eq. (89).
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