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Article

Solutions for Several Quadratic Trinomial Difference Equations and Partial Differential Difference Equations in C2

1
School of Mathematics and Computer Science, Gannan Normal University, Ganzhou 341000, China
2
School of Psychology, Jiangxi Normal University, Nanchang 330022, China
3
School of Mathematics and Computer Science, Shangrao Normal University, Shangrao 334001, China
*
Author to whom correspondence should be addressed.
These authors contributed equally to this work.
Axioms 2021, 10(2), 126; https://doi.org/10.3390/axioms10020126
Submission received: 8 May 2021 / Revised: 11 June 2021 / Accepted: 16 June 2021 / Published: 21 June 2021
(This article belongs to the Special Issue Complex Analysis)

Abstract

:
This article is to investigate the existence of entire solutions of several quadratic trinomial difference equations f ( z + c ) 2 + 2 α f ( z ) f ( z + c ) + f ( z ) 2 = e g ( z ) , and the partial differential difference equations f ( z + c ) 2 + 2 α f ( z + c ) f ( z ) z 1 + f ( z ) z 1 2 = e g ( z ) , f ( z + c ) 2 + 2 α f ( z + c ) f ( z ) z 1 + f ( z ) z 2 + f ( z ) z 1 + f ( z ) z 2 2 = e g ( z ) . We establish some theorems about the forms of the finite order transcendental entire solutions of these functional equations. We also list a series of examples to explain the existence of the finite order transcendental entire solutions of such equations. Meantime, some examples show that there exists a very significant difference with the previous literature on the growth order of the finite order transcendental entire solutions. Our results show that some functional equations can admit the transcendental entire solutions with any positive integer order. These results make a few improvements of the previous theorems given by Xu and Cao, Liu and Yang.

1. Introduction

Let α 2 ( 0 , 1 ) , z + c = ( z 1 + c 1 , z 2 + c 2 ) for z = ( z 1 , z 2 ) and c = ( c 1 , c 2 ) . This paper is devoted to investigating the transcendental entire solutions with finite order of the quadratic trinomial difference equation
f ( z + c ) 2 + 2 α f ( z ) f ( z + c ) + f ( z ) 2 = e g ( z ) ,
and the quadratic trinomial partial differential difference equations
f ( z + c ) 2 + 2 α f ( z + c ) f ( z ) z 1 + f ( z ) z 1 2 = e g ( z ) ,
f ( z + c ) 2 + 2 α f ( z + c ) f ( z ) z 1 + f ( z ) z 2 + f ( z ) z 1 + f ( z ) z 2 2 = e g ( z ) ,
where c 1 , c 2 are constants and g ( z ) is a polynomial in C 2 . When α = ± 1 , Equations (1)–(3) can be turned to the following equations
f ( z ) ± f ( z + c ) = ± e 1 2 g ( z ) ,
f ( z + c ) ± f z 1 = ± e 1 2 g ( z ) ,
f ( z + c ) ± ( f z 1 + f z 2 ) = ± e 1 2 g ( z ) ,
respectively. In fact, it is easy to get the entire solutions of (4)–(6); for example, f ( z ) = e z 1 + z 2 is a finite-order transcendental entire solution of Equation (4), if ( 1 ± e c 1 + c 2 ) = ± e b and g ( z ) = e 2 ( z 1 + z 2 ) + 2 , and f ( z ) = e a 1 z 1 + a 2 z 2 is a finite order entire solution of Equations (5) and (6), if e a 1 c 1 + a 2 c 2 ± a 1 = ± e b and e a 1 c 1 + a 2 c 2 ± ( a 1 + a 2 ) = ± e b , respectively, where g ( z ) = e 2 ( a 1 z 1 + a 2 z 2 ) + 2 b , a 1 ( 0 ) , a 2 , b are constants. When α = 0 and g ( z ) = 0 , Equations (1) and (2) become the Fermat type difference equations
f ( z + c ) 2 + f ( z ) 2 = 1
and
f ( z + c ) 2 + f z 1 2 = 1 ,
which were discussed by Xu and Cao [1]. They pointed out that the transcendental entire solution with finite order of Equation (7) must satisfy f ( z ) = sin ( A 1 z 1 + A 2 z 2 + C o n s t a n t ) , where A 1 2 = 1 and A 1 e i ( A 1 c 1 + A 2 c 2 ) = 1 , if c 2 0 , and any nonconstant entire solution with finite order of Equation (7) has the form of f ( z ) = cos ( A 1 z 1 + A 2 z 2 + C o n s t a n t ) , where A 1 c 1 + A 2 c 2 = π 2 2 k π , k Z . As is known, the study of the Fermat type functional equation
f 2 + g 2 = 1
can be tracked back to about sixty years ago or even earlier (see [2,3,4]). In 1966, Gross [2] discussed the existence of solutions of Equation (9) and showed that the entire solutions are f = cos a ( z ) , g = sin a ( z ) , where a ( z ) is an entire function. In recent years, with the development of Nevanlinna theory and difference Nevanlinns theory of meromorphic function with one and several variables ([5,6,7,8,9,10,11]), there were many references focusing on the solutions of Fermat type functional equations (readers can refer to [12,13,14,15,16,17,18,19]).
In 1999 and 2004, E. G. Saleeby [20,21] studied the forms of the entire and meromorphic solutions of some partial differential equations, extended some of the above conclusions to the case of several complex variables, and obtained the following results.
Theorem 1
(see ([20], Theorem 1)). If f is an entire solution of
f ( z 1 , z 2 ) z 1 2 + f ( z 1 , z 2 ) z 2 2 = 1
in C 2 , then f ( z 1 , z 2 ) = η 1 z 1 + η 2 z 2 + η where η 1 , η 2 , η C and η 1 2 + η 2 2 = 1 .
Theorem 2
(see ([21], Theorem 1)). The nonconstant entire and meromorphic solutions of equation
f ( z 1 , z 2 ) 2 + f ( z 1 , z 2 ) z 1 2 + f ( z 1 , z 2 ) z 2 2 = 1
are of the form f ( z 1 , z 2 ) = sin ( η 1 z 1 + η 2 z 2 + η ) , where η 1 , η 2 , η C and η 1 2 + η 2 2 = 1 .
In 2005, Li [22] discussed the partial differential equation of Fermat-type
u z 1 2 + u z 2 2 = e g ,
where g is a polynomial or an entire function in C 2 and obtained some results on the forms of entire solution of Equation (11) as follows:
Theorem 3
([22], Theorem 2.1). Let g be a polynomial in C 2 . Then, u is an entire solution of the partial differential Equation (11), if and only if:
(i)
u = f ( c 1 z 1 + c 2 z 2 ) ; or
(ii)
u = ϕ 1 ( z 1 + i z 2 ) + ϕ 2 ( z 1 i z 2 ) ,
where f is an entire function in C satisfying that f ( c 1 z 1 + c 2 z 2 ) = ± e 1 2 g ( z ) , c 1 and c 2 are two constants satisfying that c 1 2 + c 2 2 = 1 , and ϕ 1 and ϕ 2 are entire functions in C satisfying that ϕ 1 ( z 1 + i z 2 ) ϕ 2 ( z 1 i z 2 ) = 1 4 e g ( z ) .
Later, E. G. Saleeby [23] further investigated the entire and meromorphic solutions for the quadratic trinomial functional equations
f 2 + 2 α f g + g 2 = 1 , α 2 1 , α C ,
and obtained
Theorem 4
(see ([23], Theorem 2.1)).The entire and meromorphic solutions of (12) have the form given in, respectively,
f = 1 2 cos h 1 + α + sin h 1 α , g = 1 2 cos h 1 + α sin h 1 α
and
f = α 1 α 2 β 2 ( α 1 α 2 ) β , g = 1 β 2 ( α 1 α 2 ) β ,
where h is entire and β is meromorphic on C n .
Theorems 1–4 suggest the following question as an open problem.
Question 1.
What would happen to the existence and form of solution of Equation (12) when g is replaced of some special forms of f, and the right side of those equations 1 is replaced by a function e φ in Theorem D, where φ is a polynomial?

2. Results and Examples

Motivated by the above question, this article is concerned with the entire solutions for the difference Equation (1) and the partial differential difference Equations (2) and (3). The main tools are used in this paper are the Nevanlinna theory and difference Nevanlinna theory. Our results are obtained to generalize the previous theorems given by Xu and Cao, Liu, and Yang [1,24]. Here and below, let α 2 0 , 1 , and
A 1 = 1 2 1 + α i 2 1 α , A 2 = 1 2 1 + α + i 2 1 α .
Thus, we have A 1 A 2 = 4 1 α 2 .
The first main theorem is about the existence and the forms of the solutions for the quadratic trinomial difference Equation (1).
Theorem 5.
Let g ( z ) be a polynomial in C 2 and α 2 0 , 1 , c C 2 . If the difference Equation (1) admits a transcendental entire solution f ( z ) of finite order, then g ( z 1 , z 2 ) must be of the form g ( z 1 , z 2 ) = L ( z 1 , z 2 ) + H ( c 2 z 1 c 1 z 2 ) , where L ( z 1 , z 2 ) is a linear form of L ( z 1 , z 2 ) = a 1 z 1 + a 2 z 2 , H ( s ) is a polynomial in s, and a 1 , a 2 C . Further, f ( z 1 , z 2 ) must satisfy one of the following cases:
(i)
f ( z 1 , z 2 ) = 1 2 ( A 1 ξ + A 2 ξ 1 ) e 1 2 [ L ( z 1 , z 2 ) + H ( c 2 z 1 c 1 z 2 ) ] ,
where ξ ( 0 ) C and a 1 , a 2 , c 1 , c 2 , ξ , A 1 , A 2 satisfying
e 1 2 ( a 1 c 1 + a 2 c 2 ) = A 2 ξ + A 1 ξ 1 A 1 ξ + A 2 ξ 1 ;
or
(ii)
f ( z 1 , z 2 ) = 1 2 A 1 e L 1 ( z 1 , z 2 ) + H 1 ( c 2 z 1 c 1 z 2 ) + A 2 e L 2 ( z 1 , z 2 ) + H 2 ( c 2 z 1 c 1 z 2 ) ,
where L 1 ( z 1 , z 2 ) = a 11 z 1 + a 12 z 2 , L 2 ( z 1 , z 2 ) = a 21 z 1 + a 22 z 2 , H j ( s ) are polynomials in s, a i j C , ( i = 1 , 2 ; j = 1 , 2 ) satisfy L 1 ( z 1 , z 2 ) L 2 ( z 1 , z 2 ) ,
g ( z 1 , z 2 ) = L 1 ( z 1 , z 2 ) + L 2 ( z 1 , z 2 ) + H 1 ( c 2 z 1 c 1 z 2 ) + H 2 ( c 2 z 1 c 1 z 2 ) = L ( z 1 , z 2 ) + H ( c 2 z 1 c 1 z 2 ) ,
and
e a 11 c 1 + a 12 c 2 = A 2 A 1 , e a 21 c 1 + a 22 c 2 = A 1 A 2 , e a 1 c 1 + a 2 c 2 = 1 .
The following examples show that the forms of solutions are precise to some extent.
Example 1.
Let α = 1 2 and ξ = 1 . Then, it follows that A 1 = 1 3 ( 1 2 3 2 i ) , A 2 = 1 3 ( 1 2 + 3 2 i ) . Let
f ( z ) = 1 2 e z 1 + z 2 + 1 .
Thus, ρ ( f ) = 1 and f ( z ) is a transcendental entire solution of (1) with g ( z ) = 2 ( z 1 + z 2 ) + 2 and ( c 1 , c 2 ) = ( π i , 3 π i ) .
Remark 1.
Here and below, ρ ( f ) is the order of the function f, which is defined by
ρ ( f ) = lim sup r + log T ( r , f ) log r ,
where T ( r , f ) is the Nevanlinna characteristic function (see [9]).
Example 2.
Let α = 1 2 , a 11 = a 12 = 1 3 , a 21 = a 22 = 2 3 and b 1 = b 2 = 0 . Then, it follows that
f ( z ) = 1 3 e 1 3 ( z 1 + z 2 ) π 2 ( 3 z 1 z 2 ) 2 1 3 π i + e 2 3 ( z 1 + z 2 ) + π 4 ( 3 z 1 z 2 ) 4 + 1 3 π i .
Thus, ρ ( f ) = 4 and f ( z ) is a transcendental entire solution of (1) with ( c 1 , c 2 ) = ( π i 2 , 3 π i 2 ) and
g ( z ) = ( z 1 + z 2 ) π 2 ( 3 z 1 z 2 ) 2 + π 4 ( 3 z 1 z 2 ) 4 .
When f ( z + c ) is replaced by f z 1 or f z 1 + f z 2 in (1), we obtain the second theorem as follows.
Theorem 6.
Let α 2 0 , 1 , α C and g ( z ) be a polynomial in C 2 . If the partial differential equation
f ( z ) 2 + 2 α f ( z ) f ( z ) z 1 + f ( z ) z 1 2 = e g ( z )
admits a transcendental entire solution f ( z ) of finite order, then g ( z ) must be of the form g ( z ) = a 1 z 1 + φ ( z 2 ) , where φ ( z 2 ) is a polynomial in z 2 and a 1 C .
Theorem 7.
Let α 2 0 , 1 , α C and g ( z ) be a polynomial in C 2 . If the partial differential equation
f ( z ) 2 + 2 α f ( z ) f ( z ) z 1 + f ( z ) z 2 + f ( z ) z 1 + f ( z ) z 2 2 = e g ( z )
admits a transcendental entire solution f ( z ) of finite order, then g ( z ) must be of the form g ( z ) = a 1 z 1 + φ ( z 2 z 1 ) , where φ ( z 2 z 1 ) is a polynomial in z 2 z 1 and a 1 C .
The following examples show that the forms of solutions are precisely to some extent.
Example 3.
Let g ( z ) = 4 z 1 + z 2 + z 2 2 . Then, it is easy to get that the function
f ( z ) = 1 2 6 ( 1 3 ) e ( 2 + 3 ) z 1 + z 2 + ( 1 + 3 ) e ( 2 3 ) z 1 + z 2 2
is a transcendental entire solution of Equation (14) with α = 2 .
Example 4.
Let g ( z ) = 6 z 1 + ( z 2 z 1 ) 2 + ( z 2 z 1 ) 4 . Then, it is easy to get that the function
f ( z ) = 1 4 2 ( 1 2 ) e ( 3 2 2 ) z 1 + ( z 2 z 1 ) 2 + ( 1 + 2 ) e ( 2 2 3 ) z 1 + ( z 2 z 1 ) 4
is a transcendental entire solution of Equation (15) with α = 3 .
From Theorem 7, it is easy to get the following corollary.
Corollary 1.
Let α 2 0 , 1 , α C and g ( z ) be a polynomial in C 2 which the degree of z 1 is more than 2. Then, the following partial differential-difference equation
f ( z ) 2 + 2 α f ( z ) f ( z ) z 1 + f ( z ) z 1 2 = e g ( z )
admits no transcendental entire solution with finite order.
For the partial differential difference counterpart of Theorem 7, we have
Theorem 8.
Let α 2 0 , 1 , c 2 0 and g ( z ) be a nonconstant polynomial in C 2 , and not the form of ϕ ( z 2 ) . If the differential-difference Equation (2) admits a transcendental entire solution f ( z ) of finite order, then g ( z ) must be of the form g ( z ) = a 1 z 1 + a 2 z 2 + b , where a 1 ( 0 ) , a 2 , b C . Further, f ( z ) must satisfy one of the following cases:
(i)
f ( z ) = 2 a 1 ( A 1 ξ 1 + A 2 ξ ) e 1 2 ( a 1 z 1 + a 2 z 2 + b ) ,
where ξ ( 0 ) C and a 1 , a 2 , b , c 1 , c 2 , A 1 , A 2 , ξ satisfying
e 1 2 ( a 1 c 1 + a 2 c 2 ) = a 1 ( A 1 ξ + A 2 ξ 1 ) 2 ( A 2 ξ + A 1 ξ 1 ) ;
or
(ii)
f ( z ) = 1 2 A 2 a 11 e a 11 z 1 + a 12 z 2 + b 1 + A 1 a 21 e a 21 z 1 + a 22 z 2 + b 2 ,
where a j ( 0 ) , b j C , ( j = 1 , 2 ) satisfy a 11 z 1 + a 12 z 2 a 21 z 1 + a 22 z 2 ,
g ( z ) = ( a 11 + a 21 ) z 1 + ( a 12 + a 22 ) z 2 + b 1 + b 2 ,
and
e a 11 c 1 + a 12 c 2 = A 2 A 1 a 11 , e a 21 c 1 + a 22 c 2 = A 1 A 2 a 21 , e a 1 c 1 + a 2 c 2 = a 11 a 21 .
The following examples explain the existence of transcendental entire solutions with finite order of (2).
Example 5.
Let α = 1 2 and ξ = 1 . Then, it follows that A 1 = 2 3 e π 6 i and A 2 = 2 3 e π 6 i . Let
f ( z ) = 2 2 e 1 2 ( 2 z 1 + 3 z 2 + b ) .
Then, f ( z ) is a transcendental entire solution of Equation (2) with g ( z ) = 2 z 1 + 3 z 2 + b , ( c 1 , c 2 ) = ( π i 2 , 3 π i 2 ) and b C .
Example 6.
Let α = 1 2 , a 11 = a 12 = a 21 = 1 , a 22 = 1 and b 1 = b 2 = 0 . Let
f ( z ) = 1 3 e z 1 + z 2 + π 6 i + e z 1 z 2 π 6 i ,
then ρ ( f ) = 1 and f ( z ) is a transcendental entire solution of Equation (2) with g ( z ) = 2 z 1 and ( c 1 , c 2 ) = ( 0 , π 3 i ) .
The following example shows that the condition c 2 0 in Theorem 5 cannot be removed.
Example 7.
Let c 2 = 0 , α = 3 , a 11 be a root of equation e x = x ( 2 2 3 ) , and a 21 be a root of equation e x = x ( 3 + 2 2 ) . Thus, it follows a 11 a 21 . Let
f ( z ) = 1 4 2 1 + 2 a 11 e a 11 z 1 + a 12 z 2 + z 2 2 + 1 2 a 21 e a 21 z 1 + a 22 z 2 + z 2 3 ,
where a 12 , a 22 C , then ρ ( f ) = 3 and f ( z ) is a transcendental entire solution of Equation (3) with g ( z ) = ( a 11 + a 21 ) z 1 + ( a 12 + a 22 ) z 2 + z 2 2 + z 2 3 and ( c 1 , c 2 ) = ( 1 , 0 ) .
Remark 2.
From Example 7, we can see that ρ ( f ) = 3 > 1 and g ( z ) is not a linear form of z 1 , z 2 when c 2 = 0 for Equation (2). These are significant differences with the condition c 2 0 in Theorem 8. Thus, this shows that our results are precise to some extent.
Theorem 9.
Let α 2 0 , 1 , c 1 c 2 and g ( z ) be a nonconstant polynomial in C 2 , and not the form of ϕ ( z 2 z 1 ) . If f ( z ) is a finite-order transcendental entire solution of the differential-difference Equation (3), then f ( z ) , g ( z ) must satisfy one of the following cases:
(i) g ( z ) = a 1 z 1 + a 2 z 2 + b and
f ( z ) = 2 a 1 + a 2 ( A 2 ξ + A 1 ξ 1 ) e 1 2 ( a 1 z 1 + a 2 z 2 + b ) ,
where ξ ( 0 ) C and a 1 , a 2 , b , c , A 1 , A 2 , ξ satisfying
e 1 2 ( a 1 c 1 + a 2 c 2 ) = 1 2 A 1 ξ + A 2 ξ 1 A 2 ξ + A 1 ξ 1 ( a 1 + a 2 ) ;
or
(ii) g ( z ) = L 1 ( z ) + L 2 ( z ) + b 1 + b 2 and
f ( z ) = 1 2 A 2 a 11 + a 12 e L 1 ( z ) + b 1 + A 1 a 21 + a 22 e L 2 ( z ) + b 2 ,
where L 1 ( z ) = a 11 z 1 + a 12 z 2 , L 2 ( z ) = a 21 z 1 + a 22 z 2 , and a i j , b j C , ( i , j = 1 , 2 ) satisfy a 11 + a 12 0 , a 21 + a 22 0 , L 1 ( z ) L 2 ( z ) , and
e a 11 c 1 + a 12 c 2 = ( a 11 + a 12 ) A 1 A 2 , e a 21 c 1 + a 22 c 2 = ( a 21 + a 22 ) A 2 A 1 .
The following examples explain the existence of transcendental entire solutions with finite order of (3).
Example 8.
Let α = 3 and ξ = 1 . Then, it follows that A 1 = 1 4 1 2 2 and A 2 = 1 4 + 1 2 2 . Let
f ( z ) = 2 4 e z 1 2 z 2 + b .
Then, ρ ( f ) = 1 and f ( z ) is a transcendental entire solution of Equation (3) with g ( z ) = 2 z 1 4 z 2 + b , ( c 1 , c 2 ) = ( 3 π i , π i ) and b C .
Example 9.
Let α = 1 2 , a 11 = 2 , a 12 = 1 , a 21 = 2 , a 22 = 3 , and b 1 = b 2 = 0 . Let
f ( z ) = 1 3 e 2 z 1 z 2 + π 6 i e 2 z 1 3 z 2 π 6 i .
Then, ρ ( f ) = 1 and f ( z ) is a transcendental entire solution of Equation (3) with g ( z ) = 4 z 1 4 z 2 and ( c 1 , c 2 ) = ( π 12 i , π 6 i ) .
The following example shows that the condition c 1 c 2 in Theorem 9 cannot be removed.
Example 10.
Let c 1 = c 2 = 1 , α = 2 , a 11 , a 12 satisfy equation e a 11 + a 12 = ( a 11 + a 12 ) ( 3 2 ) , and a 21 , a 22 satisfy equation e a 21 + a 22 = ( a 21 + a 22 ) ( 3 + 2 ) . Thus, it follows that a 11 = a 21 and a 12 = a 22 cannot hold at the same time. Let
f ( z ) = 1 2 6 1 + 3 a 11 + a 12 e a 11 z 1 + a 12 z 2 + ( z 1 z 2 ) s + 1 3 a 21 + a 22 e a 21 z 1 + a 22 z 2 + ( z 1 z 2 ) t ,
where s , t Z + . Then, ρ ( f ) = max { s , t } and f ( z ) is a transcendental entire solution of Equation (3) with g ( z ) = ( a 11 + a 21 ) z 1 + ( a 12 + a 22 ) z 2 + ( z 1 z 2 ) s + ( z 1 z 2 ) t and ( c 1 , c 2 ) = ( 1 , 1 ) .
Remark 3.
By comparing the conclusions of Theorem 8 and Example 10, we can see that there are significant differences in the form of solution f ( z ) and g ( z ) when c 1 c 2 in (3).

3. Conclusions and Discussion

From Theorems 5 and 8, one can see that our theorems are very good supplements of the previous results given by Xu and Cao [1] because Equations (1) and (2) are more general than Equations (7) and (8). Moreover, Examples 2, 7, and 10 show that Equations (1)–(3) can admit the transcendental entire solutions with any positive integer order. However, Xu and Cao [1] showed that the order of the transcendental entire solutions of Equations (7) and (8) must be one. In fact, this is a very significant difference. Besides, by comparing with the abstract form of solution in Theorem D, we can get a more specific expression of the solution of Equation (12) when g is replaced by the special forms of f such as g = f ( z + c ) , g = f z 1 , etc. Finally, one can find that we only focus on the finite-order transcendental entire solutions of Equations (1)–(3) in this article; thus, the following questions can be raised naturally:
Question 2.
Do the infinite-order transcendental entire solutions of Equations (1)–(3) exist?
Question 3.
How should the meromorphic solutions of Equations (1)–(3) be characterized?

4. Some Lemmas

The following lemmas play the key roles in proving our results.
Lemma 1
([25], Lemma 3.2). Let f be a non-constant meromorphic function in C n . Then, for any I ( Z + ) n , T ( r , I f ) = O ( T ( r , f ) ) for all r except possibly a set of finite Lebesgue measure, and where I = ( i 1 , , i n ) ( Z + ) n denotes a multiple index with | I | = i 1 + + i n , Z + = { 0 , 1 , 2 , } , and I f = I f i n ζ n i 1 ζ 1
Lemma 2
([9,10]). For an entire function F on C n , F ( 0 ) 0 and put ρ ( n F ) = ρ < . Then, there exist a canonical function f F and a function g F C n such that F ( z ) = f F ( z ) e g F ( z ) . For the special case n = 1 , f F is the canonical product of Weierstrass.
Remark 4.
Here, denote ρ ( n F ) to be the order of the counting function of zeros of F.
Lemma 3
([4]). If g and h are entire functions on the complex plane C and g ( h ) is an entire function of finite order, then there are only two possible cases:
(a) the internal function h is a polynomial and the external function g is of finite order; or
(b) the internal function h is not a polynomial but a function of finite order, and the external function g is of zero order.
Lemma 4
([26], Lemma 3.1). Let f j ( 0 ) , j = 1 , 2 , 3 , be meromorphic functions on C m such that f 1 is not constant, f 1 + f 2 + f 3 = 1 , and
j = 1 3 N 2 ( r , 1 f j ) + 2 N ¯ ( r , f j ) < λ T ( r , f 1 ) + O ( log + T ( r , f 1 ) ) ,
for all r outside possibly a set with finite logarithmic measure, where λ < 1 is a positive number. Then, either f 2 = 1 or f 3 = 1 .
Remark 5.
Here, N 2 ( r , 1 f ) is the counting function of the zeros of f in | z | r , where the simple zero is counted once, and the multiple zero is counted twice.

5. The Proof of Theorem 5

Proof. 
Assume that f ( z ) is a transcendental entire solution with finite order of Equation (1). Set
f ( z ) = 1 2 ( u + v ) , f ( z + c ) = 1 2 ( u v ) ,
where u , v are entire functions in C 2 . Thus, Equation (1) can be written as
( 1 + α ) u 2 + ( 1 α ) v 2 = e g .
Hence, we can deduce from (17) that
1 + α u e g ( z ) 2 2 + 1 α v e g ( z ) 2 2 = 1 ,
which leads to
1 + α u e g ( z ) 2 + i 1 α v e g ( z ) 2 1 + α u e g ( z ) 2 i 1 α v e g ( z ) 2 = 1 .
In view of the assumptions, there exists a polynomial p ( z ) such that
1 + α u e g ( z ) 2 + i 1 α v e g ( z ) 2 = e p ( z ) , 1 + α u e g ( z ) 2 i 1 α v e g ( z ) 2 = e p ( z ) .
Denote
γ 1 ( z ) = g ( z ) 2 + p ( z ) , γ 2 ( z ) = g ( z ) 2 p ( z ) .
In view of (19), it follows that
1 + α u = e γ 1 ( z ) + e γ 2 ( z ) 2 , 1 α v = e γ 1 ( z ) e γ 2 ( z ) 2 i .
This leads to
f ( z ) = 1 2 e γ 1 ( z ) + e γ 2 ( z ) 2 1 + α + e γ 1 ( z ) e γ 2 ( z ) 2 1 α i = 1 2 ( A 1 e γ 1 ( z ) + A 2 e γ 2 ( z ) ) ,
f ( z + c ) = 1 2 e γ 1 ( z ) + e γ 2 ( z ) 2 1 + α e γ 1 ( z ) e γ 2 ( z ) 2 1 α i = 1 2 ( A 2 e γ 1 ( z ) + A 1 e γ 2 ( z ) ) ,
where A 1 , A 2 are defined in (13). Thus, in view of (21) and (22), it follows that
A 2 A 1 e γ 2 ( z + c ) γ 2 ( z ) A 2 A 1 e γ 1 ( z ) γ 2 ( z ) + e γ 1 ( z + c ) γ 2 ( z ) 1 .
We discuss two cases below.
Case 1. Suppose that γ 1 ( z + c ) γ 2 ( z ) is a constant. Let γ 1 ( z + c ) γ 2 ( z ) = κ , κ C . In view of (20), it follows that γ 1 ( z ) γ 2 ( z ) = 2 p ( z ) . Substituting these into (23), we have
e 2 p ( z ) + ( 1 η ) A 1 A 2 = e 2 p ( z + c ) η ,
where η = e κ . If η 1 , by using the Nevanlinna second fundamental theorem, we have
T ( r , e 2 p ) N ( r , 1 e 2 p ) + N ( r , 1 e 2 p δ ) + S ( r , e 2 p ) N ( r , 1 e 2 p ( z + c ) η ) + S ( r , e 2 p ) = S ( r , e 2 p ) ,
where δ = ( 1 η ) A 1 A 2 0 . This means that p ( z ) is a constant. Set ξ = e p . Substituting this into (21) and (22), we have
f ( z ) = 1 2 ( A 1 ξ + A 2 ξ 1 ) e 1 2 g ( z ) ,
f ( z + c ) = 1 2 ( A 2 ξ + A 1 ξ 1 ) e 1 2 g ( z ) .
From (25) and (26), it follows that
( A 1 ξ + A 2 ξ 1 ) e g ( z + c ) g ( z ) 2 = A 2 ξ + A 1 ξ 1 .
In view of α 2 1 , it follows that A 2 ξ + A 1 ξ 1 = 0 and ( A 1 ξ + A 2 ξ 1 ) = 0 cannot hold at the same time. Hence, we have A 2 ξ + A 1 ξ 1 0 and ( A 1 ξ + A 2 ξ 1 ) 0 . Since g ( z ) is a polynomial, (27) implies that g ( z + c ) g ( z ) is a constant in C . Otherwise, we obtain a contradiction from the fact that the left of the above equation is not transcendental but the right is transcendental. Thus, it follows that g ( z ) = L ( z ) + H ( s ) , where L ( z ) = a 1 z 1 + a 2 z 2 + H ( s ) , a 1 , a 2 are constants, and H ( s ) is a polynomial in s = c 2 z 1 c 1 z 2 satisfying
e 1 2 ( a 1 c 1 + a 2 c 2 ) = A 2 ξ + A 1 ξ 1 ( A 1 ξ + A 2 ξ 1 ) .
If η = 1 , it follows that κ = 2 k π i , k Z , and γ 1 ( z + c ) γ 2 ( z ) = 2 k π i . In view of (23), we have γ 2 ( z + c ) = γ 1 ( z ) . By combining with (20), we have g ( z + c ) = 2 k π i + g ( z ) . Thus, it follows that g ( z ) = L ( z ) + H ( s ) , where L ( z ) = a 1 z 1 + a 2 z 2 , H ( s ) is a polynomial in s, and a 1 c 1 + a 2 c 2 = 2 k π i . Thus, this corresponds to ξ 4 = 1 in (28). Thus, from the above discussion, we have
f ( z ) = 1 2 ( A 1 ξ + A 2 ξ 1 ) e 1 2 ( L ( z ) + H ( s ) ) ,
where L ( z ) = a 1 z 1 + a 2 z 2 and H ( s ) is a polynomial in s satisfying (28).
Thus, this completes the proof of Theorem 5 (i).
Case 2. Suppose that γ 1 ( z + c ) γ 2 ( z ) is not a constant. Since γ 1 ( z ) , γ 2 ( z ) are polynomials, by applying Lemma 4 for (23), it follows that
A 2 A 1 e γ 1 ( z ) γ 2 ( z ) 1 , o r A 2 A 1 e γ 2 ( z + c ) γ 2 ( z ) 1 .
If A 2 A 1 e γ 1 ( z ) γ 2 ( z ) 1 , it follows from (23) that A 1 A 2 e γ 1 ( z + c ) γ 2 ( z + c ) 1 . Thus, in view of (20), we have
A 2 A 1 e 2 p ( z ) 1 , A 1 A 2 e 2 p ( z + c ) 1 ,
which imply that p ( z ) is a constant and A 2 A 1 = A 1 A 2 . This leads to A 1 2 = A 2 2 , which is a contradiction with α 2 0 , 1 .
If A 2 A 1 e γ 2 ( z + c ) γ 2 ( z ) 1 , then it follows that γ 2 ( z ) is of the form γ 2 ( z ) = L 2 ( z ) + H 2 ( s ) , L 2 ( z ) = a 21 z 1 + a 22 z 2 , H 2 ( s ) is a polynomial in s, and a 21 , a 22 , c 1 , c 2 are constants satisfying
e a 21 c 1 + a 22 c 2 = A 1 A 2 .
Moreover, it follows from (23) that A 2 A 1 e γ 1 ( z ) γ 1 ( z + c ) 1 . This means that γ 1 ( z ) is of the form γ 1 ( z ) = L 1 ( z ) + H 1 ( s ) , L 1 ( z ) = a 11 z 1 + a 12 z 2 , H 1 ( s ) is a polynomial in s, and a 11 , a 12 , c 1 , c 2 are constants satisfying
e a 11 c 1 + a 12 c 2 = A 2 A 1 .
Since e γ 1 ( z + c ) γ 2 ( z ) is not a constant, it follows that L 1 ( z ) L 2 ( z ) . In view of (20), we have
e γ 1 ( z + c ) + γ 2 ( z + c ) ( γ 1 ( z ) + γ 2 ( z ) ) e g ( z + c ) g ( z ) 1 ,
which means that g ( z ) is of the form g ( z ) = L ( z ) + H ( s ) , L ( z ) = a 1 z 1 + a 2 z 2 , and
L ( z ) = L 1 ( z ) + L 2 ( z ) , H ( s ) = H 1 ( s ) + H 2 ( s ) , e a 1 c 1 + a 2 c 2 = 1 .
Substituting these into (21), we have
f ( z ) = 1 2 ( A 1 e L 1 ( z ) + H 1 ( s ) + A 2 e L 2 ( z ) + H 2 ( s ) ) .
Therefore, this completes the proof of Theorem 5. □

6. Proofs of Theorems 6 and 7

6.1. The Proof of Theorem 6

Suppose that f ( z ) is a transcendental entire solution with finite order of Equation (14). By using the same argument as in the proof of Theorem 5, we have (21) and
f ( z ) z 1 = 1 2 e γ 1 ( z ) + e γ 2 ( z ) 2 1 + α e γ 1 ( z ) e γ 2 ( z ) 2 1 α i = 1 2 ( A 2 e γ 1 ( z ) + A 1 e γ 2 ( z ) ) .
Thus, it follows from (21) and (31) that
f ( z ) z 1 = 1 2 A 1 γ 1 ( z ) z 1 e γ 1 ( z ) + A 2 γ 2 ( z ) z 1 e γ 2 ( z ) = 1 2 ( A 2 e γ 1 ( z ) + A 1 e γ 2 ( z ) ) ,
which leads to
e γ 1 ( z ) A 1 γ 1 ( z ) z 1 A 2 = e γ 2 ( z ) A 1 A 2 γ 2 ( z ) z 1 .
By combining with (20) and (32), we have
e 2 p ( z ) ( A 1 γ 1 ( z ) z 1 A 2 ) = A 1 A 2 γ 2 ( z ) z 1 .
If p ( z ) is not a constant, then it follows from (33) that
A 1 γ 1 ( z ) z 1 A 2 = 0 , A 1 A 2 γ 2 ( z ) z 1 = 0 .
Otherwise, we have
e 2 p ( z ) = A 1 γ 1 z 1 A 2 A 1 A 2 γ 2 z 1 .
Since p ( z ) , g ( z ) are polynomials, the left of Equation (34) is transcendental, but the right of Equation (34) is a polynomial. This is a contradiction. Hence, it follows that
γ 1 ( z ) = A 2 A 1 z 1 + φ 1 ( z 2 ) , γ 2 ( z ) = A 1 A 2 z 1 + φ 2 ( z 2 ) ,
where φ 1 ( z 2 ) , φ 2 ( z 2 ) are polynomials in z 2 . Thus, we have
g ( z ) = γ 1 ( z ) + γ 2 ( z ) = A 2 A 1 + A 1 A 2 z 1 + φ ( z ) = 2 α z 1 + φ ( z 2 ) ,
where φ ( z 2 ) = φ 1 ( z 2 ) + φ 2 ( z 2 ) .
If p ( z ) is a constant, then γ 1 z 1 = γ 2 z 1 = 1 2 g z 1 . Let ξ = e 2 p , in view of (33), it follows that
( 1 2 A 1 g z 1 A 2 ) ξ = ( A 1 1 2 A 2 g z 1 ) ,
which leads to
g z 1 = 2 ( A 1 + A 2 ξ ) A 1 ξ + A 2 .
Thus, we have g ( z ) = 2 ( A 1 + A 2 ξ ) A 1 ξ + A 2 z 1 + φ ( z 2 ) .
Hence, g ( z ) must be of the form g ( z ) = a 1 z 1 + φ ( z 2 ) .
Therefore, this completes the proof of Theorem 6.

6.2. The Proof of Theorem 7

Suppose that f ( z ) is a transcendental entire solution with finite order of Equation (15). Similar to the argument as in the proof of Theorem 6, we have (21) and
f ( z ) z 1 + f ( z ) z 2 = 1 2 ( A 2 e γ 1 ( z ) + A 1 e γ 2 ( z ) ) ,
where γ 1 , γ 2 are stated as in (20). Thus, it follows from (21) and (35) that
e γ 1 ( z ) A 1 γ 1 ( z ) z 1 + γ 1 ( z ) z 2 A 2 = e γ 2 ( z ) A 1 A 2 γ 2 ( z ) z 1 + γ 2 ( z ) z 2 .
By combining with (20) and (36), we have
e 2 p ( z ) A 1 γ 1 ( z ) z 1 + γ 1 ( z ) z 2 A 2 = A 1 A 2 γ 2 ( z ) z 1 + γ 2 ( z ) z 2 .
If p ( z ) is not a constant, similar to the argument as in the proof of Theorem 6, we have
A 1 γ 1 ( z ) z 1 + γ 1 ( z ) z 2 A 2 = 0 ,
A 1 A 2 γ 2 ( z ) z 1 + γ 2 ( z ) z 2 = 0 .
The characteristic equations of (38) are
d z 1 d t = 1 , d z 2 d t = 1 , d γ 1 d t = A 2 A 1 .
Using the initial conditions z 1 = 0 , z 2 = s , and γ 1 = γ 1 ( 0 , s ) : = φ 1 ( s ) with a parameter s, we obtain the following parametric representation for the solutions of the characteristic equations: z 1 = t , z 2 = t + s ,
γ 1 ( z ) = γ 1 ( t , s ) = 0 t A 2 A 1 d t + φ 1 ( s ) = A 2 A 1 t + φ 1 ( s ) = A 2 A 1 z 1 + φ 1 ( z 2 z 1 ) ,
where φ 1 ( s ) is a transcendental entire function with finite order in s. Similarly, we have
γ 2 ( z ) = A 1 A 2 z 1 + φ 2 ( z 2 z 1 ) ,
where φ 2 ( s ) is a transcendental entire function with finite order in s = z 2 z 1 . In view of (20), (40), and (41), it follows that
g ( z ) = γ 1 ( z ) + γ 2 ( z ) = 2 α z 1 + φ 1 ( z 2 z 1 ) + φ 2 ( z 2 z 1 ) = 2 α z 1 + φ ( z ) ,
where φ ( z ) = φ 1 ( z 2 z 1 ) + φ 2 ( z 2 z 1 ) .
If p ( z ) is a constant, then
γ 1 z 1 + γ 1 z 2 = γ 2 z 1 + γ 2 z 2 = 1 2 g z 1 + g z 1 .
Let ξ = e 2 p ; in view of (37), it follows that
1 2 A 1 g z 1 + g z 2 A 2 ξ = A 1 1 2 A 2 g z 1 + g z 2 ,
which leads to
g z 1 + g z 2 = 2 ( A 1 + A 2 ξ ) A 1 ξ + A 2 .
Thus, by solving the solutions of the characteristic equations of the above equation, we have g ( z ) = 2 ( A 1 + A 2 ξ ) A 1 ξ + A 2 z 1 + φ ( z 2 z 1 ) , where φ ( z 2 z 1 ) is a polynomial in z 2 z 1 .
Hence, g ( z ) must be of the form g ( z ) = a 1 z 1 + φ ( z 2 z 1 ) .
Therefore, this completes the proof of Theorem 7.

7. Proofs of Theorems 8 and 9

7.1. The Proof of Theorem 8

Suppose that f ( z ) is a transcendental entire solution with finite order of Equation (2). By using the same argument as in the proof of Theorem 5, we have (31) and
f ( z + c ) = 1 2 e γ 1 ( z ) + e γ 2 ( z ) 2 1 + α + e γ 1 ( z ) e γ 2 ( z ) 2 1 α i = 1 2 ( A 1 e γ 1 ( z ) + A 2 e γ 2 ( z ) ) ,
where γ 1 ( z ) , γ 2 ( z ) are stated as in (20) and p ( z ) is a polynomial in C 2 . In view of (31) and (42), it follows that
f ( z + c ) z 1 = 1 2 A 1 γ 1 ( z ) z 1 e γ 1 ( z ) + A 2 γ 2 ( z ) z 1 e γ 2 ( z ) = 1 2 ( A 2 e γ 1 ( z + c ) + A 1 e γ 2 ( z + c ) ) .
Thus, we have
A 1 A 2 γ 1 ( z ) z 1 e γ 1 ( z ) γ 1 ( z + c ) + γ 2 ( z ) z 1 e γ 2 ( z ) γ 1 ( z + c ) A 1 A 2 e γ 2 ( z + c ) γ 1 ( z + c ) 1 .
Now, we discuss two cases below.
Case 1. Suppose that p ( z ) is a constant; then, it follows that γ 1 ( z + c ) γ 2 ( z + c ) = 2 p ( z + c ) is a constant. Denote ξ = e p . In view of (20) and (42), it follows that
f ( z + c ) = 1 2 ( A 1 ξ + A 2 ξ 1 ) e 1 2 g ( z ) , f ( z ) z 1 = 1 2 ( A 2 ξ + A 1 ξ 1 ) e 1 2 g ( z ) .
Thus, we can deduce from (44) that
( A 2 ξ + A 1 ξ 1 ) e 1 2 ( g ( z + c ) g ( z ) ) = 1 2 ( A 1 ξ + A 2 ξ 1 ) g ( z ) z 1 .
Since g ( z ) is a polynomial in C 2 , and not of the form ϕ ( z 2 ) , it follows that g ( z ) z 1 0 . If g ( z + c ) g ( z ) is not a constant, we can deduce from (45) that A 2 ξ + A 1 ξ 1 = 0 and A 1 ξ + A 2 ξ 1 = 0 . Otherwise, we have
e 1 2 ( g ( z + c ) g ( z ) ) = 1 2 g ( z ) z 1 A 1 ξ + A 2 ξ 1 A 2 ξ + A 1 ξ 1 .
The left of Equation (46) is transcendental, but the right of Equation (46) is a polynomial. Thus, a contradiction can be obtained from (46). The fact that A 2 ξ + A 1 ξ 1 = 0 and A 1 ξ + A 2 ξ 1 = 0 can yield that A 1 2 = A 2 2 , which is a contradiction with α 2 = 1 .
Thus, it follows that g ( z + c ) g ( z ) is a constant. Then, we have g ( z ) = L ( z ) + H ( s ) , where L ( z ) is a linear form of L ( z ) = a 1 z 1 + a 2 z 2 , a 1 , a 2 are constants, and H ( s ) is a polynomial in s = c 2 z 1 c 1 z 2 . From (46), it follows that
e 1 2 ( a 1 c 1 + a 2 c 2 ) = 1 2 A 1 ξ + A 2 ξ 1 A 2 ξ + A 1 ξ 1 ( a 1 + c 2 H ) .
In view of c 2 0 , it yields that H is a constant, which means that deg s H 1 . Hence, we can conclude that L ( z ) + H ( s ) is a linear form in z 1 , z 2 . Let us still denote g ( z ) = a 1 z 1 + a 2 z 2 + b , which implies that H 0 . Thus, by combining with (44) and (47), we have
f ( z ) = 1 2 ( A 1 ξ + A 2 ξ 1 ) e 1 2 ( a 1 z 1 + a 2 z 2 + b ) 1 2 ( a 1 c 1 + a 2 c 2 ) = 2 a ( A 2 ξ + A 1 ξ 1 ) e 1 2 ( a 1 z 1 + a 2 z 2 + b ) .
Thus, in view of (47) and (48), this completes the proof of Theorem 8 (i).
Case 2. Suppose that p ( z ) is not a constant. Then, we have that γ 1 z 1 and γ 2 z 1 cannot be equal to 0 at the same time. Otherwise, it yields that γ 1 ( z + c ) γ 2 ( z + c ) is a constant, which is a contradiction. If γ 1 z 1 0 and γ 2 z 1 0 , it thus follows from (43) that
γ 2 z 1 e γ 2 ( z ) γ 1 ( z + c ) A 1 A 2 e γ 2 ( z + c ) γ 1 ( z + c ) 1 .
Obviously, γ 2 ( z ) γ 1 ( z + c ) is not a constant. Otherwise, γ 2 ( z + c ) γ 1 ( z + c ) is a constant because γ 1 , γ 2 are polynomials. By applying the Nevanlinna second fundamental theorem for e γ 2 ( z + c ) γ 1 ( z + c ) , we have from (49) that
T ( r , e γ 2 ( z + c ) γ 1 ( z + c ) ) N ( r , 1 e γ 2 ( z + c ) γ 1 ( z + c ) ) + N ( r , 1 e γ 2 ( z + c ) γ 1 ( z + c ) + A 2 A 1 ) + S ( r , e γ 2 ( z + c ) γ 1 ( z + c ) ) N ( r , 1 γ 2 z 1 e γ 2 ( z ) γ 1 ( z + c ) ) + S ( r , e γ 2 ( z + c ) γ 1 ( z + c ) ) = S ( r , e γ 2 ( z + c ) γ 1 ( z + c ) ) ,
which is a contradiction.
If γ 1 z 1 0 and γ 2 z 1 0 , using the same argument as in the above, we can get a contradiction. Hence, we have γ 1 z 1 0 and γ 2 z 1 0 . By Lemma 4, it follows that
A 1 A 2 γ 1 z 1 e γ 1 ( z ) γ 1 ( z + c ) 1 , o r γ 2 z 1 e γ 2 ( z ) γ 1 ( z + c ) 1 .
Subcase 2.1. If A 1 A 2 γ 1 z 1 e γ 1 ( z ) γ 1 ( z + c ) 1 , it yields that γ 1 ( z ) γ 1 ( z + c ) is a constant. This implies that γ 1 ( z ) is a linear form of γ 1 ( z ) = L 1 ( z ) + H 1 ( s ) , where L 1 ( z ) = a 11 z 1 + a 12 z 2 , a 11 , a 12 are constants, and H 1 ( s ) is a polynomial in s = c 2 z 1 c 1 z 2 . Thus, it follows that
A 1 A 2 ( a 11 + c 2 H 1 ) e L 1 ( c ) 1 ,
which means that c 2 H 1 is a constant. In view of c 2 0 , it yields that deg s H 1 1 . Hence, we can conclude that L 1 ( z ) + H 1 ( s ) is a linear form in z 1 , z 2 . Let us still denote γ 1 ( z ) = L 1 ( z ) + b 1 = a 11 z 1 + a 12 z 2 + b 1 , which implies that H 1 0 . Hence, we have
e L 1 ( c ) = e a 11 c 1 + a 12 c 2 = a 11 A 1 A 2 .
In addition, in view of (43), it follows
A 2 A 1 γ 2 z 1 e γ 2 ( z ) γ 2 ( z + c ) 1 .
Similarly, we have γ 2 ( z ) = L 2 ( z ) + b 2 = a 21 z 1 + a 22 z 2 + b 2 , where a 21 , a 22 , b 2 are constants satisfying
e L 2 ( c ) = e a 21 c 1 + a 22 c 2 = a 21 A 2 A 1 .
Since γ 1 ( z + c ) γ 2 ( z + c ) is not a constant, it follows that L 1 ( z ) L 2 ( z ) . In view of (20) and (42), it follows that
g ( z ) = γ 1 ( z ) + γ 2 ( z ) = ( a 11 + a 21 ) z 1 + ( a 12 + a 22 ) z 2 + b 1 + b 2 = a 1 z 1 + a 2 z 2 + b ,
and
f ( z ) = 1 2 ( A 1 e L 1 ( z ) + b 1 L 1 ( c ) + A 2 e L 2 ( z ) + b 2 L 2 ( c ) ) = 1 2 ( A 1 A 2 a 11 A 1 e a 11 z 1 + a 12 z 2 + b 1 + A 2 A 1 a 21 A 2 e a 21 z 1 + a 22 z 2 + b 2 ) = 1 2 ( A 2 a 11 e a 11 z 1 + a 12 z 2 + b 1 + A 1 a 21 e a 21 z 1 + a 22 z 2 + b 2 ) .
Subcase 2.2. If γ 2 z 1 e γ 2 ( z ) γ 1 ( z + c ) 1 , this means that γ 2 ( z ) γ 1 ( z + c ) is a constant, without loss of generalization, denote
γ 2 ( z ) γ 1 ( z + c ) = μ 1 ,
where μ 1 is a constant. In view of (43), it thus follows that γ 1 z 1 e γ 1 ( z ) γ 2 ( z + c ) 1 , this means
γ 1 ( z ) γ 2 ( z + c ) μ 2 ,
where μ 2 is a constant. In view of (53) and (54), it yields that
γ 1 ( z ) γ 2 ( z ) + γ 1 ( z + c ) γ 2 ( z + c ) = μ 2 μ 1 ,
and by combining with (20), we have
p ( z ) + p ( z + c ) = 1 2 ( μ 2 μ 1 ) ,
this is a contradiction with the assumption that γ 1 ( z + c ) γ 2 ( z + c ) = 2 p ( z + c ) is not a constant. Thus, we get the conclusions of Theorem 8 (ii) from (50)–(52).
Therefore, this completes the proof of Theorem 8.

7.2. The Proof of Theorem 9

Suppose that f ( z ) is a transcendental entire solution with finite order of Equation (3). Similar to the argument as in the proof of Theorem 8, we have (35), (42), and
A 1 A 2 ( γ 1 z 1 + γ 1 z 2 ) e γ 1 ( z ) γ 1 ( z + c ) + ( γ 2 z 1 + γ 2 z 2 ) e γ 2 ( z ) γ 1 ( z + c ) A 1 A 2 e γ 2 ( z + c ) γ 1 ( z + c ) 1 ,
where γ 1 ( z ) , γ 2 ( z ) are stated as in (20), and p ( z ) is a polynomial in C 2 .
Now, we discuss two cases below.
Case 1. Suppose that p ( z ) is a constant. In view of γ 1 ( z + c ) γ 2 ( z + c ) = 2 p ( z + c ) , it follows that γ 1 ( z + c ) γ 2 ( z + c ) is a constant. Denote ξ = e p . In view of (20) and (55), it follows that
f ( z + c ) = 1 2 ( A 1 ξ + A 2 ξ 1 ) e 1 2 g ( z ) , f ( z ) z 1 + f ( z ) z 2 = 1 2 ( A 2 ξ + A 1 ξ 1 ) e 1 2 g ( z ) .
Thus, we can deduce from (56) that
( A 2 ξ + A 1 ξ 1 ) e 1 2 ( g ( z + c ) g ( z ) ) = 1 2 ( A 1 ξ + A 2 ξ 1 ) g ( z ) z 1 + g ( z ) z 2 .
If g ( z ) z 1 + g ( z ) z 2 0 , we have g ( z ) = ϕ ( z 2 z 1 ) by solving this partial differential equation, which is a contradiction with the assumption of Theorem 9. Thus, g ( z ) z 1 + g ( z ) z 2 0 . If g ( z + c ) g ( z ) is not a constant, we can deduce from (57) that A 2 ξ + A 1 ξ 1 = 0 and A 1 ξ + A 2 ξ 1 = 0 . Otherwise, we have
e 1 2 ( g ( z + c ) g ( z ) ) = 1 2 g ( z ) z 1 + g ( z ) z 2 A 1 ξ + A 2 ξ 1 A 2 ξ + A 1 ξ 1 .
The left of Equation (58) is transcendental, but the right of Equation (58) is a polynomial. Thus, a contradiction can be obtained from (58). The fact that A 2 ξ + A 1 ξ 1 = 0 and A 1 ξ + A 2 ξ 1 = 0 can yield that A 1 2 = A 2 2 , which is a contradiction with α 2 = 1 .
Thus, it follows that g ( z + c ) g ( z ) is a constant. Then, we have g ( z ) = L ( z ) + H ( s ) , where L ( z ) is a linear form of L ( z ) = a 1 z 1 + a 2 z 2 , a 1 , a 2 are constants, and H ( s ) is a polynomial in s = c 2 z 1 c 1 z 2 . From (58), it follows that
e 1 2 ( a 1 c 1 + a 2 c 2 ) = 1 2 A 1 ξ + A 2 ξ 1 A 2 ξ + A 1 ξ 1 [ a 1 + a 2 + ( c 2 c 1 ) H ] .
In view of c 2 c 1 , it yields that H is a constant, which means that deg s H 1 . Hence, we can conclude that L ( z ) + H ( s ) is a linear form in z 1 , z 2 . Let us still denote g ( z ) = a 1 z 1 + a 2 z 2 + b , which implies that H 0 . Thus, by combining with (56) and (59), we have
f ( z ) = 1 2 ( A 1 ξ + A 2 ξ 1 ) e 1 2 ( a 1 z 1 + a 2 z 2 + b ) 1 2 ( a 1 c 1 + a 2 c 2 ) = 2 a 1 + a 2 ( A 2 ξ + A 1 ξ 1 ) e 1 2 ( a 1 z 1 + a 2 z 2 + b ) ,
and
e 1 2 ( a 1 c 1 + a 2 c 2 ) = 1 2 A 1 ξ + A 2 ξ 1 A 2 ξ + A 1 ξ 1 ( a 1 + a 2 ) .
Thus, in view of (59) and (61), this completes the proof of Theorem 9 (i).
Case 2. Suppose that p ( z ) is not a constant. Then, we have that γ 1 z 1 + γ 1 z 2 and γ 2 z 1 + γ 2 z 2 cannot be equal to 0 at the same time. Otherwise, it yields that γ 1 ( z + c ) γ 2 ( z + c ) is a constant, which is a contradiction. If γ 1 z 1 + γ 1 z 2 0 and γ 2 z 1 + γ 2 z 2 0 , it thus follows from (55) that
γ 2 z 1 + γ 2 z 2 e γ 2 ( z ) γ 1 ( z + c ) A 1 A 2 e γ 2 ( z + c ) γ 1 ( z + c ) 1 .
Obviously, γ 2 ( z ) γ 1 ( z + c ) is not a constant. Otherwise, γ 2 ( z + c ) γ 1 ( z + c ) is a constant because γ 1 , γ 2 are polynomials. By applying the Nevanlinna second fundamental theorem for e γ 2 ( z + c ) γ 1 ( z + c ) , we have from (62) that
T ( r , e γ 2 ( z + c ) γ 1 ( z + c ) ) N ( r , 1 e γ 2 ( z + c ) γ 1 ( z + c ) ) + N ( r , 1 e γ 2 ( z + c ) γ 1 ( z + c ) + A 2 A 1 ) + S ( r , e γ 2 ( z + c ) γ 1 ( z + c ) ) N ( r , 1 ( γ 2 z 1 + γ 2 z 2 ) e γ 2 ( z ) γ 1 ( z + c ) ) + S ( r , e γ 2 ( z + c ) γ 1 ( z + c ) ) = S ( r , e γ 2 ( z + c ) γ 1 ( z + c ) ) ,
which is a contradiction.
If γ 1 z 1 + γ 1 z 2 0 and γ 2 z 1 + γ 2 z 2 0 , using the same argument as in the above, we can get a contradiction. Hence, we have γ 1 z 1 + γ 1 z 2 0 and γ 2 z 1 + γ 2 z 2 0 . By Lemma 4, it follows that
A 1 A 2 γ 1 z 1 + γ 1 z 2 e γ 1 ( z ) γ 1 ( z + c ) 1 , o r γ 2 z 1 + γ 2 z 2 e γ 2 ( z ) γ 1 ( z + c ) 1 .
Subcase 2.1. If A 1 A 2 γ 1 z 1 + γ 1 z 2 e γ 1 ( z ) γ 1 ( z + c ) 1 , it yields that γ 1 ( z ) γ 1 ( z + c ) is a constant. This implies that γ 1 ( z ) is a linear form of γ 1 ( z ) = L 1 ( z ) + H 1 ( s ) , where L 1 ( z ) = a 11 z 1 + a 12 z 2 , a 11 , a 12 are constants, and H 1 ( s ) is a polynomial in s = c 2 z 1 c 1 z 2 . Thus, it follows that
A 1 A 2 a 11 + a 12 + ( c 2 c 1 ) H 1 e L 1 ( c ) 1 ,
which means that ( c 2 c 1 ) H 1 is a constant. In view of c 2 c 1 , it yields that deg s H 1 1 . Hence, we can conclude that L 1 ( z ) + H 1 ( s ) is a linear form in z 1 , z 2 . Let us still denote γ 1 ( z ) = L 1 ( z ) + b 1 = a 11 z 1 + a 12 z 2 + b 1 , which implies that H 1 0 . Hence, we have
e L 1 ( c ) = e a 11 c 1 + a 12 c 2 = ( a 11 + a 12 ) A 1 A 2 .
In addition, in view of (55), it follows
A 2 A 1 γ 2 z 1 + γ 2 z 2 e γ 2 ( z ) γ 2 ( z + c ) 1 .
Similarly, we have γ 2 ( z ) = L 2 ( z ) + b 2 = a 21 z 1 + a 22 z 2 + b 2 , where a 21 , a 22 , b 2 are constants satisfying
e L 2 ( c ) = e a 21 c 1 + a 22 c 2 = ( a 21 + a 22 ) A 2 A 1 .
Since γ 1 ( z + c ) γ 2 ( z + c ) is not a constant, it follows that L 1 ( z ) L 2 ( z ) . In view of (20) and (55), it follows that
g ( z ) = γ 1 ( z ) + γ 2 ( z ) = ( a 11 + a 21 ) z 1 + ( a 12 + a 22 ) z 2 + b 1 + b 2 = a 1 z 1 + a 2 z 2 + b ,
and
f ( z ) = 1 2 ( A 1 e L 1 ( z ) + b 1 L 1 ( c ) + A 2 e L 2 ( z ) + b 2 L 2 ( c ) ) = 1 2 ( A 2 a 11 + a 12 e a 11 z 1 + a 12 z 2 + b 1 + A 1 a 21 + a 22 e a 21 z 1 + a 22 z 2 + b 2 ) .
Subcase 2.2. If ( γ 2 z 1 + γ 2 z 2 ) e γ 2 ( z ) γ 1 ( z + c ) 1 , similar to the argument as the proof of Subcase 2.2 in Theorem 8, we have p ( z ) + p ( z + c ) = 1 2 ( μ 2 μ 1 ) , which contradicts with the assumption that γ 1 ( z + c ) γ 2 ( z + c ) = 2 p ( z + c ) is not a constant. Thus, we get the conclusions of Theorem 9 (ii) from (63)–(65).
Therefore, this completes the proof of Theorem 9.

Author Contributions

Conceptualization, H.Y.X.; writing—original draft preparation, H.Y.X. and H.L.; writing—review and editing, H.Y.X. and H.L.; and funding acquisition, H.Y.X. and H.L. All authors have read and agreed to the published version of the manuscript.

Funding

The first author is supported by the Key Project of Jiangxi Province Education Science Planning Project in China (20ZD062), the Key Project of Jiangxi Province Culture Planning Project in China (YG2018149I), the Science and Technology Research Project of Jiangxi Provincial Department of Education (GJJ181548, GJJ180767), the 2020 Annual Ganzhou Science and Technology Planning Project in China. The second author was supported by the National Natural Science Foundation of China (11561033), the Natural Science Foundation of Jiangxi Province in China (20181BAB201001) and the Foundation of Education Department of Jiangxi (GJJ190876, GJJ202303, GJJ201813, GJJ191042) of China.

Institutional Review Board Statement

Not applicable.

Informed Consent Statement

Not applicable.

Data Availability Statement

No data were used to support this study.

Acknowledgments

We thank the referee(s) for reading the manuscript very carefully and making a number of valuable and kind comments which improved the presentation.

Conflicts of Interest

The authors declare no conflict of interest.

References

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Li, H.; Xu, H. Solutions for Several Quadratic Trinomial Difference Equations and Partial Differential Difference Equations in C2. Axioms 2021, 10, 126. https://doi.org/10.3390/axioms10020126

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Li H, Xu H. Solutions for Several Quadratic Trinomial Difference Equations and Partial Differential Difference Equations in C2. Axioms. 2021; 10(2):126. https://doi.org/10.3390/axioms10020126

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Li, Hong, and Hongyan Xu. 2021. "Solutions for Several Quadratic Trinomial Difference Equations and Partial Differential Difference Equations in C2" Axioms 10, no. 2: 126. https://doi.org/10.3390/axioms10020126

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