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Article

Global Classical Solutions of the 1.5D Relativistic Vlasov–Maxwell–Chern–Simons System

1
College of Science, Zhongyuan University of Technology, Zhengzhou 450007, China
2
Section of Mathematics, International Telematic University Uninettuno, CorsoVittorio Emanuele II, 39, 00186 Roma, Italy
3
Department of Mathematics, Faculty of Science, Hadhramout University, Mukalla 50512, Yemen
4
School of Foreign Studies Zhongyuan University of Technology, Zhengzhou 450007, China
*
Author to whom correspondence should be addressed.
These authors contributed equally to this work.
Axioms 2023, 12(7), 627; https://doi.org/10.3390/axioms12070627
Submission received: 27 April 2023 / Revised: 17 June 2023 / Accepted: 18 June 2023 / Published: 25 June 2023

Abstract

:
We investigate the kinetic model of the relativistic Vlasov–Maxwell–Chern–Simons system, which originates from gauge theory. This system can be seen as an electromagnetic fields (i.e., Maxwell–Chern–Simons fields) perturbation for the classical Vlasov equation. By virtue of a nondecreasing function and an iteration method, the uniqueness and existence of the global solutions for the 1.5D case are obtained.

1. Introduction

In this paper, we focus on the relativistic Vlasov–Maxwell–Chern–Simons (RVMCS) system [1,2]
(1) t f + v ^ 1 w f + ( E 1 + v ^ 2 B , E 2 v ^ 1 B ) · v f = 0 , (2) t E 1 = E 2 j 1 , w E 1 = B + ρ , (3) t E 2 = w B + E 1 j 2 , t B = w E 2 , (4) B ( 0 , w ) = B 0 ( w ) , E ( 0 , w ) = E 0 ( w ) , f ( 0 , w , v ) = f 0 ( w , v ) ,
on the whole space ( w , v ) R × R 2 (all physical constants are normalized to unity), where at position w R and time t 0 , f ( t , w , v ) is the density of the particles, moving with velocity v = ( v 1 , v 2 ) R 2 . The functions B ( t , w ) and E ( t , w ) = ( E 1 ( t , w ) , E 2 ( t , w ) ) stand for the magnetic and electric fields by the Chern–Simons theory, respectively. In addition, the current and charge densities are defined by
j = ( v ^ f d v ) 4 π , ρ = ( f d v ) 4 π ,
where v ^ 1 , v ^ 2 , v ^ denote the relativistic velocity, respectively:
v ^ 1 = v 1 | v | 2 + 1 , v ^ 2 = v 2 | v | 2 + 1 , v ^ = v | v | 2 + 1 .
In fact, the RVMCS system is derived from gauge theory and can be described as the interaction between Vlasov matter and Maxwell–Chern–Simons fields. The Chern–Simons theory could explain many interesting phenomena, such as high- T c superconductivity [3] and the quantum Hall effect [4]. If there is no Chern–Simons term, the corresponding system is known as the relativistic Vlasov–Maxwell system, i.e., the RVM system, which has received a lot of attention in the past decades (see, e.g., Refs. [5,6,7,8,9] and the references therein).
Although a great deal of mathematical results for the Chern–Simons theory (such as [10,11]) have been established, as the authors know, there are few results for the RVMCS system. In two dimensions, [12] obtained global classical solutions for the RVMCS system and deduced that the RVMCS system converges to the Vlasov–Yukawa equations by using the similar method of [8,13]. By virtue of the moment estimate and inhomogeneous Strichartz estimates (see [14]), ref. [2] established the global existence of a classical solution for the RVMCS system without compact momentum support.
Our main interest in this paper concerns the one-and-one-half-dimensional RVMCS system. A pioneer result by Glassey and Schaeffer [6] showed the global existence of the one-and-one-half-dimensional RVM system. When considering a fixed background η ( w ) C 0 1 ( R ) which is neutralizing in the way
ρ ( 0 , w ) d w = ( f 0 ( p , v ) d v n ( p ) ) d p = 0 ,
from w E 1 = ρ , ref. [6] proved that E 1 ( t , w ) has compact support; thus, it is clear to deduce that
sup t [ 0 , T ] ,   w R | E 1 ( t , w ) | < ,
which is the key point to obtain the existence result.
However, for the RVMCS system, we could not obtain the formula of E 1 ( t , w ) directly from w E 1 = B + ρ . It is well-known that Maxwell fields can be considered as wave equations, while the Maxwell–Chern–Simons fields may be supposed to be Klein–Gordon-type equations. Therefore, we briefly review the solution of the one-dimensional Klein–Gordon equations [15]:
t t u w w u + u = g ( t , w ) , u ( 0 , w ) = u 0 ( w ) , t u ( 0 ) = u 1 0 ( w ) .
The fundamental solution of the above equations could be written as
1 2 J 0 ( t 2 | w | 2 ) ,
where J 0 is the second kind of modified Bessel function of order zero. The interested readers are referred to [16] for a more detailed discussion about Bessel functions. In the present paper, we only give the following properties and asymptotic estimate:
J n ( z ) = 2 π z c o s ( z n π 2 π 4 ) , z 1 , z n 2 n n ! , z 1 .
and
( J 0 ( z ) ) = J 1 ( z ) , ( z 1 J 1 ( z ) ) = z 1 J 2 ( z ) , J 0 ( 0 ) = 1 , J 1 ( 0 ) = 0 .
Combining function J n ( z ) and (5), one can show that
| J 0 ( z ) | , J 1 ( z ) z , J 2 ( z ) | z | 2 C .
Using the fundamental solution J 0 ( z ) , one can easily write the solution of the one-dimensional classical Klein–Gordon equation as follows:
u ( t , w ) = 1 2 ( w t w + t J 0 ( t 2 | w p | 2 ) u 1 0 ( p ) d p + t w t w + t J 0 ( t 2 | w p | 2 ) u 0 ( p ) d p ) + 1 2 0 t w ( t s ) w + ( t s ) J 0 ( | p w | 2 + ( s t ) 2 ) g ( s , p ) d s d p .
Moreover, as for the Vlasov Equation (1), similarly with the RVM system, we can denote characteristic equations:
X ˙ ( s ) = V ^ 1 ( s ) , V ˙ ( s ) = ( E 1 ( s , X ( s ) ) + V ^ 2 ( s ) B ( s , X ( s ) ) , E 2 ( s , X ( s ) ) V ^ 1 ( s ) B ( s , X ( s ) ) ) , X ( t ) = w , V ( t ) = v ,
wherein X ( s ) = X ( s , t , w , v ) , V ( s ) = V ( s , t , w , v ) . Along the characteristic curves, f ( t , w , v ) is a constant, i.e.,
f ( t , w , v ) = f 0 ( X ( 0 ) , V ( 0 ) ) .
In the rest of this paper, C shows a positive scalar that varies from line to line and only depends on the initial inputs. C ( t ) stands for a positive nondecreasing function, which may vary from line to line. For the sake of simplicity, R 2 f d v will be written as f d v . Moreover, f ( t ) and B ( t ) are, respectively, denoted by
f ( t ) = sup ( w , v ) R × R 2 { | f ( t , w , v ) | } , | B ( t ) | = sup 0 s t { B ( s ) } , B ( t ) = sup w R { | B ( t , w ) | } .
Now, we summarize the major results of this work.
Theorem 1.
Let f 0 ( w , v ) be a nonnegative C 1 function with compact support. E 0 ( w ) and B 0 ( w ) are two C 2 functions and satisfy
w E 1 0 = B 0 + f 0 ( w , v ) d v ,
and the initial data satisfy
( w , v ) α f 0 + w β E 0 + w β B 0 < , ( | α | 1 , | β | 2 ) .
Then, with the RVMCS system exists a unique global classical solution f ( t , w , v ) , ( t , w , v ) [ 0 , + ) × R × R 2 . Furthermore, f , E , B C 1 , having initial data f 0 , E 0 , B 0 satisfy
f ( t , w , v ) = 0 f o r C ( t ) | v | ,
and
( t , w , v ) α f ( t ) + ( t , w ) α E ( t ) + ( t , w ) α B ( t ) < C ( t ) , ( | α | 1 ) ,
wherein C ( t ) is a nondecreasing function.
The outline of the remainder of this work is structured as comes next. In Section 2, we give the representation of E ( t , w ) and B ( t , w ) . By view of the Bessel function and the Gronwall inequality, the derivatives of E ( t , w ) and B ( t , w ) are controlled by f . In Section 3, we obtain our main results by constructing the iteration scheme and estimating the fields more precisely.

2. Estimates of the Fields B ( t , w ) and E ( t , w )

In this section, combining the method given in [6,17] with the solution of Klein–Gordon Equation (7), we deduce the representations of E ( t , w ) and B ( t , w ) firstly.
Lemma 1.
Assume ( f , E , B ) is a classical resolution of the system RVMCS in (1)–(4). Assume that f ( t , w , v ) has compact support in ( w , v ) for each t. Then, the fields E ( t , w ) and B ( t , w ) have representations ( k = 1 , 2 ):
E k = E ˜ k 0 + E k T + E k S + E k M + E k N , B = B ˜ 0 + B T + B S + B M + B N ,
where
E ˜ 1 0 = 1 2 w t w + t J 0 ( t 2 | p + w | 2 ) t E 1 0 ( p ) d p + t w t w + t J 0 ( t 2 | p + w | 2 ) E 1 0 ( p ) d p + 2 π w t w + t J 0 ( t 2 | p + w | 2 ) ( 1 + v ^ 1 ) f 0 ( p , v ) d v d p , E ˜ 2 0 = 1 2 w t w + t J 0 ( t 2 | p + w | 2 ) t E 2 0 ( p ) d p + t w t w + t J 0 ( t 2 | p + w | 2 ) E 2 0 ( p ) d p 2 π w t w + t J 0 ( t 2 | p + w | 2 ) v ^ 1 v ^ 2 1 v ^ 1 f 0 ( p , v ) d v d p , B ˜ 0 = 1 2 w t w + t J 0 ( t 2 | p + w | 2 ) t B 0 ( p ) d p + t w t w + t J 0 ( t 2 | p + w | 2 ) B 0 ( p ) d p 2 π w t w + t J 0 ( t 2 | p + w | 2 ) v ^ 2 v ^ 1 1 f 0 ( p , v ) d v d p , E 1 S = 0 , E 2 S = B S = 2 π 0 t w ( ς + t ) w + ( ς + t ) J 0 ( ( ς + t ) 2 | p + w | 2 ) v ( v ^ 2 1 v ^ 1 ) ( F f ) ( ς , p , v ) d v d p d ς , E 1 T = 2 π 0 t w ( ς + t ) w + ( ς + t ) J 1 ( ( ς + t ) 2 | p + w | 2 ) ( ς + t ) 2 | p + w | 2 [ ( ς + t ) ( p + w ) ] ( 1 + v ^ 1 ) f ( ς , p , v ) d v d p d ς , E 2 T = 2 π 0 t w ( ς + t ) w + ( ς + t ) J 1 ( ( ς + t ) 2 | p + w | 2 ) ( ς + t ) 2 | p + w | 2 [ ( p + w ) ( ς + t ) ] v ^ 1 v ^ 2 1 v ^ 1 f ( ς , p , v ) d v d p d ς , B T = 2 π 0 t w ( ς + t ) w + ( ς + t ) J 1 ( ( ς + t ) 2 | p + w | 2 ) ( ς + t ) 2 | p + w | 2 [ ( p + w ) ( ς + t ) ] v ^ 2 1 v ^ 1 f ( ς , p , v ) d v d p d ς .
Furthermore, the others are defined by
E 1 M = 4 π 0 t ( 1 + v ^ 1 ) f ( ς , w + ( ς + t ) , v ) d v d ς , E 2 M = 4 π 0 t v ^ 1 v ^ 2 1 v ^ 1 f ( ς , w + ( ς + t ) , v ) d v d ς , B M = 4 π 0 t v ^ 2 1 v ^ 1 f ( ς , w + ( ς + t ) , v ) d v d ς , E 1 N = 2 π 0 t w ( ς + t ) w + ( ς + t ) J 0 ( ( ς + t ) 2 | w p | 2 ) v ^ 2 f ( ς , p , v ) d v d p d ς , E 2 N = 2 π 0 t w ( ς + t ) w + ( ς + t ) J 0 ( ( ς + t ) 2 | w p | 2 ) v ^ 1 f ( ς , p , v ) d v d p d ς , B N = 2 π 0 t w ( ς + t ) w + ( ς + t ) J 0 ( ( ς + t ) 2 | w p | 2 ) f ( ς , p , v ) d v d p d ς ,
where F = ( E 1 + v ^ 2 B , E 2 v ^ 1 B ) .
Proof. 
As in [6], we define two operators as comes next:
S = t + v ^ 1 w , T = t + w .
Applying the calculations of [7,8,17], we can rewrite time and spatial derivatives below:
t = S v ^ 1 T 1 v ^ 1 , w = T S 1 v ^ 1 .
From (2) and (3), we obtain that
t t E 1 w w E 1 + E 1 = w ρ + j 2 t j 1 , t t E 2 w w E 2 + E 2 = j 1 t j 2 , t t B w w B + B = ρ + w j 2 .
Because of the calculation process of the representation of E 1 , E 2 and B are almost similar, we just only calculate E 2 .
Actually, using (7), the E 2 field could be written as follows:
E 2 = 1 2 ( t w t w + t J 0 ( t 2 | p + w | 2 ) E 2 0 ( p ) d p + w t w + t J 0 ( t 2 | p + w | 2 ) t E 2 0 ( p ) d p ) + E ˜ 2 ,
where
E ˜ 2 = 1 2 0 t w ( ς + t ) w + ( ς + t ) J 0 ( ( ς + t ) 2 | w p | 2 ) ( j 1 ς j 2 ) ( ς , p ) d p d ς ,
and in view of (9), E ˜ 2 can be rewritten as
E ˜ 2 = 0 t w ( ς + t ) w + ( ς + t ) J 0 ( ( ς + t ) 2 | p + w | 2 ) ( 2 π v ^ 1 f ) ( ς , p , v ) d v d p d ς + 0 t w ( ς + t ) w + ( ς + t ) J 0 ( ( ς + t ) 2 | p + w | 2 ) ( 2 π v ^ 2 ς f ) ( ς , p , v ) d v d p d ς = E 2 N 2 π 0 t w ( ς + t ) w + ( ς + t ) J 0 ( ( ς + t ) 2 | p + w | 2 ) v ^ 2 ( S v ^ 1 T 1 v ^ 1 ) f ( ς , p , v ) d v d p d ς = E 2 N 2 π 0 t w ( ς + t ) w + ( ς + t ) J 0 ( ( ς + t ) 2 | p + w | 2 ) v ^ 2 1 v ^ 1 S f ( ς , p , v ) d v d p d ς + 2 π 0 t w ( ς + t ) w + ( ς + t ) J 0 ( ( ς + t ) 2 | p + w | 2 ) v ^ 1 v ^ 2 1 v ^ 1 T f ( ς , p , v ) d v d p d ς = E 2 N + E ˜ 2 S + E ˜ 2 T .
By virtue of (1), we obtain
S f = F · v f = v ( F f ) .
It is now deduced that
E ˜ 2 S = 2 π 0 t w ( ς + t ) w + ( ς + t ) J 0 ( ( ς + t ) 2 | p + w | 2 ) v ^ 2 1 v ^ 1 v ( F f ) ( ς , p , v ) d v d p d ς = 2 π 0 t w ( ς + t ) w + ( ς + t ) J 0 ( ( ς + t ) 2 | p + w | 2 ) v ( v ^ 2 1 v ^ 1 ) ( F f ) ( ς , p , v ) d v d p d ς = E 2 S .
For the E ˜ 2 T term, using the definition of T , we obtain
E ˜ 2 T = 2 π 0 t w ( ς + t ) w + ( ς + t ) J 0 ( ( ς t ) 2 | p + w | 2 ) v ^ 1 v ^ 2 1 v ^ 1 ( ς + p ) f ( ς , p , v ) d v d p d ς .
Set ε ( 0 , 1 ) , by invoking integration by parts and (5), and we obtain
0 t w ( 1 ε ) ( ς + t ) w + ( 1 ε ) ( ς + t ) J 0 ( ( ς + t ) 2 | w p | 2 ) ( ς + p ) f ( ς , p , v ) d v d p d ς = 0 t w ( 1 ε ) ( ς + t ) w + ( 1 ε ) ( ς + t ) J 1 ( ( ς + t ) 2 | w p | 2 ) ( ς + t ) 2 | w p | 2 [ ( w p ) ( ς + t ) ] f ( ς , p , v ) d v d p d ς + 0 t d d ς w ( 1 ε ) ( ς + t ) w + ( 1 ε ) ( ς + t ) J 0 ( ( ς + t ) 2 | w p | 2 ) f d p d ς + ( 2 ε ) 0 t J 0 ( ε ( 2 ε ) ( ς + t ) ) f ( ς , w + ( 1 ε ) ( ς + t ) , v ) d v d ς ε 0 t J 0 ( ε ( 2 ε ) ( ς + t ) ) f ( ς , w ( 1 ε ) ( ς + t ) , v ) d v d ς .
As ε 0 , it is easy to deduce that
E ˜ 2 T = 2 π w t w + t J 0 ( t 2 | p + w | 2 ) v ^ 1 v ^ 2 1 v ^ 1 f 0 ( p , v ) d v d p + E 2 T + E 2 M .
Inserting inequalities (11)–(14) into (10), we obtain the representation of E 2 . □
Remark 1.
Because of the different fundamental function between the Klein–Gordon equations with wave equations, the representations of fields E and B for the RVMCS system have some different points from the RVM system [6]. For example, we have additional terms E k S , E k T , B S and B T . Nevertheless, these additional terms can be controlled by (5) and (6).
Now, we are devoted to estimating the fields E ( t , w ) and B ( t , w ) .
Lemma 2.
Suppose that ( f ( t , w , v ) , E ( t , w ) , B ( t , w ) ) satisfy the same conditions as in Lemma 1 and
f 0 , E 0 , B 0 , w E 0 , w B 0
are finite. If there is a nondecreasing function C ( t ) yielding
f ( t , w , v ) = 0 i f C ( t ) | v | ,
then
| B ( t ) | + | E ( t ) | C ( t ) .
Proof. 
Because of | v | < C ( t ) when f 0 , it is easy to show that
(15) v ^ 1 v ^ 2 1 v ^ 1 v 1 v ^ 2 | v | 2 + 1 v 1 = v 1 v ^ 2 ( | v | 2 + 1 + v 1 ) 1 + | v 2 | 2 2 | v 2 | 1 + | v | 2 C ( t ) , (16) v 1 ( v ^ 2 1 v ^ 1 ) = v 1 v 2 1 + | v 2 | 2 ( 1 + | v | 2 + v 1 ) = v 2 ( v ^ 1 + 1 ) | v 2 | 2 + 1 2 , (17) v 2 ( v ^ 2 1 v ^ 1 ) = 1 + | v 1 | 2 ( 1 + | v | 2 ) 3 2 ( 1 v ^ 1 ) v ^ 1 | v ^ 2 | 2 ( 1 v ^ 1 ) 2 | v | 2 + 1 1 + | v | 2 + 2 | v 1 | C ( t ) ,
where we have used 1 + | v | 2 v 1 v ^ 2 . Hence, for 0 t T , using (6) and in consideration of Lemma 1, we obtain that
E ( t ) + B ( t ) C ( t ) + C ( t ) 0 t ( E ( ς ) + B ( ς ) ) d ς C ( T ) + C ( T ) 0 t ( E ( ς ) + B ( ς ) ) d ς .
The Gronwall’s inequality implies that E ( t ) + B ( t ) C ( T ) , for 0 t T . This is the desired result. □
Next, we show that the derivatives of the fields are also bounded.
Lemma 3.
Assume that ( f , E , B ) are as in Lemma 1, and ( w , v ) f 0 , w 2 E 0 and w 2 B 0 are finite. Then,
| w B ( t ) | + | w E ( t ) | C ( t ) ( 1 + | w f ( t ) | ) .
Proof. 
Firstly, we calculate every term of w E 2 . For w E 2 S , using the definition of operators S and T, together with (1) and (9), we have
w E 2 S = 2 π 0 t w ( ς + t ) w + ( ς + t ) J 0 ( ( ς + t ) 2 | p + w | 2 ) v ( v ^ 2 1 v ^ 1 ) p ( F f ) ( ς , p , v ) d v d p d ς = 2 π 0 t w ( ς + t ) w + ( ς + t ) J 0 ( ( ς + t ) 2 | p + w | 2 ) v v ( v ^ 2 1 v ^ 1 ) · F 1 v ^ 1 · F f d v d p d ς + 2 π 0 t w ( ς + t ) w + ( ς + t ) J 0 ( ( ς + t ) 2 | p + w | 2 ) v ( v ^ 2 1 v ^ 1 ) · F T f 1 v ^ 1 d v d p d ς + 2 π 0 t w ( ς + t ) w + ( ς + t ) J 0 ( ( ς + t ) 2 | p + w | 2 ) v ( v ^ 2 1 v ^ 1 ) · p F · f d v d p d ς = w E 2 S 1 + w E 2 S 2 + w E 2 S 3 .
On the set { v : | v | < C ( t ) } , by an elementary computation as well as Lemma 1, this yields that
v v ( v ^ 2 1 v ^ 1 ) · F 1 v ^ 1 · F f C ( t ) .
Consequently, we obtain
| w E 2 S 1 | C ( t ) 0 t w ( ς + t ) w + ( ς + t ) J 0 ( ( ς + t ) 2 | p + w | 2 ) d p d ς C ( t ) .
Similar to the estimate of (13), we have
w E 2 S 2 = 2 π 0 t w ( ς + t ) w + ( ς + t ) ς ( J 0 ( ( ς + t ) 2 | p + w | 2 ) F ) v ( v ^ 2 1 v ^ 1 ) f 1 v ^ 1 d v d p d ς + 2 π 0 t w ( ς + t ) w + ( ς + t ) p ( J 0 ( ( ς + t ) 2 | p + w | 2 ) F ) v ( v ^ 2 1 v ^ 1 ) f 1 v ^ 1 d v d p d ς + 2 π w t w + t J 0 ( t 2 | p + w | 2 ) 1 v ^ 1 v ( v ^ 2 1 v ^ 1 ) · ( F f ) | ς = 0 d v d p + 4 π 0 t v ( v ^ 2 1 v ^ 1 ) · F f 1 v ^ 1 | ( ς , w + ( ς + t ) , v ) d v d ς .
By (2) and (3) and Lemma 1, for 0 ς t , we have
| ς F | C ( t ) + w E ( ς ) + w B ( ς ) .
Then, combining the properties of Bessel functions (5) and (6) with the support of f, we observe that
| w E 2 S 2 | C ( t ) 1 + 0 t ( w E ( ς ) + w B ( ς ) ) d ς .
Similarly, we have
| w E 2 S 3 | C ( t ) 0 t ( w E ( ς ) + w B ( ς ) ) d ς .
Finally, by virtue of the above inequality and (18)–(20), we obtain
| w E 2 S | C ( t ) 1 + 0 t ( w E ( ς ) + w B ( ς ) ) d ς .
Next, using equality (9), we can estimate w E 2 T ,
w E 2 T = 2 π 0 t w ( ς + t ) w + ( ς + t ) J 1 ( ( ς + t ) 2 | p + w | 2 ) ( ς + t ) 2 | p + w | 2 [ ( p + w ) ( ς + t ) ] v ^ 1 v ^ 2 1 v ^ 1 p f ( ς , p , v ) d v d p d ς = 2 π 0 t w ( ς + t ) w + ( ς + t ) J 1 ( ( ς + t ) 2 | p + w | 2 ) ( ς + t ) 2 | p + w | 2 [ ( p + w ) ( ς + t ) ] v ^ 1 v ^ 2 ( 1 v ^ 1 ) 2 S   f d v d p d ς + 2 π 0 t w ( ς + t ) w + ( ς + t ) J 1 ( ( ς + t ) 2 | p + w | 2 ) ( ς + t ) 2 | p + w | 2 [ ( p + w ) ( ς + t ) ] v ^ 1 v ^ 2 ( 1 v ^ 1 ) 2 T   f d v d p d ς , = w E 2 T S + w E 2 T T .
Then, we estimate each term in the above equality separately. For w E 2 T S , using (1), Lemma 2 and | v | C ( t ) , we show that
| w E 2 T S | 2 π 0 t w ( ς + t ) w + ( ς + t ) | ( p + w ) ( ς + t ) | v v ^ 1 v ^ 2 ( 1 v ^ 1 ) 2 · F f d v d p d ς C ( t ) 0 t w ( ς + t ) w + ( ς + t ) ( ς + t ) d p d ς C ( t ) .
For w E 2 T T , similar to the estimate of (13), in view of (5), (6) and (9), we have
| w E 2 T T | 2 π 0 t w ( ς + t ) w + ( ς + t ) | J 2 ( ( ς + t ) 2 | p + w | 2 ) ( ς + t ) 2 | p + w | 2 [ ( p + w ) ( ς + t ) ] 2 v ^ 1 v ^ 2 ( 1 v ^ 1 ) 2 f | d v d p + w t w + t | J 1 ( t 2 | p + w | 2 ) t 2 | p + w | 2 ( t ( p + w ) ) v ^ 1 v ^ 2 ( 1 v ^ 1 ) 2 f 0 d v d p | C ( t ) | 0 t w ( ς + t ) w + ( ς + t ) ( ς + t ) 2 d p d ς + w t w + t ( t ( p + w ) ) d p | C ( t ) .
Hence, combining the above estimate, we obtain | w E 2 T | C ( t ) .
For w E 2 M , we could compute it directly:
| w E 2 M | 4 π | w f ( t ) | 0 t v ^ 1 v ^ 2 1 v ^ 1 d v d ς C ( t ) | w f ( t ) | .
Then, for w E 2 N , similar to the estimates of w E 2 T , it is easy to show
| w E 2 N | C ( t ) .
Lastly, for w E ˜ 2 0 , we can obtain | w E ˜ 2 0 | C ( t ) by integration by parts. Thus, from the above estimates and Lemma 1, we have
| w E 2 | C ( t ) 1 + | w f ( t ) | + 0 t ( w E ( ς ) + w B ( ς ) ) d ς .
Again, in the same way, we can estimate w E 1 and w B . Consequently, for 0 t T , we have
| w E | + | w B | C ( t ) 1 + | w f ( t ) | + 0 t ( w E ( ς ) + w B ( ς ) ) d ς C ( T ) 1 + | w f ( T ) | + 0 t ( w E ( ς ) + w B ( ς ) ) d ς
This, together with Gronwall’s inequality, completes the proof. □
Lemma 4.
Assume that ( f ( t , w , v ) , E ( t , w ) , B ( t , w ) ) are as in Lemmas 1–3 and the conditions of Lemmas 1–3 hold. Then,
f ( t ) + E ( t ) + B ( t ) + ( w , v ) f ( t ) + w E ( t ) + w B ( t ) C ( t ) .
Proof. 
It is similar to [7] (Theorem 4) and [12] (Lemma 3.2), so we omit it. □

3. Proof of the Main Results

This section is furnished to investigate the existence and uniqueness of classical solutions for the RVMCS system. First of all, we will give a conditional existence proposition.
Proposition 1.
Let f 0 ( w , v ) be nonnegative C 1 functions. Suppose that E 0 ( w ) and B 0 ( w ) are two C 2 functions, such that
w E 1 0 = B 0 + 4 π f 0 ( w , v ) d v .
If the data satisfy
( w , v ) α f 0 + w β E 0 + w β B 0 < , ( | α | 1 , | β | 2 ) ,
and furthermore, if there is a non-decreasing function C ( t ) such that
f ( t , w , v ) = 0 f o r | v | C ( t ) .
Then, there exists a unique C 1 global classical solution for the RVMCS system.
Proof. 
In this work, we use a well-known iteration scheme method ([6,7,12,17,18]) which may be well used to prove the existence theorem. Denote f ( n ) ( t , w , v ) , E ( n ) ( t , w ) , B ( n ) ( t , w ) the iteration functions. We also take smooth initial data
f ( 0 ) ( t , w , v ) = f 0 ( w , v ) C 2 , E ( 0 ) ( t , w ) = E 0 ( w ) C 3 , B ( 0 ) ( t , w ) = B 0 ( w ) C 3 .
After the ( n 1 ) s t iteration, we set that f ( n ) is the solution of the following Vlasov problem:
t f ( n ) + v ^ 1 w f ( n ) + ( E 1 ( n 1 ) + v ^ 2 B ( n 1 ) , E 2 ( n 1 ) v ^ 1 B ( n 1 ) ) · v f ( n ) = 0 .
Hence, f ( n ) is a C 2 function if E ( n 1 ) and B ( n 1 ) are C 2 functions. By the theory of ordinary differential equations, along the characteristics equations in (21)
w ˙ = v ^ 1 , v ˙ = ( E 1 ( n 1 ) + v ^ 2 B ( n 1 ) , E 2 ( n 1 ) v ^ 1 B ( n 1 ) )
f ( n ) ( t , w , v ) is a constant. Therefore, f ( n ) ( t , w , v ) also has compact support in v. In addition,
ρ ( n ) ( t , w ) = 4 π f ( n ) ( t , w , v ) d v C 2 , j ( n ) ( t , w ) = 4 π v ^ f ( n ) ( t , w , v ) d v C 2
are well-defined. Then, we obtain E ( n ) and B ( n ) by solving the following equations
t t E 1 ( n ) w w E 1 ( n ) + E 1 ( n ) = w ρ ( n ) + j 2 ( n ) t j 1 ( n ) , t t E 2 ( n ) w w E 2 ( n ) + E 2 ( n ) = j 1 ( n ) t j 2 ( n ) , t t B ( n ) w w B ( n ) + B ( n ) = ρ ( n ) + w j 2 ( n )
with initial data E 0 ( w ) , B 0 ( w ) . Furthermore, with Lemma 4, we can prove easily that these sequences are Cauchy in the C 1 -norm and obtain the existence from Proposition 1 as in [17]. □
To prove Theorem 1, we will show that the nondecreasing function in Proposition 1 exists on [ 0 , ) . To this end, we establish a lemma for energy conservation.
Lemma 5.
Suppose ( f ( t , w , v ) , E ( t , w ) , B ( t , w ) ) are the solutions stated in Proposition 1. Then, the energy identity
t e + w 4 π v 1 f d v + E 2 B = 0
holds, where
e = 4 π 1 + | v | 2 f d v + 1 2 | E | 2 + 1 2 | B | 2 .
Moreover,
(23) w ( ς + t ) w + ( ς + t ) e ( ς , p ) d p C , (24) sup | w | < C + t ,   0 < t < T 0 t | v 2 | 1 + | v | 2 f ( ς , w + ( ς + t ) , v ) d v d ς C , (25) sup | w | < C + t w ( ς + t ) w + ( ς + t ) ρ 3 2 ( ς , p ) d p C ( ς + t ) , (26) sup | w | < C + t w ( ς + t ) w + ( ς + t ) f 1 + | v | 2 d v 3 d p C ( ς + t ) .
Proof. 
The energy identity (22) is similar to [12] (Lemma 3.3), and its certification process is omitted (see [12] for details). It is obvious that f ( t , w , v ) = 0 if | w | C + t because of w ˙ = v ^ and | v ^ |   < 1 . So, we have the total energy identity by (22), i.e., (23). Similar with [8] (Lemma 1), we can obtain (24).
To prove (25), note that for each R > 0 , we use the usual manner,
ρ | v | R f d v + | v | > R f d v C ( R 2 + e R ) .
Taking R = e 1 / 3 , we have ρ 3 / 2 C e and hence
sup w R w ( ς + t ) w + ( ς + t ) ρ 3 2 ( ς , p ) d p C ( ς + t ) .
Similarly, we can prove (26). □
Next, our goal is to deduce that P ( t ) C ( t ) where
P ( t ) = 1 + sup { | v | : f ( ς , w , v ) 0 f o r s o m e ( ς , w ) [ 0 , t ] × R } .
As the similar method in [6,7,8,12], by virtue of the estimate of P ( t ) , Proposition 1 can be extended to Theorem 1.
To this end, following from Lemma 5, we give more precise estimates of the fields than Lemma 2.
Lemma 6.
Let ( f , E , B ) be the solution furnished in Proposition 1, 0 < T ˜ < T , and then the estimate
E ( t ) + B ( t ) C ( T ˜ ) ( 1 + P 2 ( T ˜ ) )
holds for t [ 0 , T ˜ ] .
Proof. 
Combining (16) with (17), we obtain
F · v ( v ^ 2 1 v ^ 1 ) C ( | E | + | B | ) ( 1 + ( 1 + | v | 2 ) 1 2 ) .
Then, using (6) and (15) and Lemma 1, we obtain
E ( t ) + B ( t ) C ( t ) + C ( 0 t w ( ς + t ) w + ( ς + t ) ( | E | + | B | ) ( 1 + | v | 2 ) 1 2 f d v d p d ς + 0 t w ( ς + t ) w + ( ς + t ) ρ d p d ς + 0 t w ( ς + t ) w + ( ς + t ) ( | E | + | B | )   f d v d p d ς + 0 t w ( ς + t ) w + ( ς + t ) 1 + | v | 2 f d v d p d ς + 0 t | v 2 | 1 + | v | 2 f ( ς , w + ( ς + t ) , v ) d v d ς ) C ( t ) + I 1 + I 2 + I 3 + I 4 + I 5 .
Then, we calculate I i ( 1 i 5 ) , respectively. For I 1 , using the Hölder inequality, (22) and (26), we have
| I 1   | C ( 1 + P 2 ( T ˜ ) ) 0 t w ( ς + t ) w + ( ς + t ) ( | E | + | B | ) 2 d p 1 2 w ( ς + t ) w + ( ς + t ) f 1 + | v | 2 d v 2 d p 1 2 d ς C ( T ˜ ) ( 1 + P 2 ( T ˜ ) ) 0 t w ( ς + t ) w + ( ς + t ) f 1 + | v | 2 d v 3 d p 1 3 w ( ς + t ) w + ( ς + t ) d p 1 6 d ς C ( T ˜ ) ( P 2 ( T ˜ ) + 1 ) 0 t ( ς + t ) 1 2 d ς C ( T ˜ ) ( P 2 ( T ˜ ) + 1 ) .
By (25) and the Hölder inequality again, it gives that
| I 2 | C 0 t w ( ς + t ) w + ( ς + t ) ρ 3 2 d p 2 3 w ( ς + t ) w + ( ς + t ) d p 1 3 d ς C 0 t ( ς + t ) d ς C T ˜ 2 .
With the above inequality, it is easy to deduce that
| I 3 | C 0 t ( E ( ς ) + B ( ς ) ) w ( ς + t ) w + ( ς + t ) ρ d p d ς C 0 t ( ς + t ) ( E ( ς ) + B ( ς ) ) d ς C T ˜ 0 t ( E ( ς ) + B ( ς ) ) d ς .
Similar to the estimate of I 1 , we also obtain
| I 4 | C ( T ˜ ) ( 1 + P 2 ( T ˜ ) ) .
For I 5 , by (24), it yields that
| I 5 | C ( 1 + P 2 ( T ˜ ) ) .
Combining the above inequalities with (27), we obtain
E ( t ) + B ( t ) C ( T ˜ ) ( 1 + P 2 ( T ˜ ) ) + C T ˜ 0 t ( E ( ς ) + B ( ς ) ) d ς .
Thus, by the inequality of the Gronwall, it implies that
E ( t ) + B ( t ) C ( T ˜ ) ( 1 + P 2 ( T ˜ ) ) exp { C T ˜ t } C ( T ˜ ) ( 1 + P 2 ( T ˜ ) ) .
Employing the characteristic curves (8) and Lemma 6, we have
| V ( 0 , t , w , v ) | | v | + C 0 t ( E ( ς ) + B ( ς ) ) d ς C + 0 t C ( ς ) ( 1 + P 2 ( ς ) ) d ς .
It follows that
P ( t ) C + C ( t ) 0 t ( 1 + P 2 ( ς ) ) 2 d ς C + C ( T ˜ ) 0 t ( 1 + P 2 ( ς ) ) d ς ,
wherein P ( t ) is bounded via Q ( t ) on [ 0 , T ] , and also Q ( t ) satisfies
Q ( t ) = tan ( C ( T ˜ ) t + arctan C ) .
So, choosing t = T ˜ , for each T ˜ ( 0 , T ) , one obtains
P ( T ˜ ) tan ( C ( T ˜ ) T ˜ + arctan C ) = C ( T ˜ ) .
This completes the proof of the theorem.

4. Conclusions

In this manuscript, we have considered the relativistic Vlasov–Maxwell–Chern–Simons system in the 1.5D case. Different from the well-known Vlasov–Maxwell equations, the RVMCS system could be seen as a set of the Klein–Gordon-type equations and Vlasov equation. However, the Vlasov–Maxwell system could be considered as a system of the linear wave equation. The fundamental solution of the one-dimensional Klein–Gordon PDE has some decaying and bounded properties; hence, we can control B ( t , w ) and E ( t , w ) . By view of the iteration method and a nondecreasing function condition, we establish the global uniqueness and existence of the RVMCS system. In a forthcoming work, inspired by the work of [19,20,21,22,23], we may study two questions. On the one hand, we will consider establishing the well-posedness of the RVMCS system in Besov space with large Maxwell fields. On the other hand, we will consider the behavior of the RVMCS system, when the speed of light tends to infinity.

Author Contributions

Conceptualization, J.C.; data curation, O.B.; funding acquisition, J.C.; Soft- ware, Y.S.; writing—original draft preparation, J.C. and C.L.; writing—review and editing, J.C. and O.B. All authors have read and agreed to the published version of the manuscript.

Funding

This work was supported by the Training Plan for Young Teachers in Colleges and Universities of Henan Province (Grant No. 2020GGJS142) and the Natural Science Foundation of Zhongyuan University of Technology (No. K2023MS001).

Data Availability Statement

Not applicable.

Acknowledgments

The authors would like to thank reviewers and the editor for valuable comments for improving the original manuscript.

Conflicts of Interest

The authors declare no conflict of interest.

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Chen, J.; Bazighifan, O.; Luo, C.; Song, Y. Global Classical Solutions of the 1.5D Relativistic Vlasov–Maxwell–Chern–Simons System. Axioms 2023, 12, 627. https://doi.org/10.3390/axioms12070627

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Chen J, Bazighifan O, Luo C, Song Y. Global Classical Solutions of the 1.5D Relativistic Vlasov–Maxwell–Chern–Simons System. Axioms. 2023; 12(7):627. https://doi.org/10.3390/axioms12070627

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Chen, Jing, Omar Bazighifan, Chengjun Luo, and Yanlai Song. 2023. "Global Classical Solutions of the 1.5D Relativistic Vlasov–Maxwell–Chern–Simons System" Axioms 12, no. 7: 627. https://doi.org/10.3390/axioms12070627

APA Style

Chen, J., Bazighifan, O., Luo, C., & Song, Y. (2023). Global Classical Solutions of the 1.5D Relativistic Vlasov–Maxwell–Chern–Simons System. Axioms, 12(7), 627. https://doi.org/10.3390/axioms12070627

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