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Article

Total Roman {3}-domination in Graphs

1
Institute of Computing Science and Technology, Guangzhou University, Guangzhou 510006, China
2
Department of Mathematics, University of Mazandaran, Babolsar 47416-95447, Iran
3
Lehrstuhl II für Mathematik, RWTH Aachen University, 52056 Aachen, Germany
*
Author to whom correspondence should be addressed.
Symmetry 2020, 12(2), 268; https://doi.org/10.3390/sym12020268
Submission received: 4 January 2020 / Revised: 2 February 2020 / Accepted: 3 February 2020 / Published: 9 February 2020

Abstract

:
For a graph G = ( V , E ) with vertex set V = V ( G ) and edge set E = E ( G ) , a Roman { 3 } -dominating function (R { 3 } -DF) is a function f : V ( G ) { 0 , 1 , 2 , 3 } having the property that u N G ( v ) f ( u ) 3 , if f ( v ) = 0 , and u N G ( v ) f ( u ) 2 , if f ( v ) = 1 for any vertex v V ( G ) . The weight of a Roman { 3 } -dominating function f is the sum f ( V ) = v V ( G ) f ( v ) and the minimum weight of a Roman { 3 } -dominating function on G is the Roman { 3 } -domination number of G, denoted by γ { R 3 } ( G ) . Let G be a graph with no isolated vertices. The total Roman { 3 } -dominating function on G is an R { 3 } -DF f on G with the additional property that every vertex v V with f ( v ) 0 has a neighbor w with f ( w ) 0 . The minimum weight of a total Roman { 3 } -dominating function on G, is called the total Roman { 3 } -domination number denoted by γ t { R 3 } ( G ) . We initiate the study of total Roman { 3 } -domination and show its relationship to other domination parameters. We present an upper bound on the total Roman { 3 } -domination number of a connected graph G in terms of the order of G and characterize the graphs attaining this bound. Finally, we investigate the complexity of total Roman { 3 } -domination for bipartite graphs.

1. Introduction

In this paper, we introduce and study a variant of Roman dominating functions, namely, total Roman { 3 } -dominating functions. First we present some necessary terminology and notation. Let G = ( V , E ) be a graph of order n with vertex set V = V ( G ) and edge set E = E ( G ) . The open neighborhood of a vertex v V ( G ) is the set N G ( v ) = N ( v ) = { u : u v E ( G ) } . The closed neighborhood of a vertex v V ( G ) is N G [ v ] = N [ v ] = N ( v ) { v } . The open neighborhood of a set S V is the set N G ( S ) = N ( S ) = v S N ( v ) . The closed neighborhood of a set S V is the set N G [ S ] = N [ S ] = N ( S ) S = v S N [ v ] . We denote the degree of v by d G ( v ) = d ( v ) = | N ( v ) | . By Δ = Δ ( G ) and δ = δ ( G ) , we denote the maximum degree and minimum degree of a graph G, respectively. A vertex of degree one is called a leaf and its neighbor a support vertex. We denote the set of leaves and support vertices of a graph G by L ( G ) and S ( G ) , respectively. We write K n , P n and C n for the complete graph, path and cycle of order n, respectively. A tree T is an acyclic connected graph. The corona H K 1 of a graph H is the graph constructed from H, where for each vertex v V ( H ) , a new vertex v and a pendant edge v v are added. The union of two graphs G 1 and G 2 ( G 1 G 2 ) is a graph G such that V ( G ) = V ( G 1 ) V ( G 2 ) and E ( G ) = E ( G 1 ) E ( G 2 ) .
A set S V in a graph G is called a dominating set if N [ S ] = V . The domination number γ ( G ) of G is the minimum cardinality of a dominating set in G, and a dominating set of G of cardinality γ ( G ) is called a γ -set of G, [1]. A set S V in a graph G is called a total dominating set if N ( S ) = V . The total domination number γ t ( G ) of G is the minimum cardinality of a total dominating set in G, and a total dominating set of G of cardinality γ t ( G ) is called a γ t -set of G, [2].
Given a graph G and a positive integer m, assume that g : V ( G ) { 0 , 1 , 2 , , m } is a function, and suppose that ( V 0 , V 1 , V 2 , , V m ) is the ordered partition of V induced by g, where V i = { v V : g ( v ) = i } for i { 0 , 1 , , m } . So we can write g = ( V 0 , V 1 , V 2 , , V m ) . A Roman dominating function on graph G is a function f : V { 0 , 1 , 2 } such that if v V 0 for some v V , then there exists a vertex w N ( v ) such that w V 2 . The weight of a Roman dominating function (RDF) is the sum w f = v V ( G ) f ( v ) , and the minimum weight of w f for every Roman dominating function f on G is called the Roman domination number of G, denoted by γ R ( G ) , see also [3].
Let G be a graph with no isolated vertices. The total Roman dominating function (TRDF) on G, is an RDF f on G with the additional property that every vertex v V with f ( v ) 0 has a neighbor w with f ( w ) 0 . The minimum weight of any TRDF on G is called the total Roman domination number of G denoted by γ t R ( G ) . A TRDF on G with weight γ t R ( G ) is called a γ t R ( G ) -function.
The mathematical concept of Roman domination, is originally defined and discussed by Stewart [4] in 1999, and ReVelle and Rosing [5] in 2000. Recently, Chellali et al. [6] have introduced the Roman { 2 } -dominating function f as follows. A Roman { 2 } -dominating function is a function f : V { 0 , 1 , 2 } such that for every vertex v V , with f ( v ) = 0 , f ( N ( v ) ) 2 where f ( N ( v ) ) = x N ( v ) f ( x ) , that is, either v has a neighbor u with f ( u ) = 2 , or has two neighbors x , y with f ( x ) = f ( y ) = 1 [7].
In terms of the Roman Empire, this defense strategy requires that every location with no legion has a neighboring location with two legions, or at least two neighboring locations with one legion each.
Note that for a Roman { 2 } -dominating function (R { 2 } -DF) f, and for some vertex v with f ( v ) = 1 , it is possible that f ( N ( v ) ) = 0 . The sum w f = v V ( G ) f ( v ) is denoted the weight of a Roman { 2 } -dominating function, and the minimum weight of a Roman { 2 } -dominating function f is the Roman { 2 } -domination number, denoted by γ { R 2 } ( G ) . Roman { 2 } -domination is a generalization of Roman domination that has also studied by Henning and Klostermeyer [8] with the name Italian domination.
The total Roman { 2 } -domination for graphs are defined as follows [9]. Let G be a graph without isolated vertices. Then f : V { 0 , 1 , 2 } is total Roman { 2 } -dominating function (TR { 2 } -DF) if it is a Roman { 2 } -dominating function and the subgraph induced by the positive weight vertices has no isolated vertex. The minimum weight w f = v V ( G ) f ( v ) of a any total Roman { 2 } -dominating function of a graph G is called the total Roman { 2 } -domination number of G and is denoted by γ t { R 2 } ( G ) . Beeler et al. [10] have defined double Roman domination.
A double Roman dominating function (DRDF) on a graph G is a function f : V { 0 , 1 , 2 , 3 } such that the following conditions are hold:
(a)
if f ( v ) = 0 , then the vertex v must have at least two neighbors in V 2 or one neighbor in V 3 .
(b)
if f ( v ) = 1 , then the vertex v must have at least one neighbor in V 2 V 3 .
The weight of a double Roman dominating function is the sum w f = v V ( G ) f ( v ) , and the minimum weight of w f for every double Roman dominating function f on G is called the double Roman domination number of G. We denote this number with γ d R ( G ) and a double Roman dominating function of G with weight γ d R ( G ) is called a γ d R ( G ) -function of G, see also [11].
Hao et al. [12] have recently defined total double Roman domination. The total double Roman dominating function (TDRDF) on a graph G with no isolated vertex is a DRDF f on G with the additional property that the subgraph of G induced by the set { v V ( G ) : f ( v ) 0 } has no isolated vertices. The total double Roman domination number γ t d R ( G ) is the minimum weight of a TDRDF on G. A TDRDF on G with weight γ t d R ( G ) is called a γ t d R ( G ) -function. Mojdeh et al. [13] have recently defined the Roman { 3 } -dominating function correspondingly to the Roman { 2 } -dominating function of graphs. For a graph G, a Roman { 3 } -dominating function (R { 3 } -DF) is a function f : V { 0 , 1 , 2 , 3 } having the property that f ( N [ u ] ) 3 for every vertex u V with f ( u ) { 0 , 1 } . Formally, a Roman { 3 } -dominating function f : V { 0 , 1 , 2 , 3 } has the property that for every vertex v V , with f ( v ) = 0 , there exist at least either three vertices in V 1 N ( v ) , or one vertex in V 1 N ( v ) and one in V 2 N ( v ) , or two vertices in V 2 N ( v ) , or one vertex in V 3 N ( v ) and for every vertex v V , with f ( v ) = 1 , there exist at least either two vertices in V 1 N ( v ) , or one vertex in ( V 2 V 3 ) N ( v ) . This notion has been defined recently by Mojdeh and Volkmann [13] as Roman { 3 } -domination.
The weight of a Roman { 3 } -dominating function is the sum w f = f ( V ) = v V f ( v ) , and the minimum weight of a Roman { 3 } -dominating function f is the Roman { 3 } -domination number, denoted by γ { R 3 } ( G ) .
Now we introduce the total Roman { 3 } -domination concept to consider such situation.
Definition 1.
Let G be a graph G with no isolated vertex. The total Roman { 3 } -dominating function (TR { 3 } -DF) on G is an R { 3 } -DF f on G with the additional property that every vertex v V with f ( v ) 0 has a neighbor w with f ( w ) 0 , in the other words, the subgraph of G induced by the set { v V ( G ) : f ( v ) 0 } has no isolated vertices. The minimum weight of a total Roman { 3 } -dominating function on G is called the total Roman { 3 } -domination number of G denoted by γ t { R 3 } ( G ) . A γ t { R 3 } ( G ) -function is a total Roman { 3 } -dominating function on G with weight γ t { R 3 } ( G ) .
In this paper We study of total Roman { 3 } -domination versus to other domination parameters. We present an upper bound on the total Roman { 3 } -domination number of a connected graph G in terms of the order of G and characterize the graphs attaining this bound. Finally, we investigate the complexity of total Roman { 3 } -domination for bipartite graphs.

2. Total Roman { 3 } -domination of Some Graphs

First we easily see that γ { R 3 } ( G ) γ t { R 3 } ( G ) γ t d R ( G ) , because by the definitions every total Roman { 3 } -dominating function is a Roman { 3 } -dominating function and every total double Roman dominating function is a total Roman { 3 } -dominating function.
In [10] we have.
Proposition 1.
([10] Proposition 2) Let G be a graph and f = ( V 0 , V 1 , V 2 ) a γ R -function of G. Then γ d R ( G ) 2 | V 1 | + 3 | V 2 | . This bound is sharp.
As an immediate result we also have:
Corollary 1.
Let G be a graph and f = ( V 0 , V 1 , V 2 ) a total Roman { 2 } -dominating function or a Roman dominating function for which the induced subgraph by V 1 V 2 has no isolated vertex. Then γ t { R 3 } ( G ) 2 | V 1 | + 3 | V 2 | . This bound is sharp.
For some special graphs we obtain the total Roman { 3 } -domination numbers.
Observation 1.
Let n 2 . Then γ t { R 3 } ( P n ) = n + 2 i f n 1 ( mod 3 ) n + 1 o t h e r w i s e ,
Proof. 
Let P n = v 1 v 2 v n . Since by assigning 2 to the vertices v 1 and v n and value 1 to the other vertices, we have γ t { R 3 } ( P n ) n + 2 . Since f ( v 1 ) + f ( v 2 ) 3 and f ( v n 1 ) + f ( v n ) 3 , f ( v i 1 ) + f ( v i ) + f ( v i + 1 ) 3 for 4 i n 3 , f ( v i 1 ) + f ( v i ) + f ( v i + 1 ) + f ( v i + 2 ) 3 for 4 i n 4 and f ( v i 2 ) + f ( v i 1 ) + f ( v i ) + f ( v i + 1 ) + f ( v i + 2 ) 4 for 5 i n 4 , we observe that γ t { R 3 } ( P n ) n + 1 and γ t { R 3 } ( P n ) n + 2 if n 1 ( mod 3 ) . If n = 3 k , then by assigning 1 to v 3 t + 1 and v n , 2 to v 3 t + 2 , 0 to v 3 t except v n , we have γ t { R 3 } ( P n ) 3 k + 1 = n + 1 . If n = 2 + 3 k , then by assigning 1 to v 3 t + 1 , 2 to v 3 t + 2 , 0 to v 3 t , we have γ t { R 3 } ( P n ) 3 k + 1 = n + 1 . Thus the proof is complete. □
In [10], it has been shown that γ d R ( C n ) = n if n 0 , 2 , 3 , 4 ( mod 6 ) and otherwise γ d R ( C n ) = n + 1 and since γ t d R ( G ) γ d R ( G ) , we deduce that γ t d R ( C n ) n .
Here we show that γ t { R 3 } ( C n ) = n for all n 3 . If we assign weight 1 to every vertex of C n , then it is a total Roman { 3 } -dominating function of C n . Hence γ t { R 3 } ( C n ) n . In [13], we have shown that γ { R 3 } ( C n ) = n . Since γ { R 3 } ( C n ) γ t { R 3 } ( C n ) , we obtain the desired result.
Observation 2.
γ t { R 3 } ( C n ) = n .
The next result shows another family of graphs G with γ t { R 3 } ( G ) = | V ( G ) | . Let C n be a cycle with vertices v 1 , v 2 , , v n and P m be a path with vertices u 1 , u 2 , , u m for which u 1 = v 1 and for some 2 i m , u i v j . Let H be a graph obtained from a cycle C n and k paths like P m 1 , P m 2 , , P m k ( 1 k n ) such that the first vertex of any path P m i must be v i . Let G be a graph consisting of m graphs like H such that any both of them have at most one common vertex on their cycles. Figure 1 is a sample of graph G is formed of 4 cycles and 15 paths P m i , where m i 1 ( mod 3 ) .
Observation 3.
Let G be the graph constructed as above. If P m i with vertices u 1 i , u 2 i , , u m i is a path such that 3 ( m i 1 ) , then γ t { R 3 } ( G ) = | V ( G ) | .
Proof. 
Let f be a function that assign value 1 to every vertex of the cycles and if 3 ( m i 1 ) , we assign value 2 to vertices with indices 3 t , value 1 to vertices with indices 3 t + 1 , ( 1 t m i 1 3 ) and value 0 to the other vertices of the path P m i , except to the common vertex u 1 i = v i of the cycle. Therefore γ t { R 3 } ( G ) = | V ( G ) | . □
Let C n be a cycle and P m be a path with m vertices and let the first vertex of P m be the vertex v i of C n . If 3 m i or 3 ( m i 2 ) , then γ t { R 3 } ( C n P m ) = | V ( C n P m ) | + 1 . Therefore we have the following result.
Corollary 2.
In the graphs constructed above, if there are l paths P m 1 , P m 2 , , P m l such that 3 m i or 3 ( m i 2 ) for 1 m i l , then γ t { R 3 } ( G ) = | V ( G ) | + l .
The Observation 3 and Corollary 2 show that for every nonnegative integer k, there is a graph G such that γ t { R 3 } ( G ) = | V ( G ) | + k .
Proposition 2.
If G is a connected graph of order n 2 , then γ t { R 3 } ( G ) 3 and γ t { R 3 } ( G ) = 3 if and only if G has at least two vertices of degree Δ ( G ) = n 1 .
Proof. 
If n = 2 , then the statement is clear. Let now n 3 and let f = ( V 0 , V 1 , V 2 , V 3 ) be a total Roman { 3 } -dominating function on G of weight γ { R 3 } ( G ) . If V 0 , then u N ( v ) f ( u ) 3 for a vertex v V 0 and thus γ t { R 3 } ( G ) 3 . If V 0 = , then f ( x ) 1 for each vertex x V ( G ) and therefore γ t { R 3 } ( G ) n 3 .
If G has at least two vertices of degree Δ ( G ) = n 1 , then we may assume v and u are two adjacent vertices of maximum degree. Define the function f by f ( v ) = 1 , f ( u ) = 2 and f ( x ) = 0 for x V ( G ) \ { v , u } . Then f is a total Roman { 3 } -dominating function on G of weight 3 and hence γ t { R 3 } ( G ) = 3 .
Conversely, assume that γ t { R 3 } ( G ) = 3 . Then there are two adjacent vertices v , u with weights 1 and 2 respectively, for which n 2 vertices with weight 0 are adjacent to them, or there are three mutuality adjacent vertices u , v , w with weights 1 for which n 3 vertices with weight 0 are adjacent to them. Therefore there are at least two vertices of degree n 1 . □
As an immediate result we have:
Corollary 3.
If G has only one vertex of degree Δ ( G ) = n 1 , then γ t { R 3 } ( G ) = 4 .
In the follow, total Roman { 3 } -domination and total double Roman domination numbers are compared.
Since any partite set of a bipartite graph is an independent set, the weight of total Roman { 3 } -domination number of any partite set is positive. Therefore we have the following.
Proposition 3.
For any complete bipartite graph we have.
  • γ t { R 3 } ( K 1 , n ) = 4 ,
  • γ t { R 3 } ( K m , n ) = 5 for m { 2 , 3 } and n 3 .
  • γ t { R 3 } ( K m , n ) = γ d R ( K m , n ) = 6 for m , n 4 .
Proof. 
In any complete bipartite graph, let V ( G ) = U W , where U is the small partite set and W is the big partite set.
1. This follows from Corollary 3.
2. We consider two cases.
(i)
Let U = { u 1 , u 2 } and W = { w 1 , w 2 , , w n } . Let f be a TR { 3 } DF of K 2 , n . If f ( W ) = 2 , then f ( U ) 3 . If f ( W ) = 3 , then f ( U ) 2 . If f ( W ) 4 , since f ( U ) is positive, then f ( V ) 5 . Therefore f ( V ) 5 . Assigning f ( u 1 ) = 2 , f ( u 2 ) = 1 and f ( w 1 ) = 2 , shows that γ t { R 3 } ( K 2 , n ) 5 .
(ii)
Let U = { u 1 , u 2 , u 3 } and W = { w 1 , w 2 , , w n } . Using sketch of the proof of item 2, γ t { R 3 } ( K 3 , n ) 5 . If we assign value 1 to the vertices u 1 , u 2 , u 3 , weight 2 to w 1 and 0 to w j , for j 2 , then γ t { R 3 } ( K 3 , n ) 5 .
3. The function f with f ( u 1 ) = 3 = f ( w 1 ) and f ( u i ) = 0 = f ( u j ) for i , j 1 is a TR { 3 } DF for K m , n . Therefore γ t { R 3 } ( K m , n ) 6 .
Now let f be a γ t { R 3 } function of K m , n for m , n 4 . If m , n 5 , then it is easy to see that f should be assigned 0 to at least one vertex of each partite set. Therefore every partite set must have weight at least 3. If, without loss of generality, n = 4 , then let U = { u 1 , u 2 , u 3 , u 4 } . If f ( u i ) 1 for 1 i 4 , then f ( u i ) = 1 for 1 i 4 and thus f ( W ) 2 . So f ( V ) 6 and therefore γ t { R 3 } ( K m , n ) 6 , and the proof is complete. □
One can obtain a similar result for complete r-partite graphs for r 3 .
Proposition 4.
Let G = K n 1 , n 2 , , n r be the complete r-partite graph with r 3 and n 1 n 2 n r . Then:
  • If n 1 = n 2 = 1 , then γ t { R 3 } ( G ) = 3 .
  • If n 1 = 1 and n 2 2 , then γ t { R 3 } ( G ) = 4 .
  • If n 1 = 2 or n 1 3 and r 4 , then γ t { R 3 } ( G ) = 4 .
  • If r = 3 and n 1 3 , then γ t { R 3 } ( G ) = 5 .
Proof. 
Let V = i = 1 r U i where U i is the ith partite set with vertices { u i 1 , u i 2 , , u i n i } .
1. This follows from Proposition 2.
2. This follows from Corollary 3.
3. Let n 1 2 . By Proposition 2, we have γ t { R 3 } ( G ) 4 . If n 1 = 2 , then define f ( u 1 1 ) = f ( u 1 2 ) = f ( u 2 1 ) = f ( u 3 1 ) = 1 and f ( v ) = 0 otherwise. Then f is a TR { 3 } -DF on G with f ( V ) = 4 and thus γ t { R 3 } ( G ) = 4 . Now let n 1 3 and r 4 . Then any TR { 3 } -DF f on G with f ( u 1 1 ) = f ( u 2 1 ) = f ( u 3 1 ) = f ( u 4 1 ) = 1 and f ( v ) = 0 for the other vertices, is a γ t { R 3 } function on G. Therefore γ t { R 3 } ( G ) = 4 .
4. Let n 1 3 and r = 3 , and let f be a TR { 3 } -DF function on G. Since two partite sets must have positive weight, we can assume f ( U 2 ) 1 . If f ( U 2 ) = 1 , then f ( U 1 U 3 ) 4 . If f ( U 2 ) = 2 , then f ( U 1 U 3 ) 3 . If f ( U 2 ) = 3 , then f ( U 1 U 3 ) 2 . If f ( U 2 ) 4 , then f ( U 1 U 3 ) 1 . Thus f ( V ) 5 . Conversely, define f ( u 1 1 ) = f ( u 2 1 ) = 2 and f ( u 3 1 ) = 1 and f ( v ) = 0 otherwise. Then f is a TR { 3 } -DF on G with f ( V ) = 5 and so γ t { R 3 } ( G ) = 5 . □
Theorem 4.
If G is a graph with δ ( G ) = δ 2 , then γ t { R 3 } ( G ) | V ( G ) | + 2 δ , and this bound is sharp.
Proof. 
Let V ( G ) = { u 1 , u 2 , , u n } , and let v be a vertex of degree δ with neighbors { u 1 , u 2 , , u δ } . Let U = { v , u δ + 2 , u δ + 3 , , u n } { u 1 , u 2 } . Define the function f by f ( x ) = 1 for x U and f ( x ) = 0 for x V ( G ) \ U . Then x N ( u ) f ( x ) 2 for u U and x N ( u ) f ( x ) 3 for u V ( G ) \ U . Therefore f is a total Roman { 3 } -dominating function on G of weight n + 2 δ and thus γ t { R 3 } ( G ) | V ( G ) | + 2 δ .
According to Observation 2 and Propositions 3 and 8, we note that γ t { R 3 } ( C n ) = n = | V ( C n ) | + 2 δ ( C n ) , γ t { R 3 } ( K n ) = 3 = | V ( K n ) | + 2 δ ( K n ) for n 3 , γ t { R 3 } ( K 3 , 3 ) = 5 = | V ( K 3 , 3 ) | + 2 δ ( K 3 , 3 ) , γ t { R 3 } ( K 4 , 4 ) = 6 = | V ( K 4 , 4 ) | + 2 δ ( K 4 , 4 ) , γ t { R 3 } ( K 3 , 3 , 3 ) = 5 = | V ( K 3 , 3 , 3 ) | + 2 δ ( K 3 , 3 , 3 ) and γ t { R 3 } ( K n 1 , n 2 , , n r ) = 4 = | V ( K n 1 , n 2 , , n r ) | + 2 δ ( K n 1 , n 2 , , n r ) for r 4 and n 1 n 2 n r = 2 . All these examples demonstrate that the inequality γ t { R 3 } ( G ) | V ( G ) | + 2 δ is sharp. □
Hao et al. defined in [12] the family of graphs G as follows and have proved Theorem 5 below. Let G be the family of graphs that can be obtained from a star S t = K 1 , t 1 of order t 2 by adding a pendant edge to each vertex of V ( S t ) and adding any number of edges joining the leaves of S t .
Theorem 5.
[12] For any connected graph G of order n 2 ,
γ t d R ( G ) 2 n Δ
with equality if and only if G { P 2 , P 3 , C 3 } G .
This theorem with a little changing may be explored as follows.
Theorem 6.
For any connected graph G of order n 2 ,
γ t { R 3 } ( G ) 2 n Δ
with equality if and only if G { P 2 , P 3 } G .

3. Total Roman { 3 } -domination and Total Domination

In this section we study the relationship between total domination and total Roman { 3 } -domination of a graph.
In [10] (Proposition 8) the authors proved that, if G is a graph, then 2 γ ( G ) γ d R ( G ) 3 γ ( G ) .
If we use the method of the proof of Proposition 8 of [10], then it is easy to show that:
If G is a graph with a γ { R 3 } -function f = ( V 0 , V 2 , V 3 ) , then 2 γ ( G ) γ { R 3 } ( G ) 3 γ ( G ) .
In [13] Proposition 17 authors proved that:
If G is a graph, then γ ( G ) + 2 γ { R 3 } ( G ) 3 γ ( G ) , and these bounds are sharp. However, we have the following.
Proposition 5.
If G is a graph without isolated vertices, then γ t ( G ) + 1 γ t { R 3 } ( G ) 3 γ t ( G ) .
Proof. 
Let S be a γ t -set of G. Then ( V 0 = V \ S , , , V 3 = S ) is a γ t { R 3 } -function of G. Therefore γ t { R 3 } ( G ) 3 γ t ( G ) .
For the lower bound, let f = ( V 0 , V 1 , V 2 , V 3 ) be a γ t { R 3 } -function of G. We distinguish two cases.
Case 1. Let | V 2 | 1 or | V 3 | 1 . Then γ t ( G ) | V 1 | + | V 2 | + | V 3 | | V 1 | + 2 | V 2 | + 3 | V 3 | 1 = γ t { R 3 } ( G ) 1 .
Case 2. Let V 2 = V 3 = . By the definition, δ ( G [ V 1 ] ) 2 . Therefore, for each vertex v V 1 , the subgraph G [ V 1 \ { v } ] does not contain an isolated vertex. Consequently, V 1 \ { v } is total dominating set of G and hence γ t ( G ) γ t { R 3 } ( G ) 1 . □
By Proposition 5 the question may arise as whether for any positive integer r, exists a graph G for which γ t { R 3 } ( G ) = γ t ( G ) + r , where 1 r 2 γ t ( G ) . For r = 1 we have. If G is a connected graph of order n 2 with at least two vertices of maximum degree Δ ( G ) = n 1 , then Proposition 2 implies that γ t { R 3 } ( G ) = 3 . Since γ t ( G ) = 2 for such graphs, we observe that γ t { R 3 } ( G ) = γ t ( G ) + 1 .
Proposition 6.
If G is a graph without isolated vertices, then γ t { R 3 } ( G ) = γ t ( G ) + 1 if and only if G has at least two vertices of degree Δ = | V ( G ) | 1 , in the other words γ t { R 3 } ( G ) = 3 and γ t ( G ) = 2 .
Proof. 
The part “if“ has been proved. Part “only if“: Let G be a graph with γ t { R 3 } ( G ) = γ t ( G ) + 1 . Let f = ( V 0 , V 1 , V 2 , V 3 ) be a γ t { R 3 } ( G ) function. Therefore V 1 V 2 V 3 is a total dominating set for G, and | V 1 | + | V 2 | + | V 3 | γ t ( G ) = γ t { R 3 } ( G ) 1 = | V 1 | + 2 | V 2 | + 3 V 3 | 1 . Therefore | V 2 | + 2 | V 3 | 1 that is | V 2 | 1 and | V 3 | = 0 . If | V 2 | = 1 = | V 1 | or | V 2 | = 0 and | V 1 | = 3 , then G has at least two vertices of degree Δ ( G ) = | V ( G ) | 1 . Now we show that there are not any cases for G. On the contrary, we suppose that there are different cases. (1) | V 2 | = 1 and | V 1 | 2 . (2) | V 2 | = 0 and | V 1 | 4 .
Case 1. Let V 2 = { v } , | V 1 | 2 . Assume first that there exist two vertices v 1 , v 2 V 1 which are adjacent to the vertex v. Then V 2 V 1 \ { v 1 } is a γ t ( G ) -set of size | V 1 | and so γ t { R 3 } ( G ) = 2 + | V 1 | , a contradiction. Assume next that there exists only one vertex, say v 1 V 1 , which is adjacent to v. Then all other vertices of V 1 have at least two neighbors in V 1 . If v 2 V 1 with v 2 v 1 , then we observe that V 2 V 1 \ { v 2 } is a γ t ( G ) -set of size | V 1 | . It follows that γ t { R 3 } ( G ) = 2 + | V 1 | , a contradiction.
Case 2. Let | V 2 | = 0 and | V 1 | 4 . Then there exist two vertices v 1 , v 2 in which each of them has neighbors in V 1 \ { v 1 , v 2 } and G ( V 1 \ { v 1 , v 2 } ) has no isolated vertex. Therefore V 1 \ { v 1 , v 2 } is a γ t ( G ) -set that is also a contradiction. □
Now we show that for any positive integer n and integer 2 r 2 n , there exists a graph G for which γ t ( G ) = n and γ t { R 3 } ( G ) = n + r .
Proposition 7.
Let n and r be positive integers with 2 r 2 n . Then there exists a graph G for which γ t ( G ) = n and γ t { R 3 } ( G ) = n + r .
Proof. 
For graph G with γ t ( G ) = n and γ t { R 3 } ( G ) = n + 2 , we consider the following graph. Let H be the graph consisting of a cycle C n + 2 with n 3 and a vertex set V 0 of n + 2 3 further vertices. Let each vertex of V 0 be adjacent to 3 vertices of V ( C n + 2 ) such that the neighborhoods of every two distinct vertices of V 0 are different. Let V 1 = V ( C n + 2 ) . Then γ t { R 3 } ( H ) = n + 2 and γ t ( H ) = n (Figure 2).
For γ t ( G ) = n and γ t { R 3 } ( G ) = n + k , where 3 k n 1 . Let k = 3 . For γ t ( G ) = 4 and γ t { R 3 } ( G ) = 7 , we consider the cycle C 7 . For γ t ( G ) 5 , let H be the above graph where γ t ( H ) = n 3 and γ t { R 3 } ( H ) = n + 2 5 . Now we consider G = H K 3 . Then γ t ( G ) n 4 and γ t { R 3 } ( G ) = n + 3 .
Let k = 4 . For γ t ( G ) = 5 and γ t { R 3 } ( G ) = 9 , we consider the cycle C 9 . For γ t ( G ) 6 , consider the graphs G with γ t { R 3 } ( G ) = γ t ( G ) + 3 for γ t ( G ) 4 . Now we let G = G K 3 . Then we have γ t { R 3 } ( G ) = γ t ( G ) + 4 .
For 5 k n 1 we use induction on k. Let for any integer 4 m k 1 there exist graphs G such that γ t { R 3 } ( G ) = γ t ( G ) + m for γ t ( G ) m + 1 . Let m = k . For γ t ( G ) = k + 1 and γ t { R 3 } ( G ) = 2 k + 1 , we consider the cycle C 2 k + 1 . For graphs G with γ t { R 3 } ( G ) = γ t ( G ) + k for γ t ( G ) k + 2 , using hypothesis of induction, let G be the graphs with γ t { R 3 } ( G ) = γ t ( G ) + k 1 with γ t ( G ) k . Now we let G = G K 3 . It can be seen γ t { R 3 } ( G ) = γ t ( G ) + k for γ t ( G ) k + 2 .
We now verify the case of γ t { R 3 } ( G ) = 2 γ t ( G ) + r for 0 r γ t ( G ) , that is, we wish to show the existence of graphs G, so that γ t ( G ) = n and γ t { R 3 } ( G ) = 2 n + r for 0 r n . Let r = 0 . For even n, let G = C 2 n . Then γ t ( G ) = n and γ t { R 3 } ( G ) = 2 n .
For odd n = 2 k + 1 , if 2 n 1 ( m o d 3 ) or 2 n 0 ( m o d 3 ) , then we let G = P 2 n 1 , and by Observation 1, it can be seen that γ t ( G ) = n and γ t { R 3 } ( G ) = 2 n .
If 2 n 2 ( m o d 3 ) , consider a cycle C 2 n 1 with an additional vertex a that is adjacent to two vertices v 1 and v 2 . Then γ t ( G ) = n and γ t { R 3 } ( G ) = 2 n .
For r = 1 and positive even integer n, consider G = ( n 2 1 ) P 3 C 5 + , where ( n 2 1 ) P 3 is the union of n 2 1 of path P 3 and C 5 + is the cycle C 5 with a chord, then γ t ( G ) = n and γ t { R 3 } ( G ) = 2 n + 1 . For r = 1 and positive odd integer n, consider G = ( n 1 2 1 ) P 3 P 5 + where P 5 + is the path P 5 with an additional vertex adjacent to the second or fourth vertex of P 5 , then γ t ( G ) = n and γ t { R 3 } ( G ) = 2 n + 1 .
For 2 r n 1 , we do as follows. Let r = 2 and so n 3 . Let n = 3 and 2 n + 2 = 8 . Let G 1 be a graph constructed from path P 5 with vertices v 1 , v 2 , v 3 , v 4 , v 5 with additional vertices u 12 , u 13 , u 14 , u 52 , u 53 , u 54 , u 24 such that the given vertex u i , j is adjacent to vertices v i and v j of P 5 . Then γ t ( G 1 ) = 3 and γ t { R 3 } ( G 1 ) = 8 .
Let n = 4 and 2 n + 2 = 10 . Then say G 2 = 2 C 5 + . Let n = 5 and so 2 n + 2 = 12 . Then say G 3 = C 5 + P 5 + . For γ t ( G ) = k and γ t { R 3 } ( G ) = 2 k + 2 , where r + 1 k n , there consider three cases.
  • If k 0 ( m o d 3 ) , then we say G = k 3 3 P 5 G 1 .
  • If k 1 ( m o d 3 ) , then we say G = k 4 3 P 5 G 2 .
  • If k 2 ( m o d 3 ) , then we say G = k 5 3 P 5 G 3 .
It is easy to verifiable, γ t ( G ) = k and γ t { R 3 } ( G ) = 2 k + 2 .
Let r = 3 and so n 4 . For graph G 1 with γ t ( G 1 ) = 4 and γ t { R 3 } ( G 1 ) = 11 , we let G 1 = P 4 C 5 + . For graph G 2 with γ t ( G 2 ) = 5 and γ t { R 3 } ( G 2 ) = 13 , we let G 2 = P 4 P 5 + . And for graph G 3 with γ t ( G 3 ) = 6 and γ t { R 3 } ( G 3 ) = 15 , we let G 3 = 3 C 5 + . For γ t ( G ) = k and γ t { R 3 } ( G ) = 2 k + 3 , where r + 1 k n , there consider three cases.
  • If k 1 ( m o d 3 ) , then we say G = k 4 3 P 5 G 1 .
  • If k 2 ( m o d 3 ) , then we say G = k 5 3 P 5 G 2 .
  • If k 0 ( m o d 3 ) , then we say G = k 6 3 P 5 G 3 .
Let r 4 and n r + 1 . For graph G with γ t ( G ) = k and γ t { R 3 } ( G ) = 2 k + r where r + 1 k n , there consider two cases.
Case 1. Let r be an even integer. Then there exists a graph G for which γ t ( G ) = k ( r 2 ) and γ t { R 3 } ( G ) = 2 k 2 ( r 2 ) + 2 . Now let G = r 2 2 P 4 G . Then γ t ( G ) = r 2 + γ t ( G ) = k and γ t { R 3 } ( G ) = 3 ( r 2 ) + γ t { R 3 } ( G ) = 3 ( r 2 ) + 2 k 2 ( r 2 ) + 2 = 2 k + r .
Case 2. Let r be an odd integer. Then there exists a graph G for which γ t ( G ) = k ( r 3 ) and γ t { R 3 } ( G ) = 2 k 2 ( r 3 ) + 3 . If we consider G = r 3 2 P 4 G . Then γ t ( G ) = r 3 + γ t ( G ) = k and γ t { R 3 } ( G ) = 3 ( r 3 ) + γ t { R 3 } ( G ) = 2 k + r .
Finally, we want discuss the case of r = n , that is we want to find graphs G with γ t ( G ) = n and γ t { R 3 } ( G ) = 3 n . For n = 2 and 3 n = 6 , let G = P 4 . For G with γ t ( G ) = 3 and γ t { R 3 } ( G ) = 9 , let G = H 1 be a graph constructed from P 5 with vertices v 1 , v 2 , v 3 , v 4 , v 5 with three additional vertices w 1 , w 2 , w 3 and three pendant edges v 2 w 2 , v 3 w 3 , v 4 w 4 . Then it can be seen that γ t ( H 1 ) = 3 and γ t { R 3 } ( H 1 ) = 9 .
Let n 4 . If n is an even, then let G = n 2 P 4 and if n is an odd, then let G = n 3 2 P 4 H 1 . In both cases γ t ( G ) = n and γ t { R 3 } ( G ) = 3 n . □

4. Total Roman { 3 } and Total Roman { 2 } -domination

In [13] it has been shown that, for a connected graph G with a γ { R 3 } -function f = ( V 0 , V 2 , V 3 ) , γ { R 3 } ( G ) γ ( G ) + γ { R 2 } ( G ) .
In this section we investigate the relation between total Roman { 3 } and total Roman { 2 } -domination. First we have the following.
Observation 7.
Let G be a graph and ( V 0 , V 1 , V 2 ) be a γ t { R 2 } function of G. Then ( V 0 = V 0 , V 2 = V 1 , V 3 = V 2 ) is a TR { 3 } -DF function. Conversely, if ( V 0 , V 1 , V 2 , V 3 ) is a γ t { R 3 } of G, then ( U 0 = V 0 , U 1 = V 1 V 2 , U 2 = V 3 ) is a TR { 2 } -DF of G.
Proof. 
The proof is straightforward. □
The following results state the relation between γ t { R 3 } and γ t { R 2 } of graphs G when γ t { R 3 } ( G ) is small.
Proposition 8.
Let G be a graph. Then:
  • γ t { R 3 } ( G ) = 3 if and only if γ t { R 2 } ( G ) = 2 .
  • If γ t { R 3 } ( G ) = 4 , then γ t { R 2 } ( G ) = 3 .
  • If γ t { R 2 } ( G ) = 3 , then 4 γ t { R 3 } ( G ) 5 .
Proof. 
1. Let γ t { R 3 } ( G ) = 3 . Then there exist two adjacent vertices v , u with label 2 , 1 respectively so that each vertex with label 0 is adjacent to them or there exist three mutually adjacent vertices v , u , w with label 1 so that each vertex with label 0 is adjacent to them. In the first case, we change the vertex with label 2 to the label 1 and in the second case we change one of the vertices with label 1 to the label 0. These changing labels give us a γ t { R 2 } ( G ) -function with weight 2. Conversely, let γ t { R 2 } ( G ) = 2 . Then there exist two vertices with label 1 for which every vertex is adjacent to them. We change one of the labels to 2, and therefore the result holds.
2. Let γ t { R 3 } ( G ) = 4 . There are three cases.
2.1.
There exist 4 vertices v , u , w , z with label 1 for which the induced subgraph by them is the cycle C 4 , the graph K = K 4 e or the complete graph K 4 . In any induced subgraph, there are no two vertices of them for which any vertex with label 0 is adjacent to them. Thus in the case of a TR { 2 } -DF we change one of the labels 1 to the label 0. Therefore γ t { R 2 } ( G ) = 3 .
2.2.
There exist 2 vertices v , u with label 1 and one vertex w with label 2, for which the induced subgraph by them is the cycle C 3 , or the path P 3 = v w u . In any of the two cases each vertex with label 0 is adjacent to v , w or u , w or three of them. Now we change the label of w to 1, and we obtain a γ t { R 2 } -function for G with weight 3.
2.3.
There exist 2 vertices v , u with label 3 and label 1, respectively, for which the induced subgraph by v , u is K 2 . By this assumption each vertex with label 0 is adjacent to v, but there maybe exist some vertices (none of them) which are adjacent to u. Now we change the label v to 2, and we obtain a γ t { R 2 } -function for G with weight 3.
3. Let γ t { R 2 } ( G ) = 3 . There are two cases.
3.1.
There exist 3 vertices v , u , w with label 1 for which the induced subgraph by v , u , w is the cycle C 3 or a path P 3 . If each vertex with label 0 is adjacent to v , w or u , w , then by changing the label w to 2, we obtain a γ t { R 3 } -function for G with weight 4.
If some vertices with label 0 are adjacent to v , u , some of them are adjacent to v , w and the other are adjacent u , w , then by changing two vertices of v , u , w to label 2, we obtain a γ t { R 3 } -function for G with weight 5.
3.2.
There exist 2 vertices v , u with label 2 and label 1, respectively, for which the induced subgraph by v , u is K 2 . By this assumption each vertex with label 0 is adjacent to v, but there maybe exist some vertices (none of them) which are adjacent to u. Now we change the label v to 3, and we obtain a γ t { R 3 } -function for G with weight 4. Therefore 4 γ t { R 3 } ( G ) 5 . □
In the following we want to find the relation between total Roman { 3 } -domination, total domination and total Roman { 2 } -domination of graphs.
Observation 8.
Let G be a connected graph with a γ t { R 3 } -function f = ( V 0 , V 2 , V 3 ) . Then γ t { R 3 } ( G ) γ t ( G ) + γ t { R 2 } ( G ) .
Proof. 
Let ( V 0 , V 2 , V 3 ) be a γ t { R 3 } -function of G. Then γ t ( G ) | V 2 | + | V 3 | . If we define g = ( V 0 = V 0 , V 1 = V 2 , V 2 = V 3 ) , then g is a total Roman { 2 } -dominating function on G. Therefore γ t ( G ) + γ t { R 2 } ( G ) | V 2 | + | V 3 | + | V 1 | + 2 | V 2 | 2 | V 2 | + 3 | V 3 | = γ t { R 3 } ( G ) . □
In Observation 8 the condition of γ t { R 3 } -function f = ( V 0 , V 2 , V 3 ) is necessary. Because there are many graphs for which the result of Observation 8 does not hold. For example, for the complete graphs K n ( n 2 ) , cycles C n and paths P n for n 5 , we observe that γ t { R 3 } ( G ) < γ t ( G ) + γ t { R 2 } ( G ) . However, in the following we establish, for any integer n 5 , there is a graph G such that γ t { R 3 } ( G ) = γ t { R 2 } ( G ) + γ t ( G ) .
Proposition 9.
For any positive integer n 5 , there is a graph G for which γ t { R 3 } ( G ) = γ t { R 2 } ( G ) + γ t ( G ) .
Proof. 
For n = 5 let G = C 5 + . Then γ t { R 2 } ( G ) = 3 , γ t ( G ) = 2 and γ t { R 3 } ( G ) = 5 . For n = 6 , let G be a bistar of order 6. Then γ t { R 3 } ( G ) = 6 = 4 + 2 = γ t { R 2 } ( G ) + γ t ( G ) . For n = 7 , let G = G 1 in Figure 3. For n = 8 , let G = G 2 in Figure 3. For n = 9 , let G = G 2 in Figure 3. For n 10 , by induction we consider the graph G = C 5 + H where the graph H (H may be connected or disconnected) for which γ t { R 3 } ( H ) = n 5 = γ t { R 2 } ( H ) + γ t ( H ) . □
Finally, we show that for any positive integer n 5 , there is a graph G such that γ t { R 3 } ( G ) = n , γ t { R 2 } ( G ) = n 1 and γ t ( G ) = n 2 .
For this, let G be the graph constructed in Proposition 3 as graph H for n 5 . Then γ t { R 3 } ( H ) = n , γ t { R 2 } ( H ) = n 1 and γ t ( H ) = n 2 .

5. Large Total Roman { 3 } -domination Number

In this section, we characterize connected graphs G of order n with γ t { R 3 } ( G ) = 2 n k for 1 k 4 . For this we use the following result.
Theorem 9.
Let G be a connected graph of order n 2 . Then γ t { R 3 } ( G ) ( 3 n ) / 2 , with equality if and only if G is the corona H K 1 where H is a connected graph.
Proof. 
If n = 2 , then the statement is valid. Let now n 3 . If | L ( G ) | n / 2 , then define f : V ( G ) { 0 , 1 , 2 , 3 } by f ( x ) = 2 for x L ( G ) and f ( x ) = 1 for x V ( G ) \ L ( G ) . Then f is a total Roman { 3 } -dominating function on G of weight
2 | L ( G ) | + n | L ( G ) | = n + | L ( G ) | 3 n 2 .
If | L ( G ) | > n / 2 , then define f : V ( G ) { 0 , 1 , 2 , 3 } by f ( x ) = 1 for x L ( G ) and f ( x ) = 2 for x V ( G ) \ L ( G ) . Then f is a total Roman { 3 } -dominating function on G of weight
| L ( G ) | + 2 ( n | L ( G ) | ) = 2 n | L ( G ) | < 3 n 2 .
If G = H K 1 for a is a connected graph H, then γ t { R 3 } ( G ) = ( 3 n ) / 2 .
Conversely, let γ t { R 3 } ( G ) = ( 3 n ) / 2 . Then the proof above shows that | L ( G ) | = n / 2 . Assume that there exists a vertex v V ( G ) which is neither a leaf nor a support vertex. Define f : V ( G ) { 0 , 1 , 2 , 3 } by f ( x ) = 1 for x L ( G ) { v } and f ( x ) = 2 for x V ( G ) \ ( L ( G ) { v } ) . Then f is a total Roman { 3 } -dominating function on G of weight
| L ( G ) | + 2 ( n | L ( G ) | 1 ) + 1 = 2 n | L ( G ) | 1 = 3 n 2 1 ,
a contradiction. Thus every vertex is a leaf or a support vertex. Since | L ( G ) | = n / 2 , we deduce that G = H K 1 with a connected graph H. □
Corollary 4.
For any connected graph G of order n 2 , γ t { R 3 } ( G ) = 2 n 1 if and only if G = P 2 .
Proof. 
Let γ t { R 3 } ( G ) = 2 n 1 . Then Theorem 9 implies 2 n 1 ( 3 n ) / 2 and thus n = 2 . Clearly, the statement is valid for P 2 . □
Corollary 5.
For any connected graph G of order n 3 , γ t { R 3 } ( G ) = 2 n 2 if and only if G { P 3 , P 4 } .
Proof. 
If G { P 3 , P 4 } , then the statement is valid. Conversely, let γ t { R 3 } ( G ) = 2 n 2 . Then Theorem 9 implies 2 n 2 ( 3 n ) / 2 and thus n 4 , with equality if and only if G = P 4 . In the remaining case n = 3 , we observe that G { P 3 , C 3 } with γ t { R 3 } ( P 3 ) = 4 and γ t { R 3 } ( C 3 ) = 3 , and therefore G = P 3 . □
Next we characterize the graphs G with the property that γ t { R 3 } ( G ) = 2 | V ( G ) | 3 .
Theorem 10.
For any connected graph G of order n 3 , γ t { R 3 } ( G ) = 2 n 3 if and only if G { C 3 , P 3 K 1 , C 3 K 1 } .
Proof. 
If G { C 3 , P 3 K 1 , C 3 K 1 } , then the statement is valid. Conversely, let γ t { R 3 } ( G ) = 2 n 3 . If Δ ( G ) = 2 , then G { P n , C n } and we conclude by Observations 1, 2 that G = C 3 . If Δ ( G ) = 3 , then γ t { R 3 } ( G ) = 2 n 3 = 2 n Δ ( G ) and so by Theorem 6, G G . Therefore G { P 3 K 1 , C 3 K 1 } . Let Δ ( G ) 4 . Then by Theorem 6, γ t { R 3 } ( G ) 2 n Δ ( G ) = 2 n 4 < 2 n 3 . Thus G { C 3 , P 3 K 1 , C 3 K 1 } , and the proof is complete. □
Let H be the family of connected graphs order 5 with Δ ( G ) = 3 which have exactly one leaf or the tree T 5 consisting of the path v 1 v 2 v 3 v 4 such that v 2 is adjacent to a further vertex w.
Let F be the family of graphs G = Q K 1 with a connected graph Q of order 4.
Observation 11.
If G { F , H } , then γ t { R 3 } ( G ) = 2 n 4 .
Proof. 
Clearly, γ t { R 3 } ( T 5 ) = 2 n 4 = 6 . Let G H be of order 5 with exactly one leaf u. If v is the support vertex of u, then f : V ( G ) { 0 , 1 , 2 , 3 } with f ( v ) = 2 and f ( x ) = 1 for x V ( G ) \ { v } is a TR { 3 } -DF on G and therefore γ t { R 3 } ( G ) = 6 = 2 n 4 .
If G = Q K 1 with a connected graph Q of order 4, then we have seen in proof of Theorem 9 that γ t { R 3 } ( G ) = ( 3 n ) / 2 = 2 n 4 = 12 . □
Theorem 12.
For any connected graph G of order n 4 , we have γ t { R 3 } ( G ) = 2 n 4 if and only if G { C 4 , P 5 } { c l a w , p a w } H F where claw is K 1 , 3 and paw is obtained from K 1 , 3 by adding one edge between two arbitrary distinct vertices.
Proof. 
Let G { C 4 , P 5 } { c l a w , p a w } H F . By Observations 1, 2 and 11, we have γ t { R 3 } ( G ) = 2 n 4 .
Conversely, let γ t { R 3 } ( G ) = 2 n 4 . According to Theorem 9, we have 2 n 4 = γ t { R 3 } ( G ) ( 3 n ) / 2 and thus n 8 with equality if and only if G is the corona H K 1 with a connected graph H of order 4. Therefore G F if n = 8 . Let now n 7 .
If Δ ( G ) = 2 , then G { P n , C n } and by Observations 1, 2, we have n = 2 n 4 which implies n = 4 and G = C 4 , or n + 1 = 2 n 4 which implies n = 5 and G = P 5 or n + 2 = 2 n 4 which implies G = P 6 . Since γ t { R 3 } ( C 4 ) = 4 = 2 n 4 and γ t { R 3 } ( P 5 ) = 6 = 2 n 4 but γ t { R 3 } ( P 6 ) = 7 2 n 4 , we deduce that G { C 4 , P 5 } .
Let now Δ ( G ) = 3 . Next we discuss the cases n = 4 , 5 , 6 or n = 7 .
If n = 4 , then for only two graphs G, the claw and the paw, we have γ t { R 3 } ( G ) = 4 = 2 n 4 .
If n = 5 , it is simply verified that γ t { R 3 } ( G ) = 6 = 2 n 4 if an only if G H .
If n = 6 , then let v be a vertex of degree 3 with the neighbors u 1 , u 2 , u 3 , and let w 1 and w 2 be the remaining vertices. Assume, without loss of generality, that w 1 is adjacent to u 1 .
Case 1: Assume that w 2 is adjacent to u 1 . Then f : V ( G ) { 0 , 1 , 2 , 3 } with f ( v ) = f ( u 1 ) = 3 and f ( x ) = 0 for x v , u 1 is a TR { 3 } -DF on G and therefore γ t { R 3 } ( G ) 6 .
Case 2: Assume that w 2 is adjacent to w 1 . Then f : V ( G ) { 0 , 1 , 2 , 3 } with f ( v ) = f ( w 1 ) = 3 , f ( u 1 ) = 1 and f ( x ) = 0 for x v , u 1 , w 1 is a TR { 3 } -DF on G and therefore γ t { R 3 } ( G ) 7 .
Case 3: Assume that w 2 is adjacent to u 2 or u 3 , say u 2 . If there are no further edges, then γ t { R 3 } ( G ) = 9 2 n 4 .
Now assume that there are further edges. If w 2 is adjacent to u 3 , then f : V ( G ) { 0 , 1 , 2 , 3 } with f ( u 1 ) = 2 and f ( x ) = 1 for x u 1 is a TR { 3 } -DF on G and therefore γ t { R 3 } ( G ) 7 . If w 1 is adjacent to u 2 , then f : V ( G ) { 0 , 1 , 2 , 3 } with f ( v ) = f ( u 2 ) = 3 and f ( x ) = 0 for x v , u 2 is a TR { 3 } -DF on G and therefore γ t { R 3 } ( G ) 6 . If u 1 is adjacent to u 2 and there are no further edges, then γ t { R 3 } ( G ) = 9 2 n 4 . If finally, u 3 is adjacent to u 2 or u 1 , say u 2 , then f : V ( G ) { 0 , 1 , 2 , 3 } with f ( u 1 ) = f ( u 2 ) = 3 , f ( v ) = 1 and f ( x ) = 0 for x v , u 1 , u 2 is a TR { 3 } -DF on G and therefore γ t { R 3 } ( G ) 7 . Thus we see that there is no graph G of order 6 with γ t { R 3 } ( G ) = 8 = 2 n 4 .
Let now n = 7 . If | L ( G ) | 2 , then define f : V ( G ) { 0 , 1 , 2 , 3 } by f ( x ) = 2 for x L ( G ) and f ( x ) = 1 for x V ( G ) \ L ( G ) . Then f is a total Roman { 3 } -dominating function on G of weight 9 < 10 = 2 n 4 . If | L ( G ) | 4 , then define f : V ( G ) { 0 , 1 , 2 , 3 } by f ( x ) = 0 for x L ( G ) and f ( x ) = 3 for x V ( G ) \ L ( G ) . Then f is a total Roman { 3 } -dominating function on G of weight 9 < 10 = 2 n 4 .
Finally, assume that | L ( G ) | = 3 . If G has exactly 3 support vertices, then define f : V ( G ) { 0 , 1 , 2 , 3 } by f ( x ) = 1 for x L ( G ) , f ( x ) = 2 for x S ( G ) and f ( x ) = 0 for the remaining vertex. Then f is a total Roman { 3 } -dominating function on G of weight 9 < 10 = 2 n 4 . If G has exactly 2 support vertices, then define f : V ( G ) { 0 , 1 , 2 , 3 } by f ( x ) = 0 for x L ( G ) , f ( x ) = 3 for x S ( G ) and f ( x ) = 1 for the remaining two vertices. Then f is a total Roman { 3 } -dominating function on G of weight 8 < 10 = 2 n 4 .
Let Δ ( G ) = 4 . By Theorem 6, γ t { R 3 } ( G ) = 2 n 4 if and only if G G F .
Let Δ ( G ) 5 . Then by Theorem 6 γ t { R 3 } ( G ) 2 n 5 < 2 n 4 . Therefore the proof is complete. □

6. Complexity

In this section, we study the complexity of total Roman { 3 } -domination of graphs. We show that the total Roman { 3 } -domination problem is N P -complete for bipartite graphs. Consider the following decision problem.
Total Roman { 3 } -domination problem TR3DP.
Instance: Graph G = ( V , E ) , and a positive integer k | V | .
Question: Does G have a total Roman { 3 } -domination of weight at most k?
It is well-known that the Exact-3-Cover (X3C) problem is NP-complete. We show that the NP-completeness of TR3D problem by reducing the Exact-3-Cover (X3C), to TR3D.
EXACT 3-COVER ( X 3 C )
Instance: A finite set X with | X | = 3 q and a collection C of 3-element subsets of X.
Question: Is there a subcollection C of C such that every element of X appears in exactly one element of C ?
Theorem 13.
TR3D is N P -Complete for bipartite graphs.
Proof. 
It is clear that TR3DP belongs to N P . Now we show that, how to transform any instance of X3C into an instance G of TR3D so that, the solution one of them is equivalent to the solution of the other one. Let X = { x 1 , x 2 , , x 3 r } and C = { C 1 , C 2 , , C t } be an arbitrary instance of X3C.
For each x i X , we form a graph G i obtained from a path P 5 : y i 1 - y i 2 - y i 3 - y i 4 - y i 5 by adding the edge y i 2 y i 5 . For each C j C , we form a star K 1 , 5 with center c j for which one leaf is labeled l j . Let L = { l 1 , l 2 , , l t } . Now to obtain a graph G, we add edges l j y i 1 if y i 1 C j . Set k = 4 t + 13 r . Let H = i = 1 3 r V ( G i ) be the subgraph of G induced by the i = 1 3 r V ( G i ) . Observe that for every total Roman { 3 } -dominating function f on G with f ( V ( G i ) ) 4 , all vertices on each cycle C 4 = y i 2 - y i 3 - y i 4 - y i 5 - y i 2 are total Roman { 3 } -dominated. Moreover, since G i has a total Roman { 3 } -domination number equal to 6, we can assume that f ( V ( G i ) ) 6 . More precisely, if f ( V ( G i ) ) = 6 , then, without loss of generality, we may assume that f ( y i 2 ) = f ( y i 3 ) = f ( y i 2 ) = f ( y i 3 ) = 1 and f ( y i 1 ) = 2 . If also, f ( V ( G i ) ) { 4 , 5 } , then obviously at least one vertex of G i (including y i 1 ) is not total Roman { 3 } -dominated. In this case, we can assume that vertices of G i are assigned as f ( y i 2 ) = f ( y i 3 ) = f ( y i 4 ) = f ( y i 5 ) = 1 so that, only y i 1 is not total Roman { 3 } -dominated and f ( y i 1 ) { 0 , 1 } .
Suppose that the instance X, C of X 3 C has a solution C . We build a total Roman { 3 } -dominating function f on G of weight k. For every C j , assign the value 2 to l j if C j C and 1 to the other l j if C j C . Assign value 3 to every c j and value 0 to each leaf adjacent to c j . Finally, for every i, assign 1 to y i 2 , y i 3 , y i 4 , y i 5 , and 0 to y i 1 of G i . Since C exists, | C | = r , the number of l j s with weight 2 is r, having disjoint neighborhoods in { y 1 1 , y 2 1 , , y 3 r 1 } , where every y i 1 has one neighbors assigned 1 and one neighbor assigned 2. Also since the number of l j s with weight 1 is t r . Hence, it can be easily seen that f is a TR3-D function with weight f ( V ) = 3 t + 2 r + t r + 12 r = k .
Conversely, let g = ( V 0 , V 1 , V 2 , V 3 ) be a total Roman { 3 } -dominating function of G with weight at most k. Obviously, every star needs a weight of at least 4, and so without loss of generality, we may assume that g ( c j ) = 3 and all the leaves neighbor of c j are assigned 0. Since l j c j E ( G ) , it implies that each vertex l j can be assigned by 1. Moreover, for each i, g ( V ( G i ) ) { 4 , 6 } , as mentioned above. We can let the vertices of G i are assigned the values given in the above paragraph depending on whether g ( V ( G i ) ) = 4 or g ( V ( G i ) ) = 6 . Let p be the number of G i s having weight 6. Then g ( V ( H ) ) = 6 p + 4 ( 3 r p ) = 12 r + 2 p . Now, if g ( l j ) > 1 for some j, then l j total Roman { 3 } -dominates some vertex y s 1 , and, in that case, g ( l j ) = 2 (since g ( y i 2 ) = 1 ) . Let z be the number of l j s assigned 2 and t z of others be assigned 1. Then 3 t + 2 z + t z + 12 r + 2 p k = 4 t + 13 r , implies that z + 2 p q . On the other hand, since each l j has exactly three neighbors in { x 1 1 , x 2 1 , , x 3 r 1 } , we must have 3 z 3 r p . From these two inequalities, we achieve at p = 0 and then z = q . Consequently, C = { C j : g ( l j ) = 2 } is an exact cover for C. □

7. Open Problems

In the preceding sections a new model of total Roman domination, total Roman { R 3 } -domination has been introduced. There are the relationships between the total domination, total Roman { R 2 } -domination and total Roman { R 3 } -domination numbers as follows:
If G is a graph without isolated vertices, then γ t ( G ) + 1 γ t { R 3 } ( G ) 3 γ t ( G ) , (Proposition 5).
If G is a graph without isolated vertices, then γ t { R 3 } ( G ) = γ t ( G ) + 1 if and only if G has at least two vertices of degree Δ = | V ( G ) | 1 , in the other words γ t { R 3 } ( G ) = 3 and γ t ( G ) = 2 . (Proposition 6).
For any positive integer n 5 , there is a graph G of order n in which γ t { R 3 } ( G ) = γ t { R 2 } ( G ) + γ t ( G ) , (Proposition 9).
For a family of graphs we have shown that γ t { R 3 } ( G ) = | V ( G ) | , (Observation 3).
We have already characterized graphs G in which γ t { R 3 } ( G ) = 2 | V ( G ) | r , where 1 r 4 .
Problems
1. Characterize the graphs G for which γ t { R 3 } ( G ) = 3 γ t ( G ) .
2. Does there exist any characterization of graphs G for which γ t { R 3 } ( G ) = γ t ( G ) + r , where 2 r γ t ( G ) 2 ?
3. For positive integers n 5 , characterize the graphs G for which γ t { R 3 } ( G ) = γ t { R 2 } ( G ) + γ t ( G ) .
4. Does there exist any characterization of graphs G for which γ t { R 3 } ( G ) = | V ( G ) | ?
5. Can one characterize graphs G in which γ t { R 3 } ( G ) = 2 | V ( G ) | r for 5 r | V ( G ) | 1 ?
6. Is it possible to construct a polynomial algorithm for computing of γ t { R 3 } ( T ) for any tree T?

Author Contributions

Conceptualization, D.A.M., Z.S., and L.V.; writing, D.A.M.; revising, L.V., Z.S., and D.A.M. All authors have read and agreed to the published version of the manuscript.

Funding

This research received no external funding.

Acknowledgments

The first author’s research work was supported by the National Key R & D Program of China (Grant No. 2019YFA0706402) and the Natural Science Foundation of Guangdong Province under Grant 2018A0303130115, and the second author’s research work has been supported by a research grant from the University of Mazandaran. The authors thank the three referees of this paper for valuable suggestions and useful comments.

Conflicts of Interest

The authors declare no conflict of interest.

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Figure 1. A sample of graph G.
Figure 1. A sample of graph G.
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Figure 2. A graph H with n = 3 .
Figure 2. A graph H with n = 3 .
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Figure 3. Examples.
Figure 3. Examples.
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Shao, Z.; Mojdeh, D.A.; Volkmann, L. Total Roman {3}-domination in Graphs. Symmetry 2020, 12, 268. https://doi.org/10.3390/sym12020268

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Shao Z, Mojdeh DA, Volkmann L. Total Roman {3}-domination in Graphs. Symmetry. 2020; 12(2):268. https://doi.org/10.3390/sym12020268

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Shao, Zehui, Doost Ali Mojdeh, and Lutz Volkmann. 2020. "Total Roman {3}-domination in Graphs" Symmetry 12, no. 2: 268. https://doi.org/10.3390/sym12020268

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