Romero FA, Razonable RR. Infections in liver transplant recipients. World J Hepatol 2011; 3(4): 83-92
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Raymund R Razonable, MD, Division of Infectious Diseases Marian Hall 5, Mayo Clinic, 200 First Street SW, Rochester, MN 55905, United States. firstname.lastname@example.org
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World J Hepatol. Apr 27, 2011; 3(4): 83-92 Published online Apr 27, 2011. doi: 10.4254/WJH.v3.i4.83
Infections in liver transplant recipients
Fabian A Romero, Raymund R Razonable
Fabian A Romero, Raymund R Razonable, Division of Infectious Diseases and the William J von Liebig Transplant Center, Mayo Clinic, Rochester, MN 55905, United States
Author contributions: Romero FA and Razonable RR contributed equally to this review.
Correspondence to: Raymund R Razonable, MD, Division of Infectious Diseases Marian Hall 5, Mayo Clinic, 200 First Street SW, Rochester, MN 55905, United States. email@example.com
Telephone: +1-507-2843747 Fax: +1-507-2557767
Received: October 20, 2010 Revised: December 6, 2010 Accepted: December 13, 2010 Published online: April 27, 2011
Liver transplantation is a standard life-saving procedure for the treatment of many end-stage liver diseases. The success of this procedure may be limited by infectious complications. In this article, we review the contemporary state of infectious complications during the post-operative period, with particular emphasis on those that occur most commonly during the first 6 mo after liver transplantation. Bacteria, and less commonly Candida infections, remain the predominant pathogens during the immediate post-operative period, especially during the first month, and infections caused by drug-resistant strains are emerging. Infections caused by cytomegalovirus and Aspergillus sp. present clinically during the “opportunistic” period characterized by intense immunosuppression. As newer potent immunosuppressive therapies with the major aim of reducing allograft rejection are developed, one potential adverse effect is an increase in certain infections. Hence, it is essential for liver transplant centers to have an effective approach to prevention that is based on predicted infection risk, local antimicrobial resistance patterns, and surveillance. A better understanding of the common and most important infectious complications is anticipated to lead to improvements in quality of life and survival of liver transplant recipients.
Citation: Romero FA, Razonable RR. Infections in liver transplant recipients. World J Hepatol 2011; 3(4): 83-92
Liver transplantation is a life-saving procedure for many end-stage liver diseases. According to the United Network for Organ Sharing (UNOS), a total of 6331 liver transplantations were performed in the United States during 2008-2009, with a survival rate of 85% at one year[1-3]. Survival after liver transplantation has improved over the years, partly due to advances in surgical techniques, and a reduction in allograft rejection. However, there remain multiple preventable conditions that contribute to the poor prognosis of liver transplant recipients. Understanding these complications may optimize management strategies, and further improve the quality of life, and survival rate of patients.
Despite measures such as the use of protective barriers, antimicrobial prophylaxis, and vaccination, infections still represent a major cause of morbidity and mortality after liver transplantation[1,2,4-13]. It is estimated that up to 80% of liver recipients will develop at least one infection during the first year after transplantation, and, while most are successfully treated, some will result in death. Indeed, opportunistic infections are a leading cause of death during the first three years after liver transplantation[4,9]. Often, the diagnosis of these infections is delayed because, as part of allograft-conserving strategies, immunosuppressive therapy diminishes inflammatory responses, and the clinical signs of infection may be blunted or absent, leading to delayed diagnosis and treatment.
There are three consecutive and often overlapping periods after liver transplantation that are associated with specific types of infections (Table 1). This article reviews the contemporary state of infections after liver transplantation, with special emphasis on bacterial infections (surgical site, intra-abdominal, and bloodstream infections) and selected viral [cytomegalovirus (CMV)] and fungal (Candida species and Aspergillus species) opportunistic pathogens.
Table 1 Selected infections after liver transplantation.
Time period after liver transplantation
Between 1st and 6th mo
Beyond 6th mo
General risks: surgical procedure, prolonged hospitalization, prior colonization, mechanical ventilation, indwelling vascular and urinary catheterization, donor-transmitted diseases, among others
General risks: over-immunosuppression, D+/R- mismatch status for viruses, allograft rejection, donor-transmitted diseases, repeated biliary tract manipulations, re-transplantation
General risks: variable
High-risk patients include those with recurrent rejection and allograft dysfunction that would require intense immunosuppression
Bacterial infections including resistant pathogens – bloodstream infections, pneumonia, surgical site infections, intra-abdominal infections, abscesses, urosepsis, Clostridium difficile associated colitis
Bacterial infections continue to occur in some patients – bloodstream infections, pneumonia, abdominal infections, C difficile associated colitis
Minimal immunosuppression – usual community acquired infections and zoster
Herpes simplex virus infection – herpes labialis or genitalis with potential for disseminated disease
Opportunistic pathogens: cytomegalovirus, Epstein-Barr virus, human herpesvirus 6 and 7, Aspergillus species, Pneumocystis jirovecii, Nocardia species, Mycobacterium tuberculosis, endemic mycoses, Toxoplasma gondii, among others
Intense immunosuppression due to allograft rejection and dysfunction – infections occurring during the opportunistic period (see middle column) continue to occur; course of chronic viral hepatitis may be accelerated
Bacterial pathogens are the most common causes of infection after liver transplantation. The highest incidence occurs during the first month after liver transplantation, and these infections predominantly involve the surgical site, the abdominal cavity, bloodstream, urinary system, and/or the respiratory tract[2,4,5,8,9,12,14,16-20]. Risk factors include biliary tract manipulation, prolonged hospitalization, and the necessity for surgical and other invasive procedures (Table 1)[14,16-18,21,22].
Virtually any bacteria can cause disease after liver transplantation, although the vast majority is caused by enterococcus, viridans streptococcus, Staphylococcus aureus, and members of the Enterobacteriaceae family[23-26]. There is an increasing trend towards antimicrobial resistance patterns among bacteria, although variations in prevalence rates among geographic regions and centers[23,26] have been found. In some centers, the prevalence rate of methicillin-resistant S. aureus (MRSA) colonization may exceed 80%[23,26], while vancomycin-resistant enterococcus (VRE) colonization may reach up to 55%. There have been reported outbreaks of infections due to extended-spectrum beta-lactamase (ESBL)-producing Klebsiella pneumonia or Escherichia coli and linezolid-resistant VRE. Risk factors for resistant bacterial pathogens are prior antibiotic use, recurrent hospitalizations, the use of invasive interventions such as mechanical ventilation and indwelling devices, and severe underlying diseases.
Surveillance for resistant bacteria (MRSA and VRE) in liver recipients may guide prevention strategies. Since MRSA colonization has been associated with risk of later infection[28-32], infection control strategies should be an integral component of liver transplant programs in order to reduce its incidence and transmission. With surveillance, cohorting, contact isolation, and nasal decolonization, the incidence of MRSA after liver transplant has been reduced[30,31]. MRSA decolonization is often achieved with the use of 2% intranasal mupirocin and chlorhexidine baths. The benefits of decolonization with oral antibiotics are debatable, due to concerns about further enhancing drug resistance. Active surveillance for VRE is also performed to prevent healthcare-associated transmission, however, there are no solid data to support antimicrobials to eradicate VRE carrier state.
Surgical site infections
One of the most common bacterial infections found to manifest itself early after liver transplantation, is surgical site infection, which has been estimated to occur in about 10% of patients. This is most often manifested as erythema, induration, tenderness, and drainage at the surgical site. In some cases, leukocytosis and fever may occur. Surgical site infection occurs more commonly in liver recipients who require a large number of blood transfusions, thus implying a more complex nature and prolonged duration of the surgical procedure. Notably, centers that perform fewer transplant procedures per year (e.g. < 50) have a higher rate of surgical site infections.
Surgical site infections are most commonly caused by Gram-positive cocci such as S. aureus and enterococcus, although Gram-negative pathogens like Escherichia coli, Acinetobacter baumannii, and Pseudomonas aeruginosa, and fungal pathogens such as Candida spp may be involved[1,9,14,22]. It is not uncommon for multiple pathogens to cause surgical site infections after liver transplantation, hence it is important to obtain samples for culture so that optimal therapy can be administered.
While surgical site infections are common causes of morbidity during the early period after liver transplantation, they may not be associated with a significant increase in overall mortality. Treatment of surgical site infections consists of a combination of surgical debridement and pathogen-directed antimicrobial therapy.
Intra-abdominal infections account for 27%-47% of early bacterial infections after liver transplantation[1,11,17,33]. Intra-abdominal abscesses, peritonitis, and cholangitis commonly present during the first few weeks after liver transplant as fever, leukocytosis, and abdominal pain, although clinically asymptomatic cases which are mainly manifested with elevated liver enzymes are not uncommon. The offending pathogens of intra-abdominal infections are often polymicrobial and, at present, often include multi-drug-resistant isolates. Some of the important bacteria causing intra-abdominal infections are enterococci, including VRE, S. aureus including MRSA, Candida species, and Gram-negative bacilli such as Pseudomonas sp., Klebsiella sp., Acinetobacter sp., and Enterobacter sp.[17,20].
Intra-abdominal infections are significantly associated with higher all-cause mortality (they double the risk), graft loss (39% vs 7%), and re-transplantation. Predisposing factors are Roux-en-Y choledochojejunostomy, hepatic artery thrombosis, or arterial stenosis. Once clinically suspected, the test to document the presence of fluid collections is radiographic imaging, either through CT scan or ultrasound. Treatment of infected collections consists of percutaneous or open surgical drainage combined with prolonged antimicrobial therapy, guided by susceptibility testing.
Bloodstream infections may occur any time after liver transplantation, although the majority occur during the first post-operative month. Clinical manifestations most often include fever and rigors, accompanied by leukocytosis and organ-specific or localizing symptoms related to the potential source of the bloodstream infection, such as erythema and drainage at vascular catheter sites (catheter-related blood stream infections), cough and dyspnea (pneumonia), and dysuria and suprapubic and flank pain (urosepsis). Risk factors include intra-abdominal infection, the need for re-operation, prolonged use of indwelling vascular catheters, and acute allograft rejection[5,21]. The gastrointestinal tract is usually the most common source of bloodstream infections in liver transplant recipients, and thus they are most commonly due to enterococcus, viridans streptococcus, Gram-negative bacilli, or may even be polymicrobial[5,35]. Other less common sources of bloodstream infection after liver transplantation include the urinary tract (urosepsis), pulmonary system (pneumonia), or infections emanating from infected indwelling vascular catheters. Interestingly, when compared to other solid organ transplant recipients, there is a higher incidence of mortality due to Gram-negative bloodstream infection among liver transplant recipients[5,35].
Bacteria causing bloodstream infection after liver transplant are predominately Gram-positive cocci such as enterococcus, viridans streptococcus and Staphylococcus sp., however, there has been an increasing trend towards Gram-negative bacteria, particularly when the source is the gastrointestinal tract[5,35,36].Today, there is an increasing prevalence of multi-drug resistant bacteria such as MRSA, which may be the cause of as much as 50% of bloodstream infections in some centers. Transplant candidates who are carriers of MRSA have a higher risk of bloodstream infection, and may thus benefit from decolonization prior to transplantation. Likewise, VRE-colonized transplant recipients have a higher risk of infection, postoperative stay in the intensive care unit, and death[37,38]. VRE colonization may also serve as an indicator of a more severe illness, an increased incidence of biliary complications, and multiple previous abdominal surgeries[37,38].
E. coli is the most common Gram-negative bacilli causing bloodstream infection after liver transplantation, followed by K. pneumoniae and P. aeruginosa. There is increasing resistance among these Gram-negative pathogens. The prevalence of ESBL-producing Gram-negative bacilli is now close to 13% in some centers[2,4,8,14], while 44% of E. coli isolates have developed resistance to quinolones, potentially due to common use of ciprofloxacin and norfloxacin as prophylaxis for spontaneous bacterial peritonitis, or levofloxacin as empiric therapy for community-acquired respiratory and urinary infections. Likewise, multidrug-resistant strains have been reported in as high as 62.5% of A. baumannii, 54.2% of Stenotrophomonas maltophilia, and 51.5% of Pseudomonas sp. isolates[19,21]. Outbreaks of carbapenem-resistant Klebsiella spp. bloodstream infections have occurred, with fatal outcomes.
Treatment of bloodstream infections should be directed towards the elimination of the predisposing factor, combined with pathogen-directed antimicrobial therapy that is guided by antimicrobial susceptibility testing. For persistent bloodstream infections, endocarditis should be evaluated by means of a transesophageal echocardiogram. Indwelling vascular and urinary catheters should be removed, intra-abdominal abscesses should be drained, and other potential nidus of infection should be surgically corrected, if feasible.
Liver recipients are somewhat unique among transplant recipients because they are commonly chronically infected with hepatitis B or C viruses, often with an accelerated clinical course. Respiratory and gastrointestinal viruses may occur throughout the post-liver transplant period, with seasonal variations for some viruses such as influenza and parainfluenza[41-43]. A list of selected viruses that affect liver transplant recipients is listed in Table 1. Among the opportunistic viral pathogens, the most commonly occurring are members of the herpes virus group[44-47], of which CMV is most important in terms of its direct and indirect impact on liver transplant outcome.
CMV seroprevalence rates in humans ranges from 45% to 100%[48,49]. Its ability to establish latency inside cells leads to a high infection rate in transplant recipients[50,51]. While immunocompetent hosts are usually infected without symptoms, liver recipients often present with more severe clinical presentation, including tissue invasion. Liver recipients at highest risk of CMV infection and disease are those who have never had CMV infection until they receive a latently infected organ from a CMV-seropositive donor (CMV D+/R- mismatch). The risk of progression into CMV disease is magnified by the intense immunosuppression required to avoid or to treat allograft rejection.
The clinical impact of CMV disease after liver transplantation can be classified into: (1) an acute infection with clinical signs known as direct effects (fever, mononucleosis, and invasive organ disease); and (2) a broad range of immunomodulatory and vascular effects, referred to as indirect effects. The most common presentation of CMV disease consists of fever and bone marrow suppression (CMV syndrome). A more aggressive form includes tissue invasion, commonly affecting the gastrointestinal tract, and presenting as gastritis or colitis. This is most often manifests itself as abdominal pain and diarrhea. Endoscopic findings include mucosal erosions and ulcerations, but mild hyperemia or even normal mucosa may also be present. A second clinical presentation that is fairly prevalent in liver recipients is CMV hepatitis, which usually presents with abnormal liver function tests in a cholestatic pattern. CMV hepatitis can be confirmed by means of biopsy, where inclusion bodies with clusters of polymorphonuclear cells is the hallmark[12,53]. A tissue sample is often necessary to rule out the alternative diagnosis of allograft rejection. Other organs such as the central nervous system and the lungs may be infected, and present themselves through headache, delirium, changes in mental function, and cough and dyspnea, respectively. Current practice relies on biologic markers (CMV pp65 antigenemia or CMV DNA by polymerase chain reaction) as the earliest indicators of infection[12,53].
It is proposed that the indirect effects of CMV result from its immunomodulatory property[54-58]. Excessive production of interleukin 10, which is an important inhibitor of the immune response, could potentially be one of the mechanisms for the higher incidence of bacteremia, fungal and other viral infections [human herpesvirus 6 (HHV-6), HHV-7, Ebstein-Barr virus (EBV) associated post-transplant lymphoproliferative disorder (PTLD), and accelerated HCV course] in CMV-infected individuals. Infection of vascular networks supplying the transplanted organ may cause functional impairment, leading to the loss of the allograft.
Because of its negative impact on overall outcome, prevention of CMV disease is a key management strategy after liver transplantation. One major strategy is antiviral prophylaxis, wherein antiviral drugs such as valganciclovir or oral ganciclovir are given to patients for at least 3 mo after liver transplantation. However, antiviral prophylaxis is associated with delayed-onset CMV disease, which typically occurs soon after completion of prophylaxis. Delayed onset CMV disease is significantly associated with increased mortality and graft failure after liver transplantation[59-61]. Risk factors for delayed onset CMV disease are CMV D+/R- mismatch status, acute allograft rejection, and the corresponding increase in immunosuppression, especially with anti-lymphocyte antibodies[59,62]. The second strategy for CMV disease prevention is pre-emptive therapy, which relies on a close virologic follow-up through serial blood markers (such as viral load or pp65 antigenemia) as the trigger for antiviral therapy, usually with intravenous ganciclovir or valganciclovir. A recent systematic review showed a low incidence (2.6%) of CMV disease in patients who had received pre-emptive valganciclovir therapy, and no case of delayed onset CMV disease was observed. Pre-emptive strategy, which allows short-term low level CMV replication, may prime the immune system to develop CMV-specific immunity, thus preventing late-occurring CMV disease. On the other hand, patients receiving universal prophylaxis had a higher incidence of late onset CMV disease (9.9% at one year). Nonetheless, systematic reviews and meta-analysis have demonstrated the similar reduction in CMV disease for both prophylaxis and pre-emptive therapy strategies, but all-cause mortality appears to be reduced by prophylaxis but not by pre-emptive therapy. There remains a concern for the rapidly replicating virus in CMV D+/R- transplant recipients, so that in this high-risk population, the recommendation is to use antiviral prophylaxis. For lower risk recipients (D+/R+ and D-/R+), universal prophylaxis or pre-emptive therapy regimens may be effectively used (Table 2).
Table 2 Suggested prevention and treatment regimens for various infections after liver transplantation.
According to risk factors (i.e. cephalosporins or vancomycin)
Susceptibility-guided antimicrobial treatment
Herpes simplex virus
Acyclovir 400 mg PO BID for 4 wk (if they are not receiving drugs for CMV prevention)
Acyclovir 5 mg/kg every 8 h for mucocutaneous disease or 10 mg/kg every 8 h for encephalitis
Valacyclovir 1 gram PO BID for less severe disease
Valganciclovir 900 mg daily for 3-6 mo
Valganciclovir PO 900 mg BID or ganciclovir IV 5 mg/kg BID.
Oral ganciclovir, 1 gram TID for 3-6 mo
If severe or life-threatening disease, initiate therapy with IV ganciclovir.
Preemptive therapy (guided by CMV PCR or antigenemia)
Treatment must continue until viral eradication is achieved, but not shorter than 2 wk
CMV Ig may be considered for severe forms of disease like pneumonitis.
Varicella zoster virus
Valacyclovir 1-gram PO TID or IV acyclovir 10 mg/kg every 8 h
Initiate with IV acyclovir for disseminated disease such as pneumonia or encephalitis
VZV immunoglobulin adds no additional benefits and not recommended
Fluconazole, echinocandin, or amphotericin B in high-risk recipients for 4 weeks
Amphotericin B 3 to 5 mg/kg IV daily
Fluconazole 800 mg loading dose, then 400 mg PO daily
Caspofungin at an initial dose of 70 mg followed by 50 mg daily
Anidulafungin initial dose of 200 mg first day followed by 100 mg daily
Voriconazole, echinocandin, or amphotericin B in high-risk patients
Voriconazole 6 mg/kg IV BID on day 1 followed by 4 mg/kg BID daily; transition to oral regimen when clinically stable
Echinocandins (caspofungin or anidulafungin)
Amphotericin B preparations
Amphotericin B (conventional or liposomal) and flucytosine (5-FC) for at least 2 wk then fluconazole as long-term maintenance (e.g. 6 mo)
Fluconazole 800 mg loading dose, then 400 mg PO daily for limited disease
TMP- SMX 160/800 mg daily or three times per week
TMP- SMX preferred; 15-20 mg/kg per day of TMP component in 3-4 divided doses (keep the sulfa level above 100); transition to oral regimen when clinically stable
Alternative: TMP-SMX 80/400 mg daily
Alternatives: Pentamidine isethionate, trimethoprim-dapsone (in patients who are not deficient in glucose-6-phosphate dehydrogenase), atovaquone, and clindamycin-primaquine.
TMP- SMX 160/800 mg daily
Pyrimethamine in combination with sulfadiazine or clindamycin.
Not recommended but TMP- SMX for Pneumocystis prophylaxis may prevent some infections
Ampicillin 2 g IV every four hours plus Gentamicin 3 mg/kg per day IV in three divided doses
TMP- SMX 10-20 mg/kg IV per day divided every 6 to 12 h
Meropenem 2 g IV every eight hours
Not recommended but TMP- SMX for Pneumocystis prophylaxis may prevent some infections
TMP-SMX preferred; 8-10 mg/kg per day of TMP component in 2-4 divided doses; higher doses may be used in severe disease; transition to oral therapy when clinically stable
Treatment of CMV disease is with intravenous ganciclovir (5 mg/kg every 12 h) or oral valganciclovir (900 mg orally twice daily) (Table 2), combined with reduction in immunosuppression. Severe cases warrant the initial use of intravenous ganciclovir, while treatment of mild to moderate cases may be initiated upfront with oral valganciclovir. For severe cases, the addition of CMV-hyperimmune globulin as adjunct treatment may be considered. The efficacy of treatment should be guided by clinical and virologic assessments, often with serial weekly monitoring of viral load or antigenemia levels. The vast majority of CMV disease cases after liver transplantation, even those occurring at delayed onset, remain susceptible to ganciclovir. Non-responders should be tested for drug-resistant virus, with UL97 and UL54 gene sequencing. Therapy for drug-resistant CMV is tailored, based on the results of genotyping. Foscarnet and cidofovir are often used for treatment of ganciclovir-resistant UL97-mutant CMV strains, but they have a high risk of nephrotoxicity.
Although various fungal species infect liver transplant recipients, by far the most common are the Candida species followed by the Aspergillus species. Cryptococcus neoformans occurs much less commonly in the form of meningitis, lung disease and cellulitis. Endemic mycoses due to Histoplasma capsulatum, Coccidiodes immitis, and Blastomyces dermatitidis may occur in liver recipients from endemic regions, and among these, C. immitis often persist and require prolonged therapy. Other less common fungi that may cause skin disease could potentially become invasive in liver transplant recipients, include Alternaria species, Sporothrix schenckii, Trichophyton rubrum, among others. Finally, infection due to Pneumocystis jirovecii occurs primarily as diffuse bilateral pneumonitis, although the use of trimethoprim sulfamethoxazole prophylaxis has remarkably reduced its incidence after liver transplantation.
Candida sp. accounts for over half of all invasive fungal infections in liver recipients. Superficial and invasive candidiasis occurs early and often during the first 1-3 mo after liver transplantation. Candida albicans is the single most common species, but collectively the non-albicans Candida species are now being reported more frequently from blood cultures. The distribution of the species varies among reports, including C. glabrata, C. parapsilosis, C. tropicalis, C. kefyr, C. guilliermondii and C. krusei[2,5,7,10,71-75]. This has implications in empiric antifungal treatment, since some of these isolates, particularly C. glabrata and C. krusei, are inherently resistant to fluconazole. The most common clinical presentation is mucosal candidiasis (e.g. oral thrush), but the much more worrisome illness, because of its impact on morbidity and mortality, is invasive candidiasis[70-76]. Invasive candidiasis is defined as the (1) direct microscopic evidence of the candida in a specimen obtained from a normally sterile site; (2) recovery of candida by culture of a sample obtained from a normally sterile site in a suspicious clinical setting; or (3) recovery of Candida species in one or more blood cultures (candidemia). Disseminated candidiasis is defined as an episode of candidemia with associated target-like abscesses in the liver or the spleen, or the presence of progressive retinal exudates on ophthalmologic examination.
The incidence of candidemia among transplant recipients ranges between 2%-8%[2,75], and the overall mortality associated with invasive fungal presentation has been reported to be as high as 77%. Invasive candidiasis could be primary or secondary to infected catheters or surgical wounds. Dissemination to involve distant sites such as the eyes and the bone may occur, and should warrant evaluation in the presence of clinical symptoms such as blurring of vision and bone pains, respectively. Surgical site infection, peritonitis, liver and abdominal abscesses, endophthalmitis, esophagitis, and urinary tract or anastomotic infections are the other clinical presentations of candidiasis[70,76].
Risk factors for invasive candidiasis are often related to the surgical procedure (such as prolonged or repeat operations and re-transplantation), high-transfusion requirement, previous Candida specie colonization during the perioperative period, and renal failure after liver transplantation (Table 3)[7,70,72,76,78]. Choleducho-jejunostomy anastomosis is especially associated with a higher risk of candidiasis when compared to choledoco-choledocho anastomosis.
Table 3 Risk factors of fungal infections after liver transplantation.
Renal insufficiency (creatinine > 3.0 mg/dL)
Renal replacement therapy within the first 30 days after transplant
Need for dialysis
Prolonged transplant operation time (> 11 h)
Second surgical intervention for any reason within 5 d of the initial transplant procedure
Transfusion of ≥ 40 units of blood products during the surgery
Fulminant hepatic failure
Early fungal colonization (within 3 d after liver transplantation)
Documented colonization (nasal, pharyngeal or rectal cultures)
Fulminant hepatic failure
The American Society of Transplantation recommends antifungal prophylaxis against Candida to high-risk liver recipients[70,76]. However, the duration of prophylaxis is not defined, with many centers providing it for 4 weeks. Echinocandins, azoles, and amphotericin B are the various options for antifungal prophylaxis. Clinical studies have shown that fluconazole, itraconazole, or amphotericin B prophylaxis markedly reduced the incidence of invasive candidiasis in liver recipients[79-81]. Caspofungin also appears to be well tolerated and has been shown to result in a low rate of invasive fungal infection[78,82]. However, a meta-analysis showed that, while antifungal prophylaxis in liver recipients significantly reduced the incidence of superficial and invasive fungal infection, it neither impacted on the overall mortality nor the need for empirical antifungal treatment. Antifungal prophylaxis is not recommended for low-risk patients due to concerns for toxicity, and may select for resistant strains[78,84].
Treatment of invasive candidiasis after liver transplantation is often a combination of antifungal therapy, elimination of nidus of infection, and reduction of immunosuppression. Empiric treatment of invasive candidiasis consists of the use of a broad-spectrum antifungal agent (such as caspofungin, micafungin and anidulafungin) in view of the increasing incidence of fluconazole-resistant strains due to non-albicans Candida species. Once the species and its antifungal susceptibility pattern have been confirmed, a more focused treatment should be used. The vast majority of C. albicans remains susceptible to fluconazole and that should be the treatment of choice. The shift from C. albicans to non-albicans species in many clinical settings has most likely resulted from the widespread use of fluconazole prophylaxis. Fluconazole resistance in invasive candidiasis should be suspected in patients who have received fluconazole during the 30 d prior to the illness. Abscesses and infected wounds need to be drained and debrided, while infected indwelling vascular and urinary catheters need to be removed. Potential sites of dissemination such as the eye (candidal retinitis and endophthalmitis) and the bones (osteomyelitis) should be examined.
After Candida sp., this highly aerobic mold is the second most common fungal infection in liver recipients, with invasive aspergillosis occurring in 1%-9.2%. The risk factors are listed in Table 3[86,87]. Among the most notable risk factors are re-transplantation, which could bring about a 30-fold higher risk, and renal failure, especially with the requirement for renal replacement therapy, which could bring about a 15-25 fold increase in risk. Other risk factors that have been described are fulminant hepatic failure, CMV disease, and prolonged ICU stay. Mortality from invasive aspergillosis is high among liver recipients, so that treatment needs to be started early and aggressively.
Aspergillus fumigatus is the most common offending species, whereas A. niger, A. flavus and A. terreus are less common. In a recent study of the clinical features of invasive aspergillosis from 23 US transplant centers, the most common clinical presentation (90%) was lung infection. Most infections occur during the first year, with a median time to diagnosis of 100 d. Other studies have described an earlier onset of invasive aspergillosis, such as within 30 d after liver transplantation, although others report a much more delayed onset of infection. Notably, liver recipients with invasive fungal infection had the highest mortality reported, perhaps as result of the severity of the illness and the patient’s underlying compromised status[13,88].
The possibility of invasive aspergillosis should be suspected in the presence of risk factors and suspicious clinical findings, and should be confirmed by one of the following: (1) lower respiratory tract infection symptoms, with associated risk factors and CT images showing well-circumscribed lesions with or without the halo sign, air-crescent sign or a cavity; (2) central nervous system infection with focal lesions on imaging or (3) recovery by culture of the mold. Since sensitivity of fungal cultures is relatively low, it has been suggested that measuring aspergillus antigens such as galactomannan in clinical samples such as plasma, serum, bronchoalveolar lavage fluid, or CSF could be useful for diagnosis. Special caution, however, is suggested in interpreting the galactomannan test in patients who are receiving β-lactam antibiotics (specifically piperacillin tazobactam and ampicillin) which cross-react with the assay, thereby providing false positive results[89,90]. These antimicrobials are semisynthetic derivatives from Penicillium species that contain galactofuran-bearing molecules, which react with the assay[91,92].
Antifungal prophylaxis against Aspergillus sp. could result in an important reduction in superficial and invasive infection, as well as mortality attributable to fungal infections. However, antifungal prophylaxis does not reduce overall mortality or the need for empirical antifungal therapy. The overall efficacy of universal antifungal prophylaxis is limited by the generally low incidence of invasive aspergillosis. Hence, providing prophylaxis only to the high-risk patients would seem to be a more rational approach. The American Society of Transplantation recommends the use of a lipid formulation of amphotericin B (3-5 mg/kg per day) or an echinocandin for liver recipients with factors that place them at high risk; the duration of antifungal prophylaxis is during the initial hospital stay or for 4 wk after liver transplantation.
Prompt diagnosis and initiation of antifungal therapy, coupled with a reduction in the immunosuppressive regimen is essential for achieving optimal outcomes with invasive aspergillosis after liver transplantation. The current guideline endorses voriconazole as the first-line choice for the treatment of invasive aspergillosis (Table 2). Antifungal therapy with amphotericin B preparations is now considered as second line therapy. Echinocandins are effective for treatment, but they have been tested mainly as salvage therapy for invasive aspergillosis. Of the echinocandins, caspofungin is currently approved by the US FDA for the treatment of invasive aspergillosis. Combination antifungal therapy has been reported in certain situations (such as severe disseminated disease), but the efficacy of this approach remains controversial. The Infectious Disease Society of America reserves the option of combination antifungal regimens as salvage therapy for non-responsive cases of invasive aspergillosis[85,88]. Surgical excision or debridement remains an integral part of the management of invasive aspergillosis. The optimal duration of therapy depends on the response to therapy, and the patient’s underlying immune function. Generally, treatment is continued for at least 12 wk, although it should be individualized, based on clinical response.
Infectious complications remain important preventable causes of morbidity and mortality among liver recipients. The vast majority of infections that occur during the immediate period after liver transplantation are often related either to surgical procedures, medical devices, or the need for prolonged hospitalization. During the highly intense period of immunosuppression, the most common opportunistic infections are cytomegalovirus and invasive fungal infections (candidiasis and less commonly aspergillosis). It is therefore essential to have in place an effective approach to prevention, based on predicted infection risk, local antimicrobial resistance patterns, and surveillance of specific risk factors. A better understanding of the common and important infectious complications is anticipated to improve quality of life and survival rate after liver transplantation.
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