In situ formation of large pore silica–MnO2 nanocomposites with H+/H2O2 sensitivity for O2-elevated photodynamic therapy and potential MR imaging

2018 ◽  
Vol 54 (24) ◽  
pp. 2962-2965 ◽  
Author(s):  
Zhimei He ◽  
Yan Xiao ◽  
Jian-Rong Zhang ◽  
Penghui Zhang ◽  
Jun-Jie Zhu

Endogenous H+-/H2O2-triggered nanohybrids for cancer cell-specific and O2 self-sufficient PDT: a promising platform for effective PDT against tumor hypoxia.




2021 ◽  
Author(s):  
Yuanbo Wang ◽  
Shidang Xu ◽  
Leilei Shi ◽  
Cathleen Teh ◽  
Guobin Qi ◽  
...  


Biomaterials ◽  
2018 ◽  
Vol 181 ◽  
pp. 310-317 ◽  
Author(s):  
Hairong Wang ◽  
Yu Chao ◽  
Jingjing Liu ◽  
Wenwen Zhu ◽  
Guanglin Wang ◽  
...  


2021 ◽  
Vol 22 (19) ◽  
pp. 10506
Author(s):  
Dimakatso R. Mokoena ◽  
Blassan P. George ◽  
Heidi Abrahamse

Breast cancer is the second most common cancer globally and the pioneering cause of mortality among women. It usually begins from the ducts or lobules, referred to as ductal carcinoma in situ, or lobular carcinoma in situ. Age, mutations in Breast Cancer Gene 1 or 2 (BRCA1 or BRCA2) genes, and dense breast tissue are the highest risk factors. Current treatments are associated with various side effects, relapse, and a low quality of life. Although conventional treatments, such as surgery and chemotherapy, have been used for decades, their adverse side effects on normal cells and tissues pose a major weakness, which calls for a non-invasive treatment option. Photodynamic therapy (PDT) has proven to be a promising form of cancer therapy. It is less invasive, target-specific, and with reduced cytotoxicity to normal cells and tissues. It involves the use of a photosensitizer (PS) and light at a specific wavelength to produce reactive oxygen species. One of the reasons for the target specificity is associated with the dense vascularization of cancer tissues, which tends to increase the surface area for the PS uptake. Photosensitizers are light-sensitive molecules, which result in cancer cell destruction followed by light irradiation. Depending on the localization of the PS within the cancer cell, its destruction may be via apoptosis, necrosis, or autophagy. This review focuses on the breast cancer etiopathology and PDT-induced cell death mechanisms in breast cancer cells.



Nanoscale ◽  
2018 ◽  
Vol 10 (48) ◽  
pp. 22937-22945 ◽  
Author(s):  
Xiaoli Cai ◽  
Yanan Luo ◽  
Yang Song ◽  
Dong Liu ◽  
Hongye Yan ◽  
...  

A mitochondria-targeting and O2-evolving PDT nanoplatform based on 3D-dendritic MSNs was proposed for highly efficient cancer PDT treatment.



2019 ◽  
Vol 55 (98) ◽  
pp. 14785-14788 ◽  
Author(s):  
Xiaochun Hu ◽  
Yonglin Lu ◽  
Xiaoke Shi ◽  
Tianming Yao ◽  
Chunyan Dong ◽  
...  

A multi-functional nanoplatform (M-Pt-BCD) for combined chemo, photothermal and hypoxia-overcoming photodynamic therapy is described.



2020 ◽  
Vol 56 (96) ◽  
pp. 15208-15211
Author(s):  
Zhuolin Fu ◽  
Yingdi Wu ◽  
Chunnian Ren ◽  
Weiling Song ◽  
Xiaoru Zhang ◽  
...  

A novel multifunctional nanoprobe was designed for cancer cell targeted multilayer imaging of two cancer biomarkers. And in situ imaging of membrane MUC1 mucin and cytoplasmic microRNA miR-21 coupled with precise photodynamic therapy was achieved.



2019 ◽  
Vol 491 (4) ◽  
pp. 5595-5620 ◽  
Author(s):  
Sanson T S Poon ◽  
Richard P Nelson ◽  
Seth A Jacobson ◽  
Alessandro Morbidelli

ABSTRACT The NASA’s Kepler mission discovered ∼700 planets in multiplanet systems containing three or more transiting bodies, many of which are super-Earths and mini-Neptunes in compact configurations. Using N-body simulations, we examine the in situ, final stage assembly of multiplanet systems via the collisional accretion of protoplanets. Our initial conditions are constructed using a subset of the Kepler five-planet systems as templates. Two different prescriptions for treating planetary collisions are adopted. The simulations address numerous questions: Do the results depend on the accretion prescription?; do the resulting systems resemble the Kepler systems, and do they reproduce the observed distribution of planetary multiplicities when synthetically observed?; do collisions lead to significant modification of protoplanet compositions, or to stripping of gaseous envelopes?; do the eccentricity distributions agree with those inferred for the Kepler planets? We find that the accretion prescription is unimportant in determining the outcomes. The final planetary systems look broadly similar to the Kepler templates adopted, but the observed distributions of planetary multiplicities or eccentricities are not reproduced, because scattering does not excite the systems sufficiently. In addition, we find that ∼1 per cent of our final systems contain a co-orbital planet pair in horseshoe or tadpole orbits. Post-processing the collision outcomes suggests that they would not significantly change the ice fractions of initially ice-rich protoplanets, but significant stripping of gaseous envelopes appears likely. Hence, it may be difficult to reconcile the observation that many low-mass Kepler planets have H/He envelopes with an in situ formation scenario that involves giant impacts after dispersal of the gas disc.



2019 ◽  
Vol 31 (27) ◽  
pp. 1901893 ◽  
Author(s):  
Dongdong Wang ◽  
Huihui Wu ◽  
Wei Qi Lim ◽  
Soo Zeng Fiona Phua ◽  
Pengping Xu ◽  
...  


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